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Colloquium

OSIRIS-REx: Sample science and the geologic context for the return regolith from active asteroid Bennu

Date
2021-08-04
Speaker
Prof. Harold C. Connolly Jr
Venue
ONLINE

Abstract

The OSIRIS-REx space mission is part of NASA's New Frontiers program and has a main goal of returning at least 60 g of pristine regolith from asteroid Bennu. On May 10th of this year, the spacecraft successfully performed a departure maneuver and left the vicinity of the Target asteroid, having achieved all of its science and engineering goals flawlessly, including the collection of regolith from asteroid Bennu. This talk will review the mission, the major findings of the mission as they pertain to sample science, discussion how our finding may illuminate the origins and evolution of the collected regolith. It will review the OSIRIS-REx collection and stowing (or the sample) process, what we know about the collected sample, and review some basic aspects of how the team will analyze and curate the sample when it returns.

Paleobiogeographic and biostratigraphic evidences for role of Ocean gateways in changing ocean circulation and global climate during Cenozoic"

Date
2021-03-24
Speaker
Prof. Devesh K Sinha
Venue
Online

Abstract

Ocean circulation plays a vital role in modulating the world’s climate. Surface currents moving from low to high latitudes deliver immense heat to the colder region and moderate the climate. One of the best examples is Gulf Stream which is considered to save North America and Europe from the extremely cold climate. The thermohaline circulation translates itself into the great ocean conveyor belt, which connects the world oceans through the surface and deep currents. The cold oceans are also a huge sink for the atmospheric carbon dioxide, while the warm oceans are the sources. The surface ocean circulation is largely controlled by the ocean-continent geometry, which has been changing through geological time. The changes have resulted in the opening and closing of major ocean gateways causing major climatic events, including the formation of the permanent ice cap on Antarctica, Northern Hemisphere Glaciation and East African aridification. During Cenozoic, the plate movements caused the opening of the Drake Passage and Tasman gateway, which resulted in the establishment of the Antarctic Circum Polar Current, a major cause for the development of ice sheets in Antarctica. The deepening of the Greenland-Scotland Ridge in the North Atlantic allowed the establishment of the North Component Deep Water and Atlantic Meridional Ocean Circulation (AMOC). The closing of the Indonesian Seaway resulted in East African aridification in the Early Pliocene, while during Late Pliocene, the closing of the Central American Seaway is attributed to enhance the northern hemisphere glaciation. Foraminiferal biogeographic and biostratigraphic studies have been very instrumental in understanding the opening and closing of the ocean gateways during the Cenozoic and their impact on palaeoceanography and paleoclimatic changes.

"Electrons in Complex Materials: from Theory to Practice”

Date
2021-03-17
Speaker
Prof. Tanusri Saha-Dasgupta
Venue
ONLINE

Abstract

The electrical, magnetic, and optical properties of materials are controlled by their composition and structure. The structure, and also the strength of materials are determined by the chemical bonding between the atoms. At the root of all of these, the physical as well as the chemical properties, are the electrons. In this talk, we will demonstrate, how electronic structure calculations can be employed to modeling of complex materials and to gain insights to complicated physical and chemical processes happening in a complex material. Examples will be drawn from diverse areas e.g. high Tc cuprates, magneto-electric double perovskites, quantum spin compounds, metal-organics.

"Coherence, Chaos and Turbulence in Plasmas"

Date
2021-03-03
Speaker
Prof. Bimla Buti
Venue
ONLINE

Abstract

Plasma science provides one of the cornerstones of our knowledge of the Sun, the stars, the interstellar medium etc. Although it is often not readily apparent, plasma science is relevant to our society in a variety of ways. Plasma science is central to the development of nuclear fusion as a clean, renewable energy source. Coherent laser-plasma radiation sources have a variety of potential applications in medicine and industry. The role of Coherent, Chaotic and Turbulent processes in plasmas will be reviewed in this presentation. A brief description of Chaos and Fractals vis-à-vis Artificial Intelligence will also be presented.

"Radiation Dosimetry and Radiation Protection in Space Missions"

Date
2021-02-03
Speaker
Dr. Bhaskar Mukherjee
Venue
ONLINE

Abstract

Outer space is continuously bombarded by energetic particles of galactic origin as well as protons of a wide energy distribution resulting from coronal mass ejection from the Sun designated as galactic cosmic rays (GCR), and solar particle events (SPE), respectively. Astronauts in space missions are directly exposed to GCR and SPE radiations. On the other hand, pilots and aircrew during long haul intercontinental flights and human population living in high-altitude mountainous regions are exposed to secondary radiations originated from cosmic ray shower (CRS) in the upper atmosphere. Using widely available Lithium Fluoride (LiF) and Beryllium Oxide (BeO) thermoluminescent dosimeter (TLD) chips a novel radiation dosimeter emulating “Mammalian Tissue-Equivalence” the LiBe-Micro Dosimeter was developed. The R&D pathway of LiBe-Micro-Dosimeter and important results including radiation dosimetry, risk assessment and radiation protection issues of astronauts resulting from space missions will be presented.

"Design Thinking and Innovation"

Date
2021-01-27
Speaker
Prof. Praveen Nahar
Venue
ONLINE

Abstract

Many organizations attempt to solve one problem but realize that it is interconnected with many other issues and challenges. Various stakeholders may have different needs or concerns, and it is not easy to make sense of them all. Design thinking (or designerly way of thinking) is an iterative framework that is used to understand the need, context, users, challenge assumptions, redefine problems and create innovative solutions to prototype and test, it is very useful in the situations where the problems which are ambiguous, unknown, and not so well defined.The presentation focuses on design, design thinking & innovation, its characteristics, skill sets, mindsets, and process framework with some case studies from Product Design and allied fields. It will also touch upon its possible contribution to scientific research in strategic planning processes and unknown territories.

"Weather Forecasting in India : Current status and future plan"

Date
2021-01-20
Speaker
Dr. Mrutyunjay Mohapatra
Venue
ONLINE

Abstract

Most of these natural disasters (about 80%) are hydro-meteorological in nature. They include cyclones, floods, droughts, landslides, heat wave, cold wave, thunderstorms, and tornadoes. The risk management of these natural disasters includes several steps based on its severity and impact: (i) hazard analysis, (ii) vulnerability analysis, (iii) preparedness and planning, (iv) early warning, (v) prevention and mitigation. The early warning component includes: (i) skill in monitoring and prediction of natural hazards, (ii) effective generation and dissemination of products for warning, (iii) coordination with emergency response units, and (iv) public awareness and perception about the credibility of the official predictions and warnings. Though there have been significant improvement in multi-hazard monitoring and warning system in recent years due to various initiatives of Ministry of Earth Sciences (MoES) / India Meteorological Department (IMD) and policy frame work of Government of India, there is still scope for improving (i) mesoscale hazard detection and monitoring, (ii) spatial and temporal scale of forecasts through technological upgradation, (iii) impact based forecast and sectoral applications, (iv) warning communication to last mile. All these aspects will be discussed with respect to current status, existing gap areas, and future scope.

"Variability of Monsoons at Different Scales"

Date
2021-01-06
Speaker
Prof. Ravi Shankar Nanjundiah
Venue
ONLINE

Abstract

The Indian Summer Monsoon governs the pulse of this country. It is known to vary at various scales. In this talk, we will discuss the mean monsoon and its variability at various scales ranging from within the season at extremely short scales (<10 days) commonly known as the synoptic scale, the intraseasonal variability (10-60 days), and from season-to-season (commonly known as interannual variability). In addition, we will briefly discuss some global phenomena that modulate the strength of monsoon, such as the El-Nino. We will also examine if this El-Nino and Monsoon linkage fluctuates with time. Additionally, we will also examine if the strength of intraseasonal variability also fluctuates and whether anthropogenic factors also affect it. Finally, we will also examine if the monsoon has fluctuations from decade-to-decade and factors that could cause this decadal variability.

Internal Bores in the Mesosphere: A manifestation of Atmospheric Gravity Waves”

Date
2020-12-23
Speaker
Prof. S. Gurubaran
Venue
ONLINE

Abstract

A plethora of wave phenomena occurs in the Earth’s atmosphere encompassing a multitude of spatial and temporal scales. Among their several manifestations in the upper layers of the atmosphere, a well-marked dynamical feature is the internal bore. A spectacular wave feature in the heights between 85 and 100 km involving an altitude dependent bright or dark wavefront followed by phase-locked crests and troughs was first reported by Mike Taylor and his coworkers in 1995 through all-sky airglow imaging observations that was later interpreted as a mesospheric bore. Since then, a number of ground and space-based investigations of this intriguing wave dynamical feature have been reported. We have analogs for the mesospheric bores in other atmospheric regions like the morning glory and tropospheric bores and also in channel bores that have been explained by the hydraulic jump theory. The mesospheric bores are occasionally observed in airglow emissions as a steep front followed by undulations or a turbulent regime behind. These bores have their origin in stable atmospheric layers characterized by temperature inversion (thermal duct) or favourable wind systems (Doppler duct). Atmospheric gravity waves propagating through those ducts can undergo amplitude steepening, resulting in bores with phase-locked crests and troughs behind (undular bore). The damping of waves behind the fronts can lead to turbulence (turbulent bore) on certain occasions. Bore-like fronts are also seen in noctilucent clouds at high altitudes. This talk will introduce this exciting subject of internal bores in the mesosphere and present some of the fascinating observational results obtained from different platforms in the recent past. The challenges in understanding the mechanisms underlying this phenomenon essentially lie in the sparsity of observational knowledge about the environmental or the background atmospheric parameters. This talk will highlight those challenges as well.

“Long term study of the Sun using the Kodaikanal Digitised archive.”

Date
2020-12-16
Speaker
Prof. Dipankar Banerjee
Venue
ONLINE

Abstract

Solar observations at the Kodaikanal observatory over the last 100+ years provide one of the longest continuous series of solar data. Apart from that, simultaneous observations in different wavelengths make this data a unique one and suitable for multi-wavelength studies. The Kodaikanal observatory has been obtaining solar images since 1904 in broadband white light, narrow band Ca II K 393.37 nm, and H-alpha 656.3 nm wavelengths. Many of these observations are still continuing. The historical data which were on photographic plates has been digitized. The study of the long-term variation of the sun is very important to understand the future of the solar activity. The solar variation affects our climate and near-earth environment. This database is also useful for theoretical modelling of the periodic generation and variation of the large-scale solar magnetic field. The preservation and distribution of such data sources through the datacenter hosted at IIA, Bangalore to the global scientific community have initiated a new platform for innovative and best practices for the dissemination of these historical and heritage resources. This presentation will demonstrate how this data archive is producing new science results. A comparison with other similar and major global archives will also be presented.

“Beyond Penrose - Blackholes and Spacetime Singularities”

Date
2020-12-09
Speaker
Prof. Pankaj Joshi
Venue
Onine

Abstract

Exciting developments have taken place in recent times in blackhole physics and gravitation theory. The recent observations on gravitational waves and imaging the compact object at galactic centers have given many new insights into the nature of Einstein theory of gravity. Spacetime singularities have been a central feature driving many of these breakthroughs, which are extreme compact regions in cosmos where all physical quantities such as matter densities, curvatures and others are arbitrarily high and the gravitational force is at its extreme. We discuss here these entities, namely singularities and blackholes, the work that was given the physics Nobel this year. We show how general relativity indicates that spacetime singularities are inevitable consequence when massive stars collapse on exhausting their internal nuclear fuel. The key open question today at the frontier of fundamental physics is, whether such singularities are visible to faraway observers in the universe, or they would be always hidden within blackholes. We review recent developments here, including our own work, which have far-reaching observational and theoretical implications on our basic understanding of the universe, including future quantum gravity theories.

"Role of waves and small-scale transients in the coronal heating"

Date
2020-11-25
Speaker
Dr. Girjesh R. Gupta
Venue
Online

Abstract

ABSTRACT The tenuous outer atmosphere of the Sun, commonly known as ‘corona', is orders of magnitude hotter (> 1 MK) than the solar surface (< 6000 K). The heating of coronal plasma remains one of the most puzzling problems in astrophysics. Magnetohydrodynamic (MHD) waves and small-scale transients are proposed to provide sufficient energy to maintain the hot corona. In this talk, observations of wave propagation and small-scale transients in the solar atmosphere, and their contribution to coronal plasma heating will be presented.

"New insights into the formation of massive stars."

Date
2020-11-18
Speaker
Dr. Lokesh Kumar Dewangan
Venue
Online

Abstract

Massive stars are astronomical objects having masses greater than 8 Msun, which is the threshold necessary for a star to evolve into a supernova. The physical process concerning the birth of massive stars (> 8 Msun) is one of the outstanding problems in astrophysics since they are extremely influential in the evolution of galaxies through their energetics. It is still unclear whether the formation mechanism of a massive star is a scaled-up version that produces low-mass stars like our Sun or if it is a fundamentally different process. In recent years, two large-scale theories are the points of interest because of their growing evidence for the formation of massive stars: (1) collision between molecular clouds, and (2) accretion through parsec-scale filaments. However, investigations of observational signatures of these processes is very challenging. In this colloquium, I will present some important observational findings, which provide new insights into the formation of massive stars.

"Precision @ LHC"

Date
2020-11-11
Speaker
Dr. Satyajit Seth
Venue
Online

Abstract

Precision calculation in the context of the Large Hadron Collider (LHC) is indispensable to understand and describe its experimental outcomes. To confirm a discovery and to reject a prediction or to put stringent bounds on it, such calculation plays an important role. In this colloquium, the nitty-gritty of such theoretical input - its utility and impact will be described.

"Space weather: From anomaly to insights"

Date
2020-11-04
Speaker
Dr. Dibyendu Chakrabarty
Venue
Online

Abstract

Space weather can have different meanings depending on the vantage point in space. In a magnetized planet like ours, which is located in a stellar neighbourhood, space weather is primarily controlled by solar disturbances. Radiation, particles in the solar wind, and the “frozen-in” magnetic field popularly known as the interplanetary magnetic field (IMF) carries the solar disturbances to the magnetic cavity of the Earth known as the magnetosphere. The way IMF affects the magnetosphere or the ionosphere depends greatly on the polarity of the IMF. It is known that the southward component of the IMF (IMF Bz) is the most relevant parameter for the northward directed terrestrial magnetic field. The interaction between oppositely directed magnetic fields leads to enhancements in currents and electric fields in the magnetosphere resulting into what is known as a geomagnetic storm. Till date, the disturbances in the ionospheric electric field and currents during geomagnetic storms have been addressed mostly based on the variations in the IMF Bz. However, in recent times, a number of works carried out at PRL have revealed that the ionospheric disturbances in the electric fields and currents can be “anomalous” on many occasions and cannot be explained by taking only the IMF Bz into account. The roles of magnetospheric substorms, solar wind density, and the east-west component of the IMF (IMF By) have been found to be equally important to understand the space weather impacts in a critical manner. In this colloquium, a few such results will be highlighted to show that the so-called “anomalous” observations can truly lead to insights into the understanding of space weather.

Electron and positron scattering from molecules

Date
2020-10-28
Speaker
Prof. Bobby K Antony
Venue
Online

Abstract

The study of leptonic collisions with matter is central to understanding many natural phenomena and to the development of many technologies of the 21st century. Furthermore, the fundamental quantum nature of such interactions is such that they are a primary example of modern physics. Despite more than a century since the first quantified experimental study of electron interactions with atoms (The Franck Hertz experiment of 1914) and the first applications of quantum mechanics to model such interactions, our knowledge of the dynamics of such collisions remains incomplete. The increasing recognition of the central role of electron collisions with molecular systems in determining chemical pathways has led to a renaissance in electron – matter interactions with ‘electron induced chemistry’ now being prevalent in industrial (e.g. development of next generation nanolithography) and clinical (next generation radiotherapy) applications. Whilst the role of electron induced physio-chemical processing is now recognized to be dominant in astrophysics/astrochemistry and from Star formation to planetary atmospheres. Simultaneously our ability to produce high fluxes of positrons has allowed anti-matter to be adopted as a scientific tool, for example, the now commonly deployed Positron Emission Tomography (PET) in the clinic. Positrons are also now widely used in material science. Besides, their role in astrophysics is important in understanding our early universe. However, detailed understanding of positron scattering from atoms and molecules is a difficult task for both theory and experiment due to various known reasons. For example, the formation of positronium (Ps) makes it even more challenging. Our group at IIT (ISM) has developed theoretical methods to study various processes of electron and positron scattering and have predicted cross section for many atoms and molecules.

Search for Symbiotic Systems: The ASTROSAT Revelation

Date
2020-10-21
Speaker
Dr. Mudit Srivastava
Venue
Online

Abstract

Symbiotic stars are the interacting binary systems that typically consist of a hot compact white dwarf and a cool giant star. The interaction between a very hot white dwarf and a very cool red giant causes phenomena which are unique to such systems and make the Symbiotic system of stars a unique astrophysical laboratory. Being one of the most intriguing astrophysical objects, they have been studied for decades. Nevertheless, there are properties of these systems which have not been understood properly. The symbiotic phenomenon is powered by the hot components of this system viz. white dwarf and accretion disk. Emissions from these two peak in the UV range and hence cannot be probed with traditional ground-based observations. In recent times, space-based observations have thrown additional light on the properties of symbiotic systems. In particular, an ordinary red giant “SU Lyn“ was discovered in X-rays which raised suspicion that it may harbour a hidden white dwarf, thereby making it a promising candidate of a new hitherto unknown class of symbiotic system. We, at PRL, have probed SU Lyn using Ultra-Violet Imaging Telescope (UVIT) aboard ASTROSAT satellite mission in addition to its ground-based optical-NIR spectroscopy. Utilizing a lesser-known spectroscopy capability of UVIT, we have successfully confirmed the symbiotic nature of the SU Lyn. The confirmation of SU Lyn as a new class of Symbiotics has opened up an incognito window to discover and study more objects of this kind. It also carries a great significance in order to solve the puzzle of a very small number of known Symbiotics, given the fact that the known population of Symbiotics are nearly a factor of thousand less than the predicted ones. To the best of our knowledge, this is the first study that utilizes the UV spectroscopy capability of UVIT/ASTROSAT in its five years of operations.

Discovery of Recent Volcanism on the Moon

Date
2020-10-07
Speaker
Dr. Neeraj Srivastava
Venue
Online

Abstract

Our knowledge about the geology of the Moon, our nearest celestial neighbor, has undergone a paradigm shift during the past decade in the wake of discoveries made from the analysis of data received from a string of remote sensing missions, such as Chandrayaan-1 (ISRO), Kaguya (JAXA), Lunar Reconnaissance Orbiter (NASA), GRAIL (NASA), and Chang'e (CNSA). One such finding relates to the current geological state of the Moon. For long, the Moon was unanimously considered to be geologically dead with no signs of volcanism during the past ~1.2 Ga. We have found tangible shreds of evidence of volcanic activities on the Moon, that occurred ~700 Ma ago in the Grimaldi Basin on the Near Side, and also as recent as 2-10 Ma before present inside the Lowell Crater, Orientale Basin on the Far Side. Besides these, evidence of recent tectonism has also been found in these areas. These findings have significant implications for our understanding of the thermal evolution of the Moon. Excerpts from some of these studies will be presented during the talk.

"Collaboratively Searching for Something that Might Not Exist: Life on Mars?"

Date
2020-03-11
Speaker
Prof. Dawn Sumner
Venue
K R Ramanathan Auditorium, PRL main campus

Abstract

Prof. Dawn Sumner's research focuses on reconstructing ancient environments on early Earth and Mars and the early evolution of bacteria, including the origin of oxygenic photosynthesis. Her group studies everything from the environmental settings, geochemistry, and morphology of Archean microbialites to the morphology, climate response, and genomics of modern microbial communities growing in ice-covered Antarctic lakes to the stratigraphy and geochemistry of sedimentary rocks on Mars. Prof. Sumner is a member of NASA's Mars Science Laboratory (MSL), helping the rover Curiosity explore ancient environments in Gale Crater on Mars. She regularly shares her research and adventures with the public. Sumner is dedicated to helping students of all backgrounds prepare for careers in science as well as to creating educational and work environments that are inclusive and supportive, including through the use of feminist research and theory. Prof. Sumner was awarded the Career Award for Outstanding Contributions in Geosciences, Geobiology, and Microbiology from the Geological Society of America in 2016. She is an elected Fellow of the Geological Society of America (in 2014). She was also selected to deliver the honorary Carl Sagan Lecture at the American Geophysical Union (AGU). She had been the Chair of the UC Davis Department of Earth & Planetary Sciences from 2014-2016. She had also been the Chancellor's Fellow, UC Davis, during 2003-2004.

“Retracing Saraswati: the lost river of the Harappan Civilization.”

Date
2019-12-11
Speaker
Prof. Jyotiranjan S. Ray
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

The most celebrated river of Indian mythology, the Saraswati, has often been hypothesized to be the river of the Bronze Age Harappan civilization in north-western India. The suspected modern counterpart of the glacier-fed Saraswati is the river Ghaggar, which unlike the former is a seasonal stream that originates in the Himalayan foot-hills. Despite the discovery of a large number of settlements along the Ghaggar, many believed that the Harappans depended solely on monsoonal rains, because no proof existed for the river’s uninterrupted flow during the peak of the civilization. This had led many to reject the very idea of the river Saraswati and its hypothesized relationship with the Harappan culture. To resolve the issues related to the existence of the river Saraswati and its drainage area, we investigated the nature of the ancient Ghaggar during the last several thousand years by studying the changes in the sources of the sediments deposited by it. Results of our study, using sophisticated geochemical and isotopic proxies, conclusively establish that the ancient Ghaggar was a round-the-year flowing, glacier-fed river during 9,000 to 4,500 years ago, when the Pre and Early Harappan settlements had flourished along its banks. This river matches with all the descriptions of the river Saraswati, thus reaffirming its existence during the Harappan period.

“High temperature Superconductivity in Fe-based materials; role of electronic structure studies”

Date
2019-12-04
Speaker
Dr. Haranath Ghosh
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Superconductors are miracle Materials --- many surprising phenomena they exhibit, from zero resistance to quantum levitation. The race is on to make the first room temperature superconductor, several examples that room temperature superconductivity is a reality will be presented. Available high temperature superconductors may be classified into two categories; conventional (BCS) and unconventional (non-BCS) superconductors. Discovery of Fe-based superconductors is ground breaking and hints for a new path way to high temperature superconductors. The new materials feature FeAs layers instead of Cu-O layers of the famous cuprate high temperature superconductors. Antiferromagnetism in both systems appear from d- electrons, however, in FeAs systems they are much more mobile than cuprates. Unconventional superconducting pairing mechanism (yet to be settled), orbital physics, rich Fermiology, phase diagram and several distinctly different physical properties make them overall a fundamentally different class --- superconductors with not only high Tc but also with technological applications. A pedagogical introduction to the field will open the talk. Structural aspects and its intimate relation to electronic structure, orbital selective nature of various aspects like electron correlation, doping, Lifshitz transition and superconductivity will be emphasized. The latest developments in the field will be discussed along with various challenges in these classes of materials.

“An indirect approach of estimating lunar refractory elements”

Date
2019-11-27
Speaker
Dr. Megha Upendra Bhatt
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

The quantitative estimation of elemental concentrations of the lunar surface is an important tool for understanding the processes relevant for the origin and evolution of the Moon. India’s Chandrayaan-1 mission equipped with three spectrometers provided unprecedented observations of the Moon surface with nearly global coverage in the near infrared (NIR) wavelength range at a spatial resolution in the range of hundreds of meters. The NIR observations can be used efficiently for indirect estimation of refractory elements e.g. Fe, Ti, Ca and Mg for obtaining high resolution global elemental maps. This is in contrast to the direct observations, gamma-ray (GRS) and X-ray spectrometers, where the spatial resolution is at least two orders of magnitude lower. The estimation of refractory elements in the NIR range either relies on empirical relationships between the derived spectral parameters of remote observations and in situ chemical analyses of returned lunar samples or on a global elemental estimation derived using remotely sensed GRS data as a reference. The successful estimation of refectory elements depends on the choice of spectral parameters that can decouple maturity from lunar soil composition. In this talk, I will present a new approach of estimating lunar refractory elements using machine learning technique of support vector regression between spectral parameters derived from the Moon Mineralogy Mapper and global elemental maps derived from the GRS measurements. The results obtained from this new approach are consistent in distribution and range with the GRS elemental maps and do not show artifacts in immature areas due to its robustness to space-weathering effects. I will discuss a couple of site specific cases and illustrate how the concept can be applied to the Chandrayaan-2 data-sets.

“ IRIS2: using representative profiles to invert IRIS Mg II h & kline ”

Date
2019-10-31
Speaker
Dr. Alberto Sainz Dalda
Venue
USO Seminar Hall

Abstract

The thermodynamics of the solar chromosphere and the transition region (TR) is critical for understanding how the solar corona is energized from the photosphere. The most common method to recover the stratified information in the solar atmosphere is through 'inversion codes' which employ an iterative algorithm to solve the radiative transfer equation for a given model atmosphere by minimizing the difference between the observed and synthetic spectra. Since 2013, NASA's Interface Region Imaging Spectrograph (IRIS) has been providing unprecedented observations of the solar atmosphere from the upper photosphere to the corona, with special attention to the chromosphere and the TR. IRIS is equipped with both spectral and imaging capabilities in several wavelengths spanning the far- and the near-UV domain. In this talk, I will present inversions of the Mg II h&k lines observed by IRIS using the STiC inversion code which considers non-LTE, partial redistribution, and plane-parallel geometry. The results from this code, while being comprehensive of the thermodynamic conditions in the chromosphere, are unfortunately, computationally intensive and expensive. An alternative approach is using the concept of the Representative Model Atmosphere with the STiC inversion code, called IRIS2. The foundation of this novel code is based on easy-to understand, easy-to-use, representative elements obtained with a basic machine learning technique, such as k-mean clustering. This allows us to obtain a depth-stratified model atmosphere from the upper photosphere to the chromosphere in a few CPU-minutes for any IRIS Mg II h&k data set. I will illustrate how the concepts behind this code can be applied to any spectro(polarimetric) data.

“Long Term Study of the Sun Using Kodaikanal Digitized Data”

Date
2019-09-19
Speaker
Prof. Dipankar Banerjee
Venue
USO Seminar Hall

Abstract

At the Kodaikanal (KKL) observatory we have four sets of data which consist of While light photoheliograms since 1904, the Ca-K line spectroheliograms since 1906, H-alpha spectroheliograms from 1912 to 1998, and Ca-K spectroheliograms of prominences from 1912 to 1998. All these data are collected with the same instruments with no change in their optics in the last 100 years. Thus, these uniform and contiguous images areextremely valuable to study the long term variations of the Sun over a century. We have recently digitized all these datasets and made them open to the global community through the portal https://kso.iiap.res.in. In this talk I will present a summary of recent science results from this digitized archive.

“Understanding radiation tolerance of PAHs in space and role of collective excitation”

Date
2019-09-18
Speaker
Dr Umesh Kadhane
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Polycyclic aromatic hydrocarbons (PAH) have emerged as strong candidates to explain the origin of infrared emission bands and diffused interstellar bands in astronomical spectra. A large amount of work is being done to understand the survival of these molecules in the harsh interstellar environment. A major channel of excitation namely collective excitation, which is common to all PAHs, has largely remained unexplored till recently. With the help of a series of multi-dimensional investigations spread over nearly 10 years, we have been able to identify the exact role of collective excitation and its after-effects in PAHs exposed to harsh electromagnetic as well as charged particle radiation. This talk presents a comprehensive sketch of this research, including the in-house instrumentation development.

“Hyperbolic Geometry and Chaos in the Complex Plane”

Date
2019-08-21
Speaker
Prof. Mahan Mj
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Instances of hyperbolic geometry come up in nature whenever a system starts developing fast interconnections. Examples include trees, the human brain, and the internet. A tell-tale signature is the existence of a fractal in one dimension less, e.g. the surfaces of trees and brains in the above examples. After dealing with the above examples, we shall discuss a special case where the fractals emerge in the complex plane as a result of symmetries of hyperbolic 3-space. These symmetries act on the complex plane as well; however the dynamics being chaotic, it is hard to get a hold on them directly. Instead, we go to hyperbolic geometry in 3 dimensions, set up a dictionary between the two and finally get a hold on the fractals in the complex plane through our study of hyperbolic geometry in 3 dimensions.

Atmospheric Aerosols in Indian Perspective: Climate and Ecosystem Health Implications

Date
2019-07-24
Speaker
Dr. Sachin Gunthe
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Atmospheric aerosols form because of various emissions from industry, human activities and natural processes. They interact with incoming solar radiation directly by scattering and absorption and indirectly by changing cloud properties. Also, the changes in cloud properties lead to change in precipitation and Hydrological cycle on the Earth. Overall, aerosols are expected to counteract global warming by greenhouse gases but aerosol-cloud interaction and many biosphere-geosphere processes involving aerosols are poorly understood and therefore, they are cause for the largest uncertainty in understanding current and future climate changes. Aerosols of biological origin (bacteria, fungal spore, pollen grains, plant and animal fragments, etc.) are one of the least understood component of the climate system. An overview of changing aerosol properties including bioaerosols over India and their role in cloud and precipitation formation processes on regional and local scale will be given.

Groundwater- A Critical but Stressed Natural Resource in India

Date
2019-05-15
Speaker
Dr. Dipankar Saha
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Food and drinking water security in India is critically dependent on the underlying aquifers. Presently 85% of rural drinking need, 64% of irrigation demand and more than 50% of urban water need is met from groundwater sources. About 8% of India’s GDP is directly linked to groundwater. India is the world’s largest groundwater extractor, with an estimated consumption exceeding a quarter of the global total. Relentless and unplanned extraction of groundwater, often exceeding the annual recharge, has resulted in multipronged un-desirable consequences. The most important of them is desaturation of aquifers, being manifested through declining water levels, drying up of wells and diminishing well yield. The other adverse effect is deteriorating water quality, both in terms of increasing salinity and elevated concentrations of harmful contaminants.

An Overview of Ground, In-Situ, and Satellite Observations to Understand Land-Ocean-Atmosphere coupling associated with the Natural Hazards

Date
2019-05-08
Speaker
Prof. Ramesh P Singh
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Natural hazards occur at any location on land, ocean and atmosphere, effects of these natural hazards have been observed in the source region and also far from the source. In recent years, efforts have been made to enhance observing systems on land, ocean and atmosphere to study characteristics of changes associated with the natural hazards using ground, borehole and satellite observations. An overview of the observing systems throughout the globe will be presented that have provided information about characteristics of land, ocean and atmosphere associated with prior, during and after occurrence of natural hazards. The dense network of observing systems in monitoring and forecast of an impending natural hazard have helped scientists to minimize loss and forecast of natural hazards. The need of dense network in India especially in the Himalayan and Indo-Gangetic plains is required to monitor and forecast of impending natural hazards. The impact of natural hazards occurring on land, ocean and atmosphere affecting all elements of earth systems have clearly shown the existence of land-ocean-atmosphere coupling.

“ Quadrupole mass analyzer: Mathematical principle and COMSOL simulation ”

Date
2019-04-10
Speaker
Prof. K. P. Subramanian
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Mass spectrometry is widely regarded as the most sensitive and specific general purpose analytical technique. Among a variety of techniques used in mass spectrometry, Quadrupole mass analyzer (QMA) has emerged as a common and handy gadget in many laboratories world over. While the principle behind conventional mass analyzers is dispersion, in QMAs mass filtering is based on stable Vs unstable oscillations of ions in a quadrupole RF field. For a given values of parameters defining the AC and DC fields inside a quadrupole, it can be seen that oscillations of ions within a certain mass range are sustained, whereas oscillations of all other ions outside this band are divergent and are removed from the beam. Therefore, QMA is regarded as a mass filter, than a spectrometer. In this colloquium, the history of QMA will be briefly discussed. The basic mathematical steps for analyzing the ion trajectory in a quadrupole field will be presented. The 'filtering property' will be explained in the context of properties of Mathiue Function, which is the governing equation for the function of QMA. From here, the steps towards consolidating these mathematical ideas into a working instrument will be illustrated with an example. Finally, COMSOL simulation of the instrument also will be presented.

Biweekly Monsoon mode in the Bay of Bengal

Date
2019-03-27
Speaker
Prof. Debasis Sengupta
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

The Asian monsoon has two quasi-periodic "modes" of sub-seasonal variability - a northward moving mode in the 30-50 day period band, and a westward moving 10-20 day mode (or the "quasi-biweekly" oscillation). These two modes have been known to tropical meteorologists for over four decades, but the discovery of sub-seasonal modes in the ocean is relatively recent. I shall discuss some remarkable 10-20 day oscillations seen in mooring, satellite and other observations from the equatorial Indian Ocean and north Bay of Bengal.

“ Space Sciences at Los Alamos National Laboratory – A Personal Perspective ”

Date
2019-03-20
Speaker
Dr. G. D. Reeves
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

This talk will be centered around some of the space science activities at Los Alamos National Laboratory (LANL) with a particular emphasis on personal involvement in some of those projects. LANL has been involved in space science for over 60 years. The origin of LANL’s Space Science program was the Vela satellite program which started in 1959 to monitor compliance with the test ban treaty. Los Alamos continues that mission to this day with systems such as the Global Position System (GPS) based nuclear detonation detection instruments and research into fundamental physics problem in collaboration with NASA and the international space sciences community. The fundamental space sciences research at LANL has greatly expanded to include solar-terrestrial interactions, studies of the heliopause and interstellar medium with energetic neutral atoms, planetary exploration, magnetospheric physics, radiation belt physics and many other areas. This talk will bring out some of that history and personal recollections of the history and of space sciences at LANL.

Femtosecond Laser Induced Spatiotemporal Control and Photothermal Spectroscopy for Remote Sensing and Computing at Nanoscale

Date
2018-10-03
Speaker
Prof. Debabrata Goswami
Venue
Nanosims Lecture Hall, PRL

Abstract

Femtosecond laser pulses have been shaped in a programable manner for coherent control at molecular level and for several coherent optical processes that have resulted in applications to fast switching, data compression, ultrasensitive detection, computing, etc. Optical and quantum interaction and their detection remain at the forefront of all such efforts. Typically, however, it is not common for ultrashort time to be connected to ultra-small dimension. Use of femtosecond optical tweezers (FOTs) makes this connection possible. We have developed a novel on-the-fly calibration method of FOT that enables in situ control and contactless measure of absolute temperature and viscosity at nanoscale dimensions. Such measurements and control at the nanoscale have been challenging since the present techniques can only provide relative off-line measurements that are of low spatial resolution. Such spatiotemporal control with ultrashort pulses provides the possibility of manipulation at nanoscale that can yield several interesting results that include visualization of colloidal aggregation in real time, computational logical operation in localized zone that is then reset with the subsequent pulse train. We simultaneously apply the high temporal sensitivity of position autocorrelation and equipartition theorem to precisely measure and control in situ temperature and the corresponding microrheological property around the focal volume of the trap at high spatial resolution. The FOTs use a single-beam high repetition rate laser for optical trapping to result in finer temperature gradients in comparison to the continuous-wave laser tweezers. Thermal effects are often treated delirious and most spectroscopy efforts remain in removing them. We have, on the other hand, used highly repetitive femtosecond laser heating to develop time-resolved photothermal lens spectroscopy that provide molecule level sensitivity.

The physics of flight: Bernoulli versus Newton

Date
2018-08-29
Speaker
Dr. Navinder Singh
Venue
Nanosims Lecture Hall, PRL

Abstract

Air travel has become one of the most common means of transportation. One wonders about the lifting capacity of uniquely designed wings of Boeing airliners. You might have peeped through the window of an airliner and have noticed the moment of ailerons and flaps when plane takes off or lands, and that might have excited your curiosity. The physics behind these mechanisms is both interesting and challenging. The common question which is generally asked is: How does an airplane gain lift? And the most common answer is via the Bernoulli principle. It turns out that it is wrongly applied in common explanations, and there are certain misconceptions in this field. In an alternative explanation the push of air from below the wing is argued to be the lift generating force via Newton's law. There are problems with this explanation too. In this presentation we will try to clear these misconceptions, and the correct explanation, using the Lancaster-Prandtl circulation theory, will be discussed. The physical meaning of the Kutta-Joukowski condition will be illustrated. At the end, a brief discussion of a new viewpoint advanced in PRL will also be presented which goes beyond the Lancaster-Prandtl theory. This talk will discuss the physics of paragliders and powered paragliders.

A Practical Approach To Strengthening Our Scientific Ecosystem

Date
2018-08-01
Speaker
Prof. Deshdeep Sahdev
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

It is an interesting and remarkable fact that every Nobel-prize winning piece of work in Experimental Physics was carried out on apparatus designed and developed by the physicist in question, be it Rutherford, Raman, Mossbauer or Binnig. I will start by taking the audience through a fascinating journey which saw my team developing Scanning Probe Microscopes, Physical Properties Measurement Systems and hi-end CVDs all the way out to internationally competitive standards. I will then describe how we have gone about enhancing the base so developed for research in material science, condensed matter physics and nano-technology, with packages for scientific computation, many designed and developed (like our instruments) essentially from scratch. By the end of the talk, I hope to have convinced the audience that the complete & seamless, indigenous integration of theory, computation, experiment and instrumentation, which we are beginning to achieve at QuazarTech holds out the promise (not only for us but for centers all over India) of tackling some really interesting physics problems, a few of which I will describe.

The Story of Magnetism

Date
2018-05-30
Speaker
Dr. Navinder Singh
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Every child has at one time or another played with a magnet and been fascinated by its mysterious ways. It is an uncanny feeling to experience the repulsion between the like poles of two magnets. The "magical" properties of magnets have fascinated mankind over the centuries. Questions like why only iron, cobalt, nickel, or their alloys show ferromagnetic behaviour whereas other elements do not, comes to every curious mind? This presentation is devoted to the historical development of the key ideas in the vast field of magnetism. The presentation follows a chronological order (which is also the logical one from the conceptual point of view). We start from the Greeks, to medieval times to and the 20th century, and highlight the key contributions of people line William Gilbert; Coulomb; Poisson; Oersted; Ampere; Faraday; Maxwell; Pierre Curie; Langevin; Weiss; van Vleck; Heisenberg; Pauli; Slater; Stoner; Anderson; Moriya, Hubbard and others. It will be shown how the advent of quantum mechanics resolved some baffling problems in the field. The current problems in the magnetic properties of strongly correlated electronic systems will be presented, and finally we will summarize the current status of the field of magnetism.

Tools, Time and Transitions: New Perspectives on Early Prehistoric Populations in South Asia

Date
2018-05-23
Speaker
Dr. Shanti Pappu
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

In the history of scientific thought, the story of our origins, has been one of the endless fascination and heated debates. The study of human evolution has been approached in recent years through interdisciplinary research including archaeology, palaeoanthropology and genetics, situated within a geochronological and palaeoenvironmental framework. Much of the early fossil and archaeological evidence for the story of human evolution arises from discoveries in Africa. Debates range around the timing and nature of dispersals of differing species out of Africa, with alternate theories being periodically proposed. In this context, the geographical position of South Asia, and its rich and diverse prehistoric archaeological record, critically informs our understanding of cultural aspects of human evolution, behavioral changes and adaptation of populations to past environmental variability. Here, we first situate the South Asian prehistoric record in a global context. We then move to our specific research project comprising excavations at the site of Attirampakkam, Tamil Nadu and other sites along the SE coast of India. Archaeological, geomorphological and geochronological studies here have led to paradigm shifts in our understanding of the prehistoric record of India, reframing current concepts of the age and nature of the early Palaeolithic (Stone Age) occupation of India. In particular age estimates for different cultural phases at Attirampakkam ranging from around 1.7 million years ago to around 172,000 years ago have stimulated global debates on existing theories of the timing and nature of population dispersals out of Africa and across Asia. Implications of these studies in terms of paradigm shifts in viewing trajectories of cultural evolution and population dispersals across Eurasia are discussed here. We conclude by emphasising the crucial importance of Indian archaeology and associated sciences in contributing towards a global perspective of human origins.

Critical phenomena in Uranium Ferromagnetic superconductors

Date
2018-03-14
Speaker
Dr. Kishore Dutta
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The recent discovery of superconductivity below 1K within a limited pressure range in uranium ferromagnetic superconductors triggered many experimental and theoretical investigation on the coexistence of superconductivity and ferromagnetism, revealing their detail electric and magnetic properties. The Curie temperatures for paramagnetic to ferromagnetic (PM-FM) phase transition in these compounds are found to depend strongly on pressure, indicating that magnetic energy is coupled to the lattice. The recent experimental results for critical behavior related to their PM-FM phase transition does not belong to any known universality classes of critical phenomena. In order to capture their critical behavior related to PM-FM phase transition, spin-lattice coupling needs to be considered in the critical theory. Through renormalization-group analysis of such a model Hamiltonian, it is shown that it can capture well the experimentally determined critical exponents for such compounds. This talk will also discuss the importance of magneto elastic interaction in the vicinity of quantum critical points in strongly correlated systems.

Time, and Time Delay, in Atomic Dynamics

Date
2018-02-07
Speaker
Prof. P. C. Deshmukh
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Einstein’s insightful analysis of the symmetry in the laws of electrodynamics changed our perception of space and time in a manner that continues to challenge common intuition. Even as time is not an observable, and perhaps not comprehensible, time-intervals are measurable. Physical atomic processes occur at ultra-fast speeds over attoseconds. In this talk, the Wigner-Eisenbud-Smith (WES) measure of time delay in atomic dynamics will be introduced. Exploiting the time-reversal symmetry, the WES time-delay is well-adapted to estimate the time-delay in the atomic photoelectric effect. Einstein’s explanation of photoionization laid the very foundation of the quantum theory. For over a hundred years, it was considered to be an ‘instantaneous’ process, but in the last decade, there have been pioneering studies, both experimental and theoretical, in which photoionization time-delays on the attosecond time scale have been reported. These are of importance for the atomic-clock technology, and to understand fundamental relativistic effects and many-body electron-correlations in atomic dynamics. This research field is very young, yet quite vast. This talk will provide a brief introduction to this exciting field and discuss our understanding of the photoionization WES time-delay, and its anisotropic character, especially in the energy regions of the Cooper-minimum, and also in the energy regions of autoionization resonances, and the shape resonances.

Electron Transport in Plasmas

Date
2017-11-15
Speaker
Prof. Amita Das
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Understanding electron beam transport and energy deposition in plasma is crucial in the context of many applications such as fast ignition etc., where it is desirable to dump energy in an over dense compressed core of the target where lasers are unable to penetrate. The talk will cover complex collective physics associated with electron beam plasma instabilities, the associated evolution of magnetic fields and the ensuing turbulence leading to possible anomalous behavior of transport. The experimental evidences in support of anomalous transport will be provided. A novel effect arising due to finite transverse beam size will also be demonstrated.

Fascinating world of photons, superposition and entanglement

Date
2017-08-30
Speaker
Dr. Urbasi Sinha
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Quantum mechanics is a cornerstone of modern physics. Just as the 19th century was called the Machine Age and the 20th century the Information Age, the 21st century promises to go down in history as the Quantum Age. In this talk, key properties of quantum systems called Quantum Superposition & Quantum Entanglement and the world of single & entangled photons will be discussed. Also, in this colloquium the ongoing work towards quantum technology in Quantum Information and Computing lab at the Raman Research Institute, Bengaluru will be discussed.

Early Days of Particle Physics in India

Date
2017-07-26
Speaker
Prof. Sreerup Raychaudhuri
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The story of how research into the physics of cosmic rays and elementary particles began in India will be told in simple and non-technical language. Starting from the days before the First World War, the growth of research in this area will be traced till the nineteen-sixties. On the way small anecdotes of the major personalities will be told. Finally, we shall discuss some lessons which can be learned from this historical exercise.

A bird's-eye view of the field of unconventional superconductivity

Date
2017-07-12
Speaker
Dr. Navinder Singh
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Superconductivity is the phenomenon in which at very low temperatures (typically below 30 K) certain metals show no resistance to the flow of electric current. The phenomenon was discovered by Kammerling Onnes in 1911, and was theoretically explained by John Bardeen, Leon Cooper, and Robert Schrieffer in 1957(the BCS paradigm). In 1986, superconductivity was discovered in unexpected materials called cuprates which superconduct at comparatively higher temperatures (of the order of 100 K). These materials go beyond the BCS paradigm, and at present, we do not have the understanding of the mechanism of superconductivity in these materials. The normal state out of which superconductivity emerges is very unconventional, and is not understood. This field, now popularly known as the field of unconventional superconductivity experiences another revival with the discovery of pnictide materials in 2008. The field has seen many different paradigms like RVB, magnetic spin fluctuation mechanisms, and the paradigm of quantum criticality. But there are problems with these paradigms. We present a survey of these developments. An objective critical analysis of the facts shows that the right direction is already there in the literature, however, much needs to be done. We will present an overview of our recent investigations in that direction, and summarize the open problems.

Do the Fundamental Constants change with Time?

Date
2017-06-21
Speaker
Dr. Nissim Kanekar
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Temporal evolution in low-energy fundamental constants such as the fine structure constant and the proton-electron mass ratio is a generic prediction of field theories that attempt to unify the Standard Model of particle physics and general relativity. The exciting possibility of low-energy tests of such unification theories has inspired a number of methods to probe fundamental constant evolution on a range of timescales, from years to billions of years. Astrophysical studies of redshifted spectral lines provide a powerful probe of such putative changes in the low-energy fundamental constants across a large fraction of the age of the Universe. After reviewing the current state of the field, I will focus on two techniques, based on radio spectral lines from the hydroxyl and methanol molecules, and will describe new high-sensitivity results from these methods. Finally, I will discuss present limitations of such studies and the improvements that are likely to be possible with the advent of new experimental and observational facilities over the next decade.

Investigating magnetic flux emergence through multi-wavelength observations

Date
2017-05-17
Speaker
Dr. Rohan Eugene Louis
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The solar magnetic field couples the dynamic processes in the convection zone to the atmosphere of the Sun. The emergence of magnetic flux at the solar photosphere is a key phase in the evolution of the magnetic field and is responsible for driving various phenomena related to solar activity, such as jets, surges, flares, etc. This talk will cover basic aspects of flux emergence, and the various observing facilities available on the ground and in space, which provide a comprehensive coverage of the solar atmosphere. He will also present recent observations pertaining to the diverse range of spatial and temporal scales associated with flux emergence. These challenge our understanding of how the magnetic field is organised in the solar interior and the processes responsible for transient events.

TeamIndus GLXP Mission

Date
2017-04-26
Speaker
Mr. Satishchandra C Wani
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

TeamIndus, is the only Indian participant for GLXP mission and is a strong contender amongst final four international teams. By participating in this mission, TeamIndus, a private space company, shall attempt to land on the moon, and be the fourth in the world after US, USSR and China. This presentation gives an overview of the mission and the different subsystems of the GLXP spacecraft. The competition requires travel on Moon’s surface for 500 m and transmission of high definition images and video to the Earth. To achieve this TeamIndus is also sending a Rover on its spacecraft. The talk shall also discuss many interesting challenges in the path of achieving the moon-shot. Apart from the mission TeamIndus believes in engaging people through its many interesting engagement program viz. Lab2Moon, MOONSHOT Wheels, Million2Moon et al that also shall be briefly touched upon during the presentation.

Chasing the Ultrafast Dynamics in Molecules : Towards Molecular Movies

Date
2017-04-19
Speaker
Dr. Rajesh Kumar Kushawaha
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Atoms and molecules are quantum systems on which many foundation experiments of Quantum mechanics were performed. The structure and dynamics of such systems play a vital role in understanding of the various physical and chemical processes occurring in nature. The nuclear dynamics is ranging from picosecond to femtosecond time domain whereas the electron dynamics is in attosecond time scale. The processes occurring in this time domain are named as ultrafast processes. Understanding the time-resolved ultrafast processes has opened a new direction in atomic and molecular physics, where the evolution dynamics and subsequence changes in molecular structure are probed during the reactions. This has led to the possibility of controlling chemical reaction for molecular engineering. The probing the electron and nuclear dynamics in time domain has given an opportunity to make molecular movies which give us dynamical, structural and products information in given molecular reactions. In this colloquium, the science and techniques to probe the ultrafast processes in molecular systems will be discussed. A few ultrafast processes such as photo-induced dynamics in molecular fragmentation and collapsing of molecular wave packets as per the Copenhagen interpretation, the Young double slit-type interference in polyatomic molecules and probing the molecular wave packets will be demonstrated during the talk. Finally, the molecular alignment and probing the electronic and nuclear wave packets by pump-probe scheme will also be discussed and a movie on molecular alignment will be shown.

Characteristics of waves and oscillations in the atmosphere

Date
2017-04-12
Speaker
Dr. Amitava Guharay
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Waves are one of the most dominant controlling agents of dynamics of the atmosphere. They are generally excited by disturbances in the lower atmosphere and propagate to higher altitudes. The most important feature of the waves is its property of transporting energy and momentum from the lower to the middle and upper atmosphere and thus control and modify large scale circulation and dynamical condition of the ambient atmosphere. Waves play as an important agent of dynamical coupling of various atmospheric regions. Most prominent waves having significant impact on global dynamics are categorized as gravity waves, tides and planetary waves. Atmospheric oscillations are generated by wave and mean flow interactions. In this presentation the characteristic features of these waves and oscillations will be discussed along with recent observations from various parts of the globe.

Oceanography: a journey from geography to biogeochemistry of the oceans

Date
2017-04-05
Speaker
Dr. Arvind Singh
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Until recently, research in oceanography was limited to mapping the oceans and exploring the surrounding lands – resembling a great similarity to geography. Due to the importance of oceans’ role in regulating the earth’s climate, oceanographers have been spurred to understand the processes that occur in the ocean. The northern Indian Ocean provides a unique opportunity to understand such processes. This colloquium will give a historical perspective of oceanography as a subject with a focus on the role of bioavailable nitrogen for ocean organisms.

Black carbon aerosol emissions of India

Date
2017-03-29
Speaker
Dr. Harish Gadhavi
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

While most aerosols (small particles in air) are believed to be producing cooling effect and counteracting warming by green-house gases, black carbon particles in the atmosphere are causing warming due to their absorbing nature. A few modelling studies have estimated warming potential of black carbon particles second only to CO2. Black carbon particles are also the smallest particles found in the atmosphere, which makes them serious health hazard and also gives them ability to survive longer in the atmosphere. Despite their unique and important role in regional and global climate, a very little progress has been made in understanding their impact quantitatively. Emission inventories constitute critical input to any climate as well as chemical transport models. This talk will discuss about how black carbon particles affects climate, the assessment of recent emission inventories and plan to improve them.

The Universe as a Giant Laboratory: The Making of Complex Molecules from Simple Atoms

Date
2017-03-22
Speaker
Dr. Kinsuk Acharyya
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Observations reveal that our Universe is surprisingly molecular. Molecules are found almost everywhere starting from the high-redshift galaxies to the nearby solar system. More than 200 different gas phase molecules and around 20 molecular species on the dust grain surface has been detected in the various astrophysical environments. Many of these molecules are organic, and therefore important astro-biologically. These molecules range in complexity from diatomic H2 to a 15-atom linear nitrile, HC13N, and many of these molecules are quite unusual by terrestrial standards. In the gas phase, H2 is the most abundant molecule by far, with CO in the second position, four order of magnitude lower. On the other hand, water dominates on the dust grain surface. More complex molecules are even less abundant – at least 4 to 10 orders of magnitude lower than H2. These molecules are very important because they could be the precursors of more complex biomolecules including simple amino acids, such as glycine. The possible molecular precursors of larger organic molecules, such as CH4, H2O, NH3, HCOOH, CH3COOH are all detected in the various astrophysical environments. Thus understanding how these molecules are formed in the variety of astrophysical conditions are of prime importance. This talk will discuss about how these molecules are formed and ongoing research work.

High Resolution Spectroscopy studies of Transiting Systems

Date
2017-03-15
Speaker
Dr. Priyanka Chaturvedi
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

A vast majority of observations of M dwarfs, of varying masses, have reported a higher radius by 10-20% than those predicted by the theoretical models. The mismatch of the radii as seen in these stars is termed as the 'M dwarf radius problem'. Studying M dwarfs in Eclipsing Binaries (EBs) with an aim to alleviate the M dwarf radius problem has been the motivation for the current research work. Mass measurements have been performed by Radial velocity observations using the high-resolution spectrograph, PARAS coupled with the 1.2 m telescope at Gurushikhar Observatory, Mount Abu, India. A software code, PARAS SPEC has been also developed to determine the stellar properties of the host star. I shall be briefly talking about this tool as well.

Luminescence Dating: Developments and Applications

Date
2017-03-08
Speaker
Dr. Naveen Chauhan
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Nowadays luminescence has gained its place in different industrial and research areas. It is finding an important place in our everyday life and knowingly or unknowingly we are using materials possessing luminescent properties. In Geo-sciences it is widely used for the paleo-climatic studies, earthquake prediction, study of meteorites, evolution of deserts, Tsunami studies and other evolutionary studies. Luminescence dating is a radiation damage based method that utilizes the trapping of radiation induced charges in lattice defects and retaining some of these for geological timescales. In this method, the trapped charge concentration in a mineral is assumed to be zero at a time t=0 which later build up due to radiation exposure at a constant rate. This trapped charges can thus be probed via stimulated luminescence emission for estimating the radiation dose and hence the duration of exposure. In the present colloquium I will discuss the basics of luminescence technique, some of the issues which are being researched. I will also discuss ongoing research and instrumental development and the new program which are initiated in PRL.

Mars: Impact Cratering and volatiles

Date
2017-02-22
Speaker
Dr. S. Vijayan
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Impact craters are the natural windows to explore the planetary bodies. They are one of the predominant surface features on the planetary bodies that formed from the early stage of planetary evolution and continuing till date (sporadically in very small size and scale). Though billion-year-old Cratering records on the Earth are not well preserved, Mars and other planetary bodies do preserve it. On Mars, the recent to older impact craters are preserved and they vary in sizes from few meters to 100’s of km. Mars hosts unique type of craters called layered ejecta craters, which are formed due to interaction with the subsurface volatiles. Along with craters, the Mars holds ample evidence for fluvial activities. The outflow channels on the Martian surface are the typical representative for surface fluvial flows. However, majority of the Martian fluvial activities ceased during the Noachian epoch (~>3.7 Ga), which is still a quest. This talk will discuss about the Cratering history on Mars, their likely correlation to fluvial activities and their contextual relationship to Mars. The geomorphic and chronological evidence suggests that the Martian fluvial activity not completely ceased during Noachian epoch, but occurred sporadically at localized zones during Amazonian (<~3.4 Ga) and Hesperian (~3.4-3.7 Ga) epochs. Chronologically, this implies that the volatile source was preserved in the Martian subsurface to form fluvial related channels on the surface or by forming layered ejecta craters on the surface of Mars.

Solar wind turbulence: a reconciliation of observation and theory

Date
2017-02-15
Speaker
Dr. Aveek Sarkar
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Sun, like other stars, can have wind in its atmosphere. Existence of such 'solar wind' was first proposed in 1958. A few years later, this proposal was confirmed via spacecraft observation. Since then it has attracted a lot of interests from solar physicists. Solar wind shows complicated turbulent behaviour. It has been suggested based on various observations that at 1 AU, solar wind consists of spaghetti-like magnetic field structures with the magnetic topology of flux tubes. It is also observed that the plasma fluctuation spectra at 1 AU show a plasma beta dependence. Reconciling these two sets of observations together, the present talk will discuss the direct numerical simulation of the full magnetohydrodynamic equations and will show that if the plasma inside the flux tube is driven unstable by spatial inhomogeneities in the background plasma pressure, the observed nature of the fluctuating power-spectra agree reasonably well with observations as well as with analytical predictions.

Observationally probing the physical processes in massive star-forming regions

Date
2017-02-01
Speaker
Dr. Lokesh Kumar Dewangan
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Massive stars (> 8 Msun) have a significant impact, through their energetics, on the evolution of galaxies and the universe in general. The energetics of massive stars can also affect star formation positively and negatively. However, despite their importance, the understanding of the birth and feedback processes involving massive stars is still under debate. In recent years, space-based infrared observations have revealed many massive star-forming regions which contain infrared dark clouds, mid-infrared shells or bubbles, 6.7 GHz methanol maser emission, HII regions, and young star clusters together. It is indeed obvious that such sites host numerous complex physical processes of star formation. At the same time, these sites are extremely promising to probe important observational evidences concerning the formation of massive stars and their feedback. I will present the results of an analysis of promising massive star-forming regions using a multi-scale and multi-wavelength approach.

Plasma Drifts in Equatorial Ionosphere: New Insights

Date
2017-01-25
Speaker
Dr. Debrup Hui
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The advancement of modern day society is increasingly becoming dependent on space based technologies. Our day to day requirements of communication, navigation and positioning system depend on trans-ionospheric transmission of electromagnetic waves. A faithful propagation of these waves requires very good knowledge of space weather conditions in the ionosphere. Improved models of space weather ask for a clear understanding of the plasma drifts in the ionosphere under influence of different drivers. Plasma drifts are caused by ionospheric electric fields that are curl-free (irrotational) in nature. In order to satisfy this curl-free condition of the ionospheric electric field during varying space weather conditions, it is necessary to understand the altitudinal as well as longitudinal variations in plasma drifts. These aspects that are important for realistic ionospheric models and for the evaluation of space weather effects on equatorial ionosphere, will be presented.

The Fundamental Parameters of Very Low Mass Stars

Date
2017-01-18
Speaker
Dr. Arvind Singh Rajpurohit
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Very Low-Mass stars (M dwarfs) are an important source of information for probing the low mass end of the main sequence, down to the hydrogen burning limit. They are the dominant stellar component of the Galaxy and make up the majority of baryonic matter in the Galaxy. Moreover, an increasing number of M dwarfs are now known to host exoplanets, including super-Earth exoplanets. The determination of accurate fundamental parameters for M dwarfs has therefore relevant implications for both stellar and Galactic astronomy as well as planetology. Despite their large number in the Galaxy, M dwarfs remain elusive objects and the modelling of their photosphere has long remained a challenge (molecular opacities, dust cloud formation). The description of these stars therefore need a strong empirical basis, or validation. This talk will focus on various method and their shortcomings in determining the fundamental stellar parameters of these Very Low-Mass stars (M dwarfs) and to test recent model atmospheres.

Different facets of Active Galactic Nuclei and their evolution

Date
2017-01-11
Speaker
Dr. Veeresh Singh
Venue
K. R. Ramanathan Auditorium,PRL

Abstract

Observations over the last couple of decades have shown that almost all galaxies host SuperMassive Black Holes (SMBHs) of the order of million to few billion solar mass in their centers. The manifestation of accreting SMBHs in the centres of galaxies is termed as 'Active Galactic Nuclei' (AGN) which can play a crucial role in galaxy evolution via feedback processes. Hiterto, AGN population studies have mainly been limited to the local Universe, but more sensitive observations in recent years allow us to unveil new population of AGN at distant Universe. Our deep radio continuum surveys combined with auxiliary optical, IR surveys have discovered a new population of AGN called ‘Infrared-Faint Radio Sources’ (IFRSs). These AGN are at the redshift of (z) ~ 2 – 4 and exhibit diverse properties in terms of their radio luminosities, sizes and spectra, indicating them to be radio-loud AGN at different evolutionary phases. The discovery of IFRSs has important implication on the models of galaxy evolution and missing unresolved component of Cosmic X-ray Background. This talk will also discuss about the role of deeper surveys from upcoming telescopes operating at radio, optical, IR and X-ray wavelengths.

From Sundials to Atomic Clocks - A glimpse into the amazing journey

Date
2016-12-28
Speaker
Dr. Amitava Sen Gupta
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

One of the things that we do not have to worry about in our day to day life today is accurate time. We just have to look at our watches, mobile phones, the internet or the radio and TV. For scientific experiments, requiring very accurate time, we can use time from atomic clocks perhaps relayed through navigation satellites such as the GPS. But have you ever wondered about the development over millenia that made such incredible timekeeping available to us today. This talk will give a brief historical development of timekeeping from the ancient days about a few millenia BC to the present day atomic clocks. We shall describe the sundials, water clocks, mechanical clocks, quartz clocks and finally the atomic clocks. The present day atomic clocks are so accurate that they can keep time to a few billionth part of a second per day.

Fourier Transform Microwave Spectroscopy: the ultimate structural tool for molecular science and astronomy

Date
2016-07-20
Speaker
Dr. Mausumi Goswami
Venue
K. R. Ramanathan Auditorium

Abstract

Fourier Transform Microwave Spectroscopy (FTMW) is an unparalleled method of choice when it comes to determining highly accurate structures of molecules and complexes in the gas phase. This talk will give a brief overview of the FTMW technique and will discuss how the advent of modern technology has led to the discovery of a revolutionary technique like 'Chirped Pulse FTMW'. Some examples from recent work will also be discussed to highlight how the FTMW techniques can be applied to determine 'near equilibrium' geometry and dynamics of weakly bound complexes, and how laboratory studies of molecular species using FTMW can lead to remarkable astronomical discoveries.

New Horizons Mission to Pluto and Beyond

Date
2016-06-01
Speaker
Dr. Henry Throop
Venue
K R Ramanathan Auditorium

Abstract

After a nine‐year journey though space, astronomers visited Pluto for the first time in July 2015, using a robotic NASA spacecraft called New Horizons. Despite being a cold and small icy body, New Horizons found Pluto's surface to be young, dynamic, and varied. Planetary Scientist Dr. Henry Throop will tell the story of this NASA spacecraft mission, from its development and construction, through launch in 2006, to its successful encounter with Pluto, and plans for onward encounters with bodies in the distant Kuiper Belt.

Quantum entanglement and the phases of matter

Date
2016-04-13
Speaker
Prof. Subir Sachdev
Venue
K.R.Ramanathan Auditorium,PRL

Abstract

Most the familiar phases of electronic matter have been understood in terms of the quantum theory of independent electrons moving in a crystal: this includes most metals, insulators, semiconductors, and superconductors. However, a number of modern materials require understanding of phases with long-range quantum entanglement between the electrons. This is especially so for certain quantum “critical” states: these turn out to have a holographic connection to the dynamics near the horizon of a charged black hole. I will describe recent experimental observations on graphene, and on the copper-based high temperature superconductors, and interpret the results using theories of quantum criticality.

Gauge Symmetries: Hiding & Seeking

Date
2016-03-16
Speaker
Prof. K. Sridhar
Venue
K R Ramanathan Auditorium

Abstract

I will present a non-technical and somewhat idiosyncratic account of the major milestones in the development of gauge theories in high-energy physics and their establishment as empirically verified theoretical descriptions of the sub-atomic world. I will describe gauge theories in the more apparent manifestations as they occur in Quantum Electrodynamics and Quantum Chromodynamics. I will then go on discuss spontaneously broken gauge theories -- which are situations where the gauge symmetry is hidden -- relevant for electroweak theories. I will discuss in some historical detail the path leading to the prediction of the existence of the Higgs boson and finally discuss the searches for the Higgs boson at colliders and its final discovery at the Large Hadron Collider in CERN.

Neutrinos and New Physics

Date
2016-02-24
Speaker
Prof. Frank Deppisch
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Neutrinos are an all present yet elusive part of the Universe. They play an important role in many phenomena, from radioactive decays and the energy production in stars to the general structure of galaxies. Yet neutrinos are still the least understood part of what constitutes known matter in the Universe. As such they currently provide the only solid departure from what is considered the Standard Model of particle physics and an explanation of their properties forms a crucial part of new theories that aim to understand the fundamental structure of nature. This makes neutrino physics a fascinating and highly important research field. In my talk I will try to give an account of how neutrinos may be used as a 'missing link' to new physics. I will address neutrino oscillations, the nature of masses in physics as well as the role neutrinos might play in explaining the origin of matter in the Universe.

How tiny fruit flies are helping us better understand the astronauts health in space?

Date
2016-02-17
Speaker
Dr. Ravikumar Hosamani
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Outer space is deep, dark and challenging, coupled with reduced gravity and radiation makes it worst experience for any life form. Fundamentally, all living organisms are evolutionarily adapted to Earth’s gravity. Microgravity has an adverse impact on an organism at various levels such as cells, molecules and genes. NASA’s historic landing of Curiosity on Mars surface and subsequent science findings elevated the hope of humanity to become multi - planetary species in near future. However, to realize this dream, one needs to understand the ill effects of microgravity and outer space environments on human health extensively. We know from ongoing research on the International Space Station (ISS), staying in this confined isolated microgravity environment for few weeks has devastating effects on the astronaut’s health. Some of the pressing health issues are loss of bone structure, muscle loss, compromised immune response, cardiovascular effects, and altered behavior. In this talk, I am going to highlight some of this research we carried out on the ISS using fruit fly as a model organism.

From Dust to Planets: The Cosmochemical Perspective

Date
2016-01-27
Speaker
Dr. Meenakshi Wadhwa
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The earliest history of our Solar System is literally written in stone ‹actually, meteorite. Meteorites are an amazing treasure trove of information about the beginning of our Solar System, how the terrestrial planets accreted and then differentiated to form core-mantle-crust, what the source of water and other volatiles was on these planets, and perhaps even how life may have emerged on our planet. In this talk, I will touch broadly on these themes, and will discuss how the methods and the powerful toolkit of cosmochemistry are allowing us to gain a better understanding of the natural world around us and of our place in the universe.

Can I see a Black Hole? --Life and Death of Massive Collapsing Stars in the Universe

Date
2016-01-06
Speaker
Prof. Pankaj S. Joshi
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The year 2015 was the 100th year of Einstein's theory of gravity, or the General Theory of Relativity, which is one of the most important cornerstones of modern physics and cosmology. Black holes and space-time singularities are amongst the most important predictions of the General Theory of Relativity. We shall review these predictions of the Einstein theory and in particular the current efforts to obtain a direct confirmation of black holes. Specifically, general relativity predicts three kinds of space-time singularities: the Big Bang, which is the origin of the observed Universe, those hidden within a black hole, and the ones which are visible or naked singularities. The latter two types arise from the gravitational collapse of massive stars, and when visible they offer an opportunity to test the Quantum Theories of Gravity or the Unification of Physics, as we shall discuss.

The Solar Ultraviolet Imaging Telescope on board Aditya-L1

Date
2015-12-30
Speaker
Dr. Durgesh Tripathi
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The Solar Ultraviolet Imaging Telescope (SUIT) is an instrument onboard the Aditya-L1 spacecraft, the first dedicated solar mission of the Indian Space Research Organization (ISRO), which will be put in a halo orbit at the Sun-Earth Langrage point (L1). SUIT uses an off-axis Ritchey–Chrétien configuration telescope with a combination of 11 narrow and broad bandpass filters that will take images of the full solar disk in the UV wavelength range 200-400 nm. It will provide near simultaneous observations of lower and middle layers of he solar atmosphere, namely the Photosphere, Chromosphere and lower transition region. These observations will help to improve our understanding of coupling and dynamics of various layers of the solar atmosphere, mechanisms responsible for stability, dynamics and eruption of solar prominences and CMEs, and possible causes of solar irradiance variability in the NUV region, which is of central interest for the Sun’s influence on climate.

Understanding environmental response to decadal and longer droughts in the Sahara-Sahel region of North Africa: Insights from two new 4He based dust records

Date
2015-12-23
Speaker
Dr. Atreyee Bhattacharya
Venue
K.R.Ramanathan Auditorium

Abstract

Mineral dust emitted from arid and semi-arid regions of North Africa is an important component of the Earth’s climate and has been causally related to prolonged periods of drought in the Sudano-Sahel region in the later part of the 20th century. In this talk, Dr. Bhattacharya will explore two proxy records of dust from the Sahara-Sahel region in relation to drought history of the Sahel region. She will conclude with possible ways to integrate proxy records of mineral dust to gain insights into the coupling between climate variability and environmental response on timescales critical for human decision making.

The Messiah of Mass and Message about More

Date
2015-12-09
Speaker
Prof. Biswarup Mukhopadhyaya
Venue
K.R.Ramanathan Auditorium,PRL

Abstract

The theoretical and experimental developments in the physics of elementary particles, which led to the discovery of the Higgs boson a few years ago, in briefly reviewed. It is thereafter indicated how the very existence of the Higgs boson can lead to possible new physics at the fundamental level.

UV/IR mixing in non-Fermi liquids

Date
2015-10-28
Speaker
Dr. Ipsita Mandal
Venue
K.R.Ramanathan Auditorium

Abstract

We devise a renormalization group analysis for quantum field theories with Fermi surface to study scaling behaviour of non-Fermi liquid states in a controlled approximation. The non-Fermi liquid fixed points are identified from a Fermi surface in (m+1) spatial dimensions, while the co-dimension of Fermi surface is also extended to a generic value. We also study superconducting instability in such systems as a function of dimension and co-dimension of the Fermi surface. The key point in this whole analysis is that unlike in relativistic QFT, the Fermi momentum KF enters as a dimensionful parameter, thus modifying the naive scaling arguments. The effective coupling constants are found to be combinations of the original coupling constants and KF.

Fascinating Life-stories of Pulsars

Date
2015-08-19
Speaker
Prof. Avinash Deshpande
Venue
K.R. Ramanathan Auditorium

Abstract

Pulsars are believed to be strongly magnetized, fast rotating neutron stars, with over 2000 discovered in our Galaxy so far. In the long march towards the elucidation of the mysterious ways of pulsars, a few special ones have taught us more than most of the rest put together. Apart from sharing our understanding of the origin and evolution of these cosmic light-houses, the talk will try to highlight a few illustrious members of the pulsar family, and focus on some of the key messages they bring to us.

Centennial-scale links between Atlantic Ocean dynamics and hydroclimate: a spotlight on the Little Ice Age

Date
2015-08-05
Speaker
Mr. Kaustubh Thirumalai
Venue
K.R.Ramanathan Auditorium

Abstract

The Gulf of Mexico (GOM) is an integral component of tropical-to-extratropical heat transfer in the Western Hemisphere. Sea-surface temperature (SST) and sea-surface salinity (SSS) in the GOM strongly influence the moisture budget of North America. Oceanographically, the GOM is dynamically complex owing to the Loop Current, a surface current that transports 23 Sv (1 Sv = 106 m3s-1) of warm Caribbean waters through the Yucatan Strait into the GOM and ultimately flows out of the Florida Straits as a precursor to the Gulf Stream. The signature of the Loop Current is manifest as SST and SSS anomalies in the northern and western GOM through eddies. The brief length of the observational record however, limits us from knowledge of long-term (century-scale) variability in GOM oceanography. Understanding variability of GOM SSTs and SSS on these timescales is crucial in understanding North American hydroclimate variability and equally importantly, can give us key insights into Atlantic Ocean dynamics. Here, using a suite of well-dated sediment cores collected from the Garrison Basin, GOM, we reconstruct local SST and SSS variability during the late Holocene by employing planktic foraminiferal geochemistry. I will make a case in this talk that the reconstructed temperature and salinity variations at Garrison Basin are representative of large-scale climatic processes on centennial timescales. With a multiproxy analysis, we show that proxy data during the Little Ice Age (1450-1850 AD) display a spatially consistent pattern compared to low-frequency spatial field correlations of observational data. Our study provides strong evidence for a tight coupling between Atlantic Ocean dynamics and hydroclimate in the Western Hemisphere, during a time period where climatic background conditions were similar to the preindustrial era.

Detection of organics with MOMA onboard 2018 ExoMars Rover : Future Prospects of GC MS in Solar System Exploration

Date
2015-07-15
Speaker
Dr. Chaitanya GIRI
Venue
K.R.Ramanathan Auditorium

Abstract

Gas Chromatograph-Mass Spectrometer’s (GC-MS) have been regular payloads on board space exploration missions aiming to identify extra-terrestrial organics in situ. Analytical chemists, across wide fields of research, acknowledge this technique as ‘Gold Standard’. GC-MS are space-proven and have identified several organics in the atmosphere of Titan (ACP/Cassini-Huygens), on comets (COSAC/Rosetta) and to a certain extent on Mars surface (Viking Biological Experiments/Viking; SAM/Mars Science Laboratory). The perchlorate and iron sulphate enriched Noachian–Hesperian terrains of Mars pose a great challenge for the usual pyrolysis driven GC-MS in detecting complex organics, if present, in their native state. In the pursuit of detecting organics in the challenging Mars surface environment, the Mars Organic Molecule Analyzer (MOMA) will be a key rover scientific instrument on board the ESA/Roscosmos ExoMars mission, scheduled for launch in 2018. With MOMA, a combined GC-MS–LD-MS (Laser Desorption–Mass Spectrometer), cutting-edge instrumental strategies have been developed to overcome the effects of organic-antagonistic environment as well as detect background organics delivered to Mars by meteorites. This talk will focus on the ongoing research and development of MOMA and mention its COSAC heritage; the latter has earned rich scientific dividends. The COSAC on board the Philae Lander recently made successful in situ detections of organics emanating from the nucleus of comet 67/Churyumov–Gerasimenko. The talk will settle with the future prospects of GC-MS technology for asteroid, cometary and planetary exploration and in the overall advancement of the transdiciplinary astro-bio-geo-chemical sciences.

Electric Dipole Moment of the Electron: Present Status and Future Prospects

Date
2015-05-06
Speaker
Prof. B. P. Das
Venue
K.R.Ramanathan Auditorium

Abstract

The observation of a permanent electric dipole moment (EDM) of a physical system is a signature of the simultaneous violations of parity (P) and time-reversal (T) symmetries. T violation implies the violation of the combined symmetries of charge conjugation and parity;i.e. CP violation via the CPT theorem. The origin of CP violation is still not well understood. This phenomenon has only been observed in the K and B mesons, and the results are essentially in agreement with the predictions of Kobayashi and Maskawa in the framework of the standard model of particle physics. However, this model cannot explain the matter-antimatter asymmetry in the universe for which CP violation is a prerequisite. In addition, its prediction of the electron EDM is several orders of magnitude below its current limit. Indeed the electron EDMs is an excellent probe of new physics beyond the standard model. The talk will focus on the EDM of the electron. After touching upon the connection of the electron EDM with the standard model, its manifestation in atoms and molecules will be highlighted. The symbiotic relationship between atomic/molecular theory and experiment in determining the electron EDM will be emphasised. The present status and the future prospects of the search for the electron EDM will be presented and their implications for physics beyond the standard model will be discussed.

Human Brain & Market Behavior: Are they Identical?

Date
2015-04-01
Speaker
Prof. Prasanta K. Panigrahi
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

It has been conjectured that, human brain and stock market behave in a similar manner, with the neurons in the brain, representing the companies. Various sectors in the stock market show similar fluctuation properties, as of various domains in the brain. It has been experimentally shown that high frequency fluctuations correlate the neurons in a given domain, and the low frequency ones, help establish correlations between different domains in the brain. With the help of ‘Wavelet transform’, to disentangle multi-scale dynamics and ‘Random Matrix’ to characterize them, we explore the precise nature of the fluctuations in the market behaviour. The evolving Network of the sectors in the stock market at different levels of fluctuation, points to the veracity of the above conjecture.

Kinematics and Consequences of Coronal Mass Ejections in the Heliosphere

Date
2015-03-25
Speaker
Mr. Wageesh Mishra
Venue
K. R. Ramanathan Auditorium, PRL.

Abstract

Coronal mass ejections (CMEs) are the most energetic eruptive phenomena occurring in the heliosphere. Investigating their heliospheric evolution and consequences is critical to understanding the solar-terrestrial relationship. Prior to the development of wide-angle imaging of the heliosphere, the studies about propagation of CMEs was limited to analysing their plane-of-sky projected remote observations within few solar radii of the Sun, and in situ observations in the vicinity of the Earth. Also, the kinematics of CMEs can change significantly in interplanetary medium in case of two or more CMEs interaction/collision or strong aerodynamic drag experienced by CMEs with ambient solar wind. Heliospheric Imagers (HIs) on-board STEREO providing multiple views of CMEs in the heliosphere, for the first time, have filled the vast and crucial observational gap between near the Sun and the Earth. Therefore, the 3D kinematics of CME, from its lift-off in the corona to the Earth or even beyond, can be estimated by implementing 3D reconstruction methods on STEREO observations. In this talk, I will discuss about the continuous tracking and estimation of 3D kinematics of CMEs in the heliosphere using HIs data. The use of 3D kinematics of CMEs to predict their arrival time at the Earth will also be presented. In my talk, I will focus on the evolution and consequences of the interacting/colliding CMEs in the heliosphere using their remote and in situ observations. We have also studied the pre- and post-collision dynamics, momentum and energy exchange between the CMEs during the collision phase. My talk will show the need of longer tracking of CMEs in the heliosphere and use of their post-collision dynamics for the purpose of improved arrival time prediction of CMEs at the Earth.

Hot stuff

Date
2015-03-18
Speaker
Prof. Sourendu Gupta
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

Hot strongly interacting matter once filled the universe, but in the last 14 billion years it has only been briefly produced in relativistic collisions of heavy ions. Its properties can be extracted from a quantum field theory using supercomputers. Now a collaboration of experiments and theory is beginning to test this connection accurately, I will describe what has been found, the context, and what we hope to gain in the next few years.

"Physics of light flavoured quarks"

Date
2015-02-25
Speaker
Prof. B. Ananthanrayan
Venue
K R Ramanathan Auditorium, PRL, Ahmedabad.

Abstract

Familiar objects like protons and neutrons are composite objects made up of light quarks and gluons. These objects are confined inside protons and neutrons and due to the nature of the strong interactions that bind them, extracting their properties is a huge challenge, but crucial for our understanding of nature. In this talk, which would be accessible to any physicist, we will describe the state of the art in the physics of light quarks, beginning with a discussion on the extraction of the coupling constant of the strong interactions. Some recent experiments that probe the lifetime of crucial particles such as the neutral pion, and a description of the upcoming experiments to measure the anomalous magnetic moment of the muon will also be covered. Some technical details will be mentioned for sake of completeness, but in as accessible a manner as possible.

New Results Concerning Earth's Van Allen Radiation Belts

Date
2015-02-18
Speaker
Prof. Daniel N. Baker
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

The first great scientific discovery of the Space Age was that the Earth is enshrouded in toroids, or ?belts?, of very high-energy magnetically trapped charged particles. Early observations of the radiation environment clearly indicated that the Van Allen belts could be delineated into an inner zone dominated by high-energy protons and an outer zone dominated by high-energy electrons. Subsequent studies showed that electrons in the energy range 100 keV < E< 1 MeV often populated both the inner and outer zones with a pronounced ?slot? region relatively devoid of energetic electrons existing between them. This two-belt structure for the Van Allen moderate-energy electron component was explained as being due to strong interactions of electrons with electromagnetic waves just inside the cold plasma (plasma pause) boundary. The energy distribution, spatial extent and particle species makeup of the Van Allen belts has been subsequently explored by several space missions. However, recent observations by the NASA dual-spacecraft Van Allen Probes mission have revealed wholly unexpected properties of the radiation belts, especially at highly relativistic (E > 2 MeV) and ultra-relativistic (E > 5 MeV) kinetic energies. In this presentation we show using high spatial and temporal resolution data from the Relativistic Electron-Proton Telescope (REPT) experiment on board the Van Allen Probes that multiple belts can exist concurrently and that an exceedingly sharp inner boundary exists for ultra-relativistic electrons. Using additionally available Van Allen Probes data, we demonstrate that these remarkable features of energetic electrons are not due to a physical boundary within Earth?s intrinsic magnetic field. Neither is it likely that human-generated electromagnetic transmitter wave fields might produce such effects. Rather, we conclude from these unique measurements that slow natural inward radial diffusion combined with weak, but persistent, wave-particle pitch angle scattering deep inside the Earth?s magnetosphere can conspire to create an almost impenetrable barrier through which the most energetic Van Allen belt electrons cannot migrate.

Dark Matter (DM) and Dark Energy (DE) from a Bose-Einstein Condensate

Date
2015-02-04
Speaker
Prof. Rajat K. Bhaduri
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

We first point out the necessity of Dark Matter and Dark Energy (DE) to explain the experimental data. We postulate that cold DM may be in the form of a Bose-Einstein Condensate (BEC) of ultra-light bosons, whose macroscopic wave function has a range comparable to the size of the visible universe. This BEC wave function gives a Bohm potential that contributes a DE term to the equation of motion of the Friedmann universe. The resulting "cosmological constant" has the right order of magnitude.

Fe-based superconductors ; 7 years after its discovery

Date
2015-01-21
Speaker
Dr. Haranath Ghosh
Venue
K R Ramanathan Auditorium, PRL, Ahmedabad.

Abstract

Discovery of Fe-based superconductors is ground breaking and seminal. Unconventional superconducting pairing mechanism (yet to be settled), orbital physics, rich Fermiology, phase diagram and several distinctly different physical properties makes them overall a fundamentally different class. A pedagogical introduction to these systems will open the colloquium. Structural aspects and its intimate relation to electronic structure, magnetism, superconductivity, orbital ordering will be discussed along with latest understanding on various challenges in these classes of materials. The discussion will also comprise of various unusual physical properties like electronic specific heat, BCS characteristic ratio, spin resonance, electronic nematicity etc. A balanced presentation for beginners, unknown to the field, as well as for experts would be made.

Ooty Interplanetary Scintillation Observations and 3-D Heliosphere

Date
2014-12-17
Speaker
Prof. P.K. Manoharan
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL.

Abstract

Interplanetary scintillation (IPS) measurements from the Ooty Radio Telescope provide estimates of solar wind in the heliocentric distance range of ~10-250 solar radii and at most of the heliospheric latitudes. A routine monitoring of IPS on a large number radio sources, along different lines of sight through the heliosphere, allows the reconstruction of three-dimensional structures of quasi-stationary and transient solar wind over a size ~3 AU heliosphere. I will review the results on the three-dimensional distribution of solar wind density and speed and the propagation characteristics of coronal mass ejection (CME) events. This talk will also include a discussion on the IPS tracking of solar disturbances within the inner heliosphere and its usefulness in forecasting the CME arrival by model(s). For example, in the current solar cycle, though weak, a group of large active regions produced five wide and fast CMEs during 12-23 July 2012 and Ooty results on these events have been compared with STEREO measurements, which included an 'ultra fast' CME event originated behind the Sun. The 3-D views of these events obtained from Ooty have extremely been useful in understanding their expansion characteristics as well as to track the far-side originated disturbance.

Indian summer monsoon and associated extreme events based on RegCM projections under CORDEX programme

Date
2014-11-26
Speaker
Prof. Sushil K. Dash
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL.

Abstract

In this study, the seasonal mean summer monsoon over India is projected for the 21st century under the RCP4.5 and RCP 8.5 scenarios using the regional model RegCM CORDEX simulations over the South Asia domain. Here, the state-of-the-art version 4 of RegCM has been integrated from 1970 to 2099 at 50 km horizontal resolution driven by the global model GFDL-ESM2M. The simulated mean summer monsoon circulation and associated rainfall by RegCM4 are validated against the observed values in the reference period 1975 to 2004 based on GPCP and IMD data sets. Future projections are categorized as near-future (2010-2039), mid-future (2040-2069) and far-future (20702099). Results show that the monsoon circulation may become weaker in the future, associated with decrease in rainfall over Indian land points. The RegCM4 projected decrease in JJAS rainfall under RCP8.5 scenario over the central, eastern and peninsular India by the end of the century is in the range of 25-40% of their mean reference period values significant at 5% level. This talk will also project the changes in temperature and rainfall extremes at some selected locations in the country based RegCM CORDEX simulation. Results indicate significant increase in the maximum and minimum temperatures and also decrease in the occurrence of cold nights even at the regional level.

Shock Waves Research in IISc: Taking them to Commercial Arena

Date
2014-11-12
Speaker
Prof. K. P. J. Reddy
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL.

Abstract

Shock Waves are like lasers in their nascent stage, waiting for applications. Until the middle of the twentieth century the field of Shock Waves was mostly confined to gas dynamics, high-speed aerodynamics, and military technology and it quickly developed into a large interdisciplinary field by its own only few decades ago. With the progress in the understanding of fundamental theory, methods of producing shock waves in the laboratory, equation-of-state data, high-speed measurement techniques and visualization methods and computational fluid dynamic techniques, many basic science and engineering branches have emerged in recent times. The spirit of this interdisciplinary nature of shock waves is well captured in the ongoing research work in the Laboratory for Hypersonic and Shock Wave Research (LHSR) in the Department of Aerospace Engineering, IISc. Main focus of the work in LHSR is on using shock waves produced in shock tubes to drive high speed wind tunnels called hypersonic shock tunnels. These tunnels are extensively used to study the planetary reentry aerodynamics and high temperature aerothermodynamics of vehicle configurations which are of interest to our space and defense programs. These studies are useful for the development of thermal protection systems for hypersonic vehicles and also for the enhancement of their performance. However shock waves are also being used for research in other fields including chemistry, material science, biology, veterinary science, medical and industrial applications. In addition, many new methods of producing shock waves for specific applications have also been invented in the laboratory. In this talk we will present a overview of the shock waves research work in LHSR and describe some of our recent inventions and commercial products.

Fast ion-molecule collisions: Interdisciplinary science

Date
2014-11-05
Speaker
Prof. Lokesh C. Tribedi
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL.

Abstract

Present-day atomic collision physics is closely related to interdisciplinary science, besides being a useful tool for the study of atomic, molecular and quantum mechanics. Collisional interactions of fast ions or electrons with clusters and other mesoscopic objects are useful to bridge the gap between gas atoms and bulk solids. A homo-nuclear diatomic molecules, H2 be considered as a smallest double-slit to observe Young type electron interference, originally proposed by Cohen and Fano. The complex allotropes of carbon, such as, fullerenes, nanotubes and large organic molecules of biological (DNA bases) interest have been at the focus of recent atomic collision research. The secondary electron emission from bio-molecules/nucleobases is an important parameter to estimate the radiation damage caused by fast ions. This process is highly influenced by the many-body effects, such as, collective excitation or size effect. The C60 fullerene is used as a bench mark system which manifests the collective plasmon excitation/The electron spectroscopy provides a clear understanding of this process i.e. giant plasmon resonance (GPR). Other class of large molecules (PAH) are interesting from space and astrophysical perspective. The high resolution x-ray studies of highly charged ions find applications in astrophysical plasmas. A recently installed 14.5 GHz ECR-plasma-ion-accelerator and existing 14 MV Pelletron tandem accelerator at TIFR are being used for these measurements with keV-to-MeV energy highly charged ions. The tools for the experiments are continuum electron and recoil-ion spectrometers, high resolution x-ray spectrometer etc. A brief overview of the active field of atomic collision research and its implications in different branches of science will be presented.

QCD Critical Point : A Synergy between Theory and Experiment

Date
2014-10-15
Speaker
Prof. Rajiv V. Gavai
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL.

Abstract

Quantum Chromo Dynamics (QCD), the theory of strong interactions, has a large coupling between its constituents quarks and gluons, necessitating new theoretical tools. QCD on a space-time lattice is the most reliable such tool available to us. One can employ it to look for new phases of strongly interacting matter at high temperatures and densities, and investigate their properties. QCD phase diagram has been a subject of intense discussions. QCD critical point has recently attracted a lot of theoretical, and now experimental, attention and lattice QCD results will be discussed. We argue that the freeze-out curve in the QCD phase diagram, which embodies a substantial amount of precise experimental data in heavy ion collisions, can be used in conjunction with lattice QCD to search for the critical point at RHIC, BNL, New York and other upcoming facilities. While the variance, skewness and kurtosis of baryon number distribution are smooth & monotonic along it at RHIC and LHC energies, the beam energy scan at RHIC should see deviations, signalling the presence of a nearby critical point. Its experimental discovery will be a profound and unique landmark in physics.

Bayesianism in Geosciences

Date
2014-10-08
Speaker
Dr. R. N. Singh
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL

Abstract

Geosciences construct knowledge by using deduction, induction and abduction. Earth has a complex history replete with unique events. This leaves only little scope for deduction, leaving induction and abduction as alternatives. Most research is reduced to either estimation of parameters or selection among hypotheses, both beset with uncertainties. Currently, Bayesianism is preferred in geosciences to deal with all kinds of uncertainties. In the Bayesianism, both the parameters and hypotheses are taken as random variables. Bayes theorem is used to get posterior distribution of parameters or hypotheses which is proportional to their prior probabilities and likelihood function of the data. All which we need to infer or decide are derived from the posterior distribution, mostly using Monte Carlo methods. However, subjectivity in choosing prior distribution invites scope for scepticism in the results. In this talk speaker will discuss the scope and pitfalls of Bayesian methodology in geosciences, with an example of understanding climate change from borehole temperature data.

Melting of shell effects and radiating dumbbells - two interesting problems in nuclear physics

Date
2014-10-01
Speaker
Dr. V. M. Datar
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL

Abstract

In this talk two problems,in low energy nuclear physics will be discussed,as examples of interesting physics that can be explored at facilities such as the Pelletron Linac Facility at Mumbai. The first concerns the damping of the shell effect with temperature predicted by Ramamurthy et al. [PRL 25, 386 (1970)]. This was recently addressed experimentally by measuring neutron TOF spectra using the triton transfer -fusion reaction on 205Tl and 181 Ta targets with a 7Li beam. The second example relates to electromagnetic signatures of the alpha cluster structure of 8 Be. This nucleus, while being unstable in the ground state, lives long enough for subsequent capture by another alpha particle to form 12 C through the Hoyle state at 7.65 MeV. A precise measurement of the rare electromagnetic transition (branch~10−7) from the 4+resonance to the 2 +resonance in8Be, which confronts ab initio calculationsof light nuclei and the simpler cluster model, will be described. The need for a measurement of the much weaker and more challenging 2 +-to-0+transitions , together with calculations that treat state - of -the - art structure models with reaction theory, will be emphasized.

Haloarchaea - an Astrobiological relevance

Date
2014-08-27
Speaker
Dr. Manikandan Muthu
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL

Abstract

Microorganisms are at the frontier of science in the study of origin of life due to their ubiquitous existence, survival and adaptability to harsh conditions. The extreme conditions include high and low pH, temperature , salts, radiation etc. Invariably, these extreme environments have been found to harbour a t least a group of microorganism. Thus it of utmost interest to unravel the facts behind their adaptabilit y, which perhaps will provide clues that would trace back their origin and existence in other planets since, many harsh conditions of earth share commonness of other planets. Salt loving m icro organisms, halophiles, had been well known for their adaptation to extreme conditions such as radiation, halite and stromatolite inclusions that are expected in extra - terrestrial environments. In this background , t he talk will a d dress, the diversity of haloarchaea existing on halite crystals obtained from salterns of Tamilnadu, India and the reasons for their high sense of adaptability. The survival ability of microbes after a prolonged storage at refrigerated conditions will also be discussed. Finally, the probability of a possible voyage of these unique bacteria and their chances of survival under Martian or extraterrestrial environments would be postulated

The Flavour Puzzle and Grand Unification

Date
2014-08-06
Speaker
Dr. Ketan Patel
Venue
Seminar Hall, Above NANOSIMS Laboratory, PRL

Abstract

From the electron mass (0.5 MeV) to the top - quark mass (173 GeV), the masses of electrically charged fundamental fermions s pan over six orders of magnitude. Neutrino masses (< eV) expand this range by another at least six orders of magnitude. Further, it is a puzzling fact that there exist several similarities and differences between the masses and mixing patterns of different fermion flavours. While the standard model of particle physics can successfully account for the observed fermion masses, it does not shed any light on this puzzle. Some of its extensions, originally proposed for the unification of fundamental interactions , provide a more appropriate platform to address this puzzle by unifying also the fundamental fermions. In this talk, I will review some of the grand unified theory based attempts to understand and resolve the flavour puzzle. Examples of approaches based o n new symmetries will be discussed. Alternative proposals from the grand unified theories in higher space - time dimensions will also be discussed.

Supersymmetry, shape invariance and the Legendre equation

Date
2014-07-16
Speaker
Prof. Ashok Das
Venue
K. R. Ramanathan Auditorium, PRL

Abstract

In this talk we will examine the underlying symmetry principle which makes the Legendre equation and the associated Legendre equation soluble. This symmetry relation will also bring out various interesting features associated with these system s such as the recursion relations and the Rodrigues' formula. We will also comment about the solubility of other equations associated with orthogonal polynomials.

Indigenous technology in a Globalized World: A Case Study or Resolving Atoms in our Backyards

Date
2014-04-23
Speaker
Dr. Deshdeep Sahdev
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

It is an interesting and remarkable fact that every Nobel - prize winning piece of work in Experimental Physics has been carried out on apparatus which has been designed and developed by the physicist in question, be it Raman, Mossbauer or Binnig. This makes the question of how we build an instrumentational base for cutting - edge research in India relevant. I will discuss this in the context of several hi -tech instruments which my team has developed: Scanning Tunneling Microscopes for various ap plications,Physical Properties Measurement Systems, High - end Gas Chromatographs, Mass Flow Controllers, and Data Acquisition Systems - to mention but a few. The talk will, in addition, focus on how the expertise we have built up can help in facilitating research (in the pertinent fields) at all our institutions.

Fundamental physics using laser cooled radioactive atoms

Date
2014-02-26
Speaker
Prof. Yasuhiro Sakemi
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

Construction of the high intensity source to produce radioactive heavy atoms is currently in progress at the Cyclotron and Radioisotope Center (CYRIC), Tohoku University. These atoms serve as powerful tools to study the fundamental symmetries of nature such as parity non - conservation (PNC) and CP violation, whose effects are enhanced enormously in these systems. Our aim is to find out the electron electric dipole moment (EDM) by measuring the EDM of the francium (Fr) atom for understanding the matter - antima tter asymmetry of the universe. The Fr atoms are created with the fusion reaction of the heavy ion beams supplied by AVF cyclotron at CYRIC. The procedures to decelerate the produced Fr atoms in the laser cooling technique, their transportation from the ac cumulation cell to the science chamber using the optical dipole trap for measuring EDM, and to trap the atoms by the optical lattices will be reported, which will be of their first kinds upon their successful implementation. The present status of the proje ct together with the overview of the research activities at CYRIC that span over the nuclear physics to the life science, such as proton therapy and Positron Emission Tomography (PET),using the beam supplied by our AVF cyclotron will be discussed.

The Top with spin Zero

Date
2014-02-19
Speaker
Dr. Sudhir Vempati
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

The recently discovered Higgs boson has a mass within a very interesting range: (124 - 127) GeV. This mass range has implications not only for the Standard Model but also for extensions for it, like Supersymmetric models. In these models, the H iggs mass is predicted and its value crucially depends on the properties of the supersymmetric (spin zero) partner of the top particle, the stop. In the present talk, we discuss the properties of this particle and discuss implications on several supersymme tric models. Interestingly, for stops less than 1 TeV, the Higgs mass requires the stop mass parameters to be in a critical range: a minor change in these parameters could mean that our universe resides in a meta - stable vacuum.

Gravitinos, Reheating and the Matter-Antimatter Asymmetry of the Universe

Date
2014-01-15
Speaker
Dr. Raghavan Rangarajan
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

Astrophysical observations indicate that the Universe is made up primarily of matter rather than both matter and antimatter. This matter-antimatter asymmetry of the Universe can be explained by the asymmetric decay of some heavy particles if the early Universe is sufficiently hot after a phase called reheating. But these high temperatures also lead to an over-abundance of particles called gravitinos whose presence has very adverse cosmological consequences, which is referred to as the ‘gravitino problem’. We shall discuss the matter-antimatter asymmetry of the Universe and the gravitino problem, and then examine whether or not the gravitino abundance can be suppressed.

Learning from volcanoes: the story of India's only active volcano

Date
2014-01-08
Speaker
Dr. J. S. Ray
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

A volcanic eruption is one of the most pectacular events of nature. Volcanoes discharge hot ash high into the air and pour streams of molten rock down their flanks. They are the most visible proof that our planet is very much alive. They constantly remind us that, even after 4.56 billion years of its formation, Earth’s interior is still hot and dynamic. Volcanic eruptions vary greatly in style and the materials they produce. Large explosive volcanism can cause widespread destruction of life and property and affect the climate. Therefore, it is necessary to study and understand the eruptive styles and cycles of volcanoes located close to civilizations. My interest in volcanoes lies in the very fact that they provide us a window to the deep Earth. I have been studying products of ancient volcanism in India and elsewhere in the world in an effort to understand the chemical evolution of Earth’s mantle through time. My current endeavor is focused on contemporary volcanism in the Barren Island Volcano, the lone active volcano of India, with the main objectives of deciphering its origin and evolution and the character of the mantle source. Being located in an active subduction zone, the volcano holds keys to our understanding of nature recycling of crustal material into the mantle. In the talk, I will discuss some important results of our research based on geochronology and geochemistry of lavas and tephra derived from this intriguing volcano.

Aerosol-cloud interactions: the uncertain component of climate system

Date
2013-12-18
Speaker
Dr. G. Pandithurai
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

Aerosol and clouds play the key role in the climate system. Anthropogenic aerosols enhance cloud reflectivity by increasing the number concentration of cloud droplets leading to a cooling effect on climate that is known as the aerosol first indirect effect. The resulting smaller cloud droplets also suppress the collision-coalescence process and thereby inhibit rainfall and enhance cloud lifetime. The fundamental cloud microphysical properties are driven by dynamics;vertical motions and mixing processes between the cloud and its environment determine the concentration of cloud water, a key parameter for both climate and precipitation. However, aerosol particles can significantly affect the microphysics and dynamics of clouds by changing the size distribution of drops, their ability to grow to raindrops, their rates of evaporation, and their mixing with the environment. However, many uncertainties still remain. This colloquium will present an overview of the role of aerosol and clouds in the climate system with emphasis on their interactions. Quantifying the role of aerosol and clouds in the climate system paves the way to the understanding of their impact on the climate change.

Omnipresent Ethernet: From Concepts to Products - Secure Communications, Networking and Control Framework

Date
2013-12-11
Speaker
Dr. Ashwin Gumaste
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

The talk begins with the clean-slate design problem of the Internet along with current service provider pain-points, focusing on plausible solutions, narrowing to the concept of Omnipresent Ethernet (OE). The OE concept is introduced as next generation carrier-class Internet architecture. OE extends Ethernet for end-to-end provisioning across the LAN, MAN and WAN, using concepts of Carrier Ethernet in conjunction with simple network architectural understanding. The advantages of OE such as low-latency, low energy, small foot print are discussed. OE working is presented especially in conjunction with some of the advances in Carrier Ethernet. Mapping OE to multiple layers of the protocol stack and some of the base problems that we have considered will also be showcased. A pragmatic 1-micro-second port-to-port supporting 96 Gbps cross-connect Carrier Ethernet Switch Router will be showcased. The working, analysis and the development of this architecture is discussed. OE has led to a family of products, conceptualized, designed, prototyped at IIT Bombay and now made available through DAE's PSU the Electronics Corporation of India Ltd, ECIL. An overview of these products, how these have been developed, the internal workings of the hardware and software as well as deployments in the nation's leading networks and data-centers will be discussed.Some open problems will also be presented.

Spin masing, and looking for an atomic EDM of nuclear origin

Date
2013-12-04
Speaker
Prof. K. Asahi
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

A permanent electric dipole moment (EDM) is an electric polarization vector that spontaneously occurs in a particle with nondegenerate internal state, due to violation of CP. The CP violation embodied in this flavor-diagonal quantity EDM, however, should be different from the "normal" CP violation already included in the Standard Model (the Kobayashi-Maskawa CP violation) and, if observed to be finite,definitely evidences presence of physics beyond the Standard Model. We, at Tokyo Tech, have been preparing for an experiment to search for a 129Xe (Xenon) atomic EDM, with an external feedback nuclear spin maser which enables spin precession to last for an unlimitedly long period. We are now in a stage to incorporate a 3He comagnetometer, and will be conducting an EDM search run in coming spring. Finally discussion will be given on a future extension of the 129Xe EDM experiment incorporating 131Xe spins as a co-magnetometer.

Molecular Beam Microwave Spectroscopy: Applications in Radio-astronomy and Intermolecular Bonding

Date
2013-11-27
Speaker
Prof. E. Arunan
Venue
K.R. RAMANATHAN AUDITORIUM

Abstract

Microwave spectroscopy has played a major role in identifying molecules in space.Our laboratory has built a molecular beam microwave spectrometer, which is one of about 15 all over the world. This spectrometer has a range of 2-26 GHz and the typical line width is only a few kHz enabling measurement of molecular frequencies to 9 or 10 significant figures. We have used this spectrometer to record the microwave spectrum of various molecules and also their weakly bound complexes formed under supersonic jet conditions. Among the molecules recently investigated in our laboratory, two are of interest to astrophysics: phenylacetylene and propargyl alcohol. Both are crucial intermediates to the formation of poylycyclic aromatic hydrocarbons (PAH) which lead to interstellar dusts and also soot particles in diesel engines. While the mechanism of PAH formation (2 dimensional growth) is well established, how do PAH become soot (3dimensional growth) is not well understood.Weakly bound molecular complexes are proposed as intermediates to soot formation. As our spectrometer is equipped with a molecular beam source, such molecular complexes can be formed and investigated. Structures of these molecular complexes are governed by intermolecular interactions which were typically classified as van der Waals interaction and hydrogen bonding. However, there has been a continuous debate about how these two interactions were different. Comprehensive experimental and theoretical studies in our laboratory helped us understand these interactions with unprecedented clarity. This also led us to initiate and complete an IUPAC project to redefine hydrogen bonds. Our work on Argon-propargyl alcohol complex also led us to define a ‘carbon bond’ analogous to the ‘hydrogen bond’. Carbon bonding appears to be important in hydrophobic interactions and also in SN2 reactions. Following our predictions, experimental evidence for carbon bonding has been found using charge density analysis in crystal structure.

Declining solar magnetic fields: Are we heading towards a Maunder minimum?

Date
2013-10-23
Speaker
Prof. S. Ananthakrishnan
Venue
K.R.Ramanathan Auditorium

Abstract

One of the primary indicators of Solar activity is the Sunspot number and the associated 11 year solar cycle. This activity is controlled by the solar magnetic field. There are clear indications based on a variety of studies that the magnetic field on the Sun has been steadily decreasing in the past ~ 20 years resulting in lower activity on the Sun. The Sunspot formation has decreased by ~ 30% since the early 90’s. It has been speculated that if this continues, there will be no sunspots by the latter part of this decade, leading to a Maunder-like minimum in the next cycle. Using Interplanetary scintillation data from radio telescopes, surface photospheric fields measured by National Solar Observatory and He abundances measured by ACE, SDO spacecraft, my collaborators from PRL, Ahmedabad & Harvard Smithsonian Observatory and I have been studying this monotonic decrease.

Signatures of magnetic reconnection in solar flares: A multi - wavelength perspective

Date
2013-10-09
Speaker
Dr. Bhuwan Joshi
Venue
K.R.Ramanathan Auditorium

Abstract

Solar flares are characterized by the sudden release of excess energy stored in the magnetic fields of solar corona. The modern multi-wavelength observations have immensely improved our understanding of the various physical processes occurring in different atmospher ic layers of the Sun during a solar flare. The standard flare model has been successful in broadly recognizing these physical processes as the consequence of large-scale magnetic reconnection in the corona.The objective of the present talk is to summarize the multi-wavelength observations of solar flares taken mainly from the space borne instruments over the last two decades. I will particularly highlight the new results obtained from the RHESSI mission on the X -ray emission from the coronal loops. I will further compare these new observations with present theoretical interpretations in order to discuss the scopes and challenges for future investigations.

Exploring Quark Gluon Plasma with photons, jets, and heavy quarks

Date
2013-09-18
Speaker
Prof. D. Srivastava
Venue
K.R.Ramanathan Auditorium

Abstract

We discuss the developments which have made single photons a valuable probe of quark-gluon plasma produced in the wake of collisions of heavy nuclei at relativistic energy. We also discuss a simple model to simulate jet quenching which provides valuable information on flavour dependence of energy lots of high energy partons as they traverse quark gluon plasma.

Big Bang to Little Bang - Exploring the Quark - Gluon Plasma at R HIC and LHC

Date
2013-09-11
Speaker
Prof. Tapan Nayak
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Under extreme conditions of temperature and/or energy density, normal hadronic matter goes through a phase transition to a new form of matter consisting of de-confined quark-gluon plasma (QGP). The QGP might have been the primordial matter, which filled the Universe until a few microseconds after the Big Bang. The formation of QGP and the nature of the phase transition have been explored at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory and the Large Hadron Collider (LHC) at CERN, by colliding heavy - ions at ultra -relativistic energies. Major findings will be summarized,particularly from STAR and ALICE experiments where the Indian groups have made major contributions.

Oceanic nitrogen cycling: new results based on isotopic trace rs

Date
2013-09-04
Speaker
Prof. R. Ramesh
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Nitrogen is abundant in the Earth’s atmosphere, but much of it is not directly useful for life. Reactive nitrogen is needed for life processes and a small amount of reactive nitrogen is controlling life processes and hence the global carbon cycle. Over the last decade, we have investigated various aspects on the marine nitrogen cycle in the Indian Ocean. Using 15N and 13C tracers we have quantified, besides the biological productivity in the ocean (rate at which carbon is fixed by photosynthesis by marine planktons, measured in units of g C m –2day–1) and its temporal and spatial ariability, the ‘newproduction’, the fraction of the carbon that is dispatched to the deep ocean to stay for longer time scales.We have developed experimental methodologies to measure the direct fixation of atmospheric nitrogen by marine diazatrophs such as Trichodesmium in the water column and also sediments. Further we have quantified the nitrification process, which compensates for the loss of reactive nitrogen to the atmosphere by denitrification.For the latter, we have modified the traditional Rayleigh isotopic fractionation model. We have also evaluated the nitrogen transport to the ocean through rivers and atmospheric transport.In this talk, while highlighting some important new results, we also propose to discuss current and future research in this area.

Challenges in Modeling the Global Climate System

Date
2013-08-28
Speaker
Dr. Govindaswamy Bala
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

There is consensus now that anthropogenic emissions of carbon dioxide and other greenhouse gases since the pre-industrial period are the primary drivers of the current climate warming. How do we verify this? Climate models are the only experimental that is available to us to investigate the sensitivity and future changes to the global climate system. Unlike in a chemistry or biology laboratory where one can perform multiple controlled experiments, it is not desirable to perform experiments with the global climate system. If the outcome of an experiment with our climate system goes awry, the consequences could be catastrophic. Indeed, the current debate on climate change, environmental damage and sustainability stems from the unintentional experiment that we are performing on the planet: land use and land cover change and the growth of atmospheric greenhouses gases and aerosols from the burning fossil fuels. Climate modeling is “Big Science” today: a diverse group of experts are required for the establishment of a modeling center. Contemporary climate models have comprehensive 3-dimensional numerical representation of the major components of the climate system and the interactions and feedbacks between them. Climate models are also known as general circulation models (GCMs). The early general circulation models solved only atmospheric equations of motion, and they are called atmospheric general circulation models (AGCMs). The contemporary models couple the atmosphere, oceans, land, and ice and they are called coupled models or coupled atmosphere-ocean general circulation models (AOGCMs). The state-of-art in climate modeling is to couple the AOGCMs to the global carbon, nitrogen and other biogeochemical cycles and to include of interactive atmospheric aerosols and chemistry. In this talk, I will discuss the challenges involved in the development and applications of these global climate models.

Upcoming 4-meter class optical telescopes at devasthal observatory

Date
2013-08-21
Speaker
Prof. Ram Sagar
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Devasthal, located in the Kumaun region of Himalayas is emerging as one of the best optical astronomy the continent. Currently, a 130 - cm fast and wide field of view optical telescope is operating at the site. By early 2014, a 4 - m international liquid mirror telescope and a 3.6 meter new technology optical telescope shall become operational. Present status of these upcoming telescopes, key scientific projects to be taken with them, along with their first generation back-end instruments shall be presented in the colloquium.

ITER- A Burning Plasma Experiment

Date
2013-08-14
Speaker
Prof. Dhiraj Bora
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Controlled thermonuclear fusion is one of the alternate clean energy sources for future. A worldwide research program in fusion has been going on for many years. Abundant availability of fuel, inherent safety, negligible radioactive waste and no greenhouse emissions are some of the advantages of this source. We note that not only is fusion an attractive source, it is realistic as well. With the acceptance of the International Thermonuclear Experimental Reactor (ITER) baseline in July 2010, the project has now moved into the construction phase at the Cadarache site in the south of France. Therefore, Fusion is no more a dream but a reality. ITER is an international collaboration of seven parties including India to build the first FUSION SCIENCE EXPERIMENT capable of producing a self - sustaining fusion reaction, called “burning plasma”.Unique features will be its ability to operate for long durations and at power levels ~500 MW sufficient to demonstrate the physics of the burning plasma in a power plant like environment. It will also serve as a test - bed for additional fusion power plant technologies. ITER is a long pulse Tokamak with elongated plasma and single null poloidal divertor. In the first phase, nominal inductive operation would produce a DT fusion power of 500 MW for a burn length of ~400 s, with the injection of 50 MW of auxiliary power. The construction phase of ITER will end in November 2020 with the first plasma and DT experiments will start in early 2027. India has joined this international project as the seventh member of the team. Major part of the contribution of each member during the construction phase would be in kind. The present status of the ITER project will be discussed during the talk.

Distinct Volatile Reservoirs in the moon

Date
2013-08-07
Speaker
Dr. Amit Basu Sarbadhikari
Venue
K.R.Ramanathan Auditorium,PRL

Abstract

It has been argued for decades whether the moon contains significant quantities of indigenous water.Initial chemical analyses of lunar rocks in the Apollo era turned up virtually no evidence of lunar water.Recent discoveries of water and other volatiles in the lunar volcanic materia ls indicate that the early evolution of the lunar mantle was influenced by the nature and composition of different volatile species present in it. However, the concentration of those volatiles in the bulk Moon is highly uncertain owing to variation found among the analyzed materials. I have carried out a study on apatite and melt - inclusion in a lunar mare basalt revealing few interesting facts on this heterogeneous distribution of volatiles in the lunar interior, which will be discussed in the colloquium.

On the Magnetic Field Structure and Evolution of flare/CME productive Solar Active Regions

Date
2013-07-31
Speaker
Mr. Vemareddy Panditi
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

Solar flares and Coronal Mass Ejections (CMEs) are energetic, explosive transient events releasing enormous amounts of energy due to sudden destabilization of magnetic field structure in the active regions. Although, flares and CMEs are two different aspects of a large-scale magnetic energy release of the same magnetically driven phenomenon, there is no clear one-to-one relationship between them. Large flares and CMEs are the primary causes of space-weather disturbances; therefore there is need to understand the underlying physics and associated phenomena in these events. A fundamental aspect of the eruption involves gradual storage of magnetic energy of the active region by various mechanisms and its release. As the field lines originate from, and line-tied to, the dense photosphere, plasma motions can stress the field lines to store energy that might lead the system to a magnetically unstable state. So, the complexity of field line connectivity and the non-potential state of active region is defined by flux motions. After the magnetic system of the active region has reached a state of sufficiently adequate energy, its sudden release requires a suitable triggering mechanism to drive the eruption. I will discuss in detail various processes of energy storage and triggering mechanism of these eruptions during the evolution of the active regions. The 3-D magnetic field structures of ARs evolve gradually in response to the photospheric flux motions and also catastrophically as a result of transient events. In the absence of the measurements above chromosphere, one can resort to the technique of magnetic field extrapolations using the photospheric observations as the boundary conditions. Therefore, the models of constructing active region 3-D magnetic fields to coronal heights under force-free assumption using photospheric magnetic field observations and their validity with the coronal EUV observations will also be discussed.

Floating Frogs and Levitating Latoos

Date
2013-07-24
Speaker
Prof. Surendra Singh
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

History and principles of levitation of physical objects using static electromagnetic fields will be described. The role of Earnshaw’s theorem in the development of the field will be discussed and the principles involved will be demonstrated using a working device.

Scaling the Potential Predictability Barrier of the Indian Summer Monsson Rainfall: An Indian Initiative

Date
2013-07-17
Speaker
Prof. B. N. Goswami
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Indian summer monsoon rainfall (June - September rainfall over the Indian continent, ISMR), lifeline for about one sixth of world’s population influences the Indian GDP up to 2 - 5% during a drought year. Skillful prediction of ISMR one season in advance, therefore, is not only of great importance for agricultural planning and policy making for disaster preparedness but also influences the economy through nonlinear influence on other economic drivers. The prediction of ISMR, however,remains a ‘grand challenge’ for the climate science community. The continued poor skill of the ocean - atmosphere coupled models in predicting ISMR remains an enigma in the backdrop of these models’ high skill in predicting seasonal mean rainfall one season in advance over the rest of the Tropics. In this Talk, I will provide an overview of processes that are responsible for limited skill of present climate models and outline a framework for achieving the limit on potential predictability within a reasonable time frame. IITM is leading a program called Monsoon Mission supported by the Ministry of Earth Sciences. The Mission envisages building partnership between operational forecasting agencies and R & D organizations both within India as well as Inter national R & D Organizations to work on improving monsoon prediction. The conceptual framework and the roadmap for the Mission will also be highlighted.

Uncertainity Quantification in Geophysics

Date
2013-04-03
Speaker
Prof. Mrinal K. Sen
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Geophysical inverse problems involve estimating earth model parameters from remotely sensed measurements. The observations are almost always insufficient, inadequate and inconsistent. Thus the inverse problems are highly ill-posed resulting in non - unique estimates of the model parameters. In other words, often multiple models are proposed that can explain the observations equally well.Mathematical techniques such as regularization can be imposed to obtain average or smooth models but they may result in geologically unrealistic solutions. One other approach is to examine all possible models and attempt to estimate uncertainty in the answer. A Bayesian formulation of the inverse problems appears fairly attractive for achieving this goal. In a Bayesian framework, prior information in the model (independent of observations) is combined with observation using a likelihood function to estimate a posteriori probability density (PPD) function in model space. The PPD is indeed the answer to our inverse problem. Unfortunately, for highly non-linear geophysical inversion problems, the PPD does not have an analytic form and is generally multi-modal.It has been demonstrated that the Markov chain Monte Carlo (MCMC) method is asymptotically convergent for sampling from such a PPD. Unfortunately, MCMC methods based on Metropolis -Hastings or Gibss'sampler is computationally expensive for our problems. We have developed several meta-heuristics that offer practical ways for sampling from multi-modal PPDs. These include multiple very fastsimulate annealing (MVFSA) and multi-chain genetic algorithms. More recent approaches include Hamiltonian Monte Carlo and Langevin Monte Carlo methods, which make efficient use of local gradient information. Several examples of these methods from geophysical inverse problems will be discussed.

Determining Authorship: Criteria & Ethical N iceties .

Date
2013-03-20
Speaker
Dr. Ashima Anand
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Over the past three decades, I have been involved in various issues that come under the purview of “Universality of Science” which is a statute of the I nternational Council of Scientific Unions. These are ‘Freedom’ of scientists to engage in scientific activity with freedom of movement, association,expression and communication and ‘ Responsibility’ of scientists at all levels to carry out, communicate scientific work with integrity, respect, fairness trustworthiness. I would discuss the issue of communication of scientific work i.e., writing of scientific papers with respect and fairness. Appropriate authorship which involves granting due credit to those contributing substantially is an important aspect of this.

Colourful Story of Diamond: A Journey from Crown Jewel to Quantum Information Processing – Role of Spectroscopy of point defects

Date
2013-03-13
Speaker
Dr. M. D. Sastry
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Diamond with a sp 3 hybridized Carbon having tetrahedral structure, is a well known gem stone with many interesting physical properties. It is the hardest material with highest thermal conductivity and also has very high Debye temperature (2200K) resulting in low vibrational density of states. I n general, with an exception of nitrogen and hydrogen to a lesser extent, diamond does not contain chemical impurities . Diamonds with undetectable amounts of nitrogen are classified as type IIa and those with detectable amounts of nitrogen are classified as type Ia or Ib depending on the type of nitrogen aggregation. Among these, type Ia is the most commonly occurring form (~98%).Both type Ia and IIa type diamonds are colorless, and type Ib with isolated nitrogen impurity has a yellow color. Colouration can be induced and manipulated by electron beam treatment (EBT) followed by a thermal cycling . It is possible to produce attractive blue, pink and cognac colors by EBT and heat treatments. These colours are due to the stabilization of point defects consisting of a variety of nitrogen -vacancy complexes. Among these, negatively charged NV complex with zero phonon line at 637 nm has been found to be suitable for quantum information processing (QIP) at room temperature. It has been experimentally established that apart from NV - centre , centers such as SiV- and a nickel complex, termed as NE8, are also suitable as single photon emitters at room temperature and can be used for quantum information processing. The feasibility of quantum computation at room temperature using a highly stable material with optically and thermally stable centres holds a great promise for a practical quantum computer. The relevant aspects will be presented.

Ultrafast science: Adventures on the interface of physics, chemistry and biology

Date
2013-03-06
Speaker
Prof. Deepak Mathur
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Access to ultra short laser pulses that last long enough to accommodate only a few optical cycles, is beginning to allow time - dependent nuclear and electron dynamics to be probed within atoms and molecules, thereby enhancing our ability to gain proper insights into how quantum systems react to strong external fields and how they might be subjected to optical control. In this talk I shall present an overview of how we have utilized intense laser pulses of duration as short as ~4 fs to explore dynamical effects of relevance to diverse areas of the physical and engineering sciences, including applications pertaining to DNA damage, laser -induced materials modification and green photonics.

Challenges in Autonomous Robotics Research and its Applications

Date
2013-02-27
Speaker
Prof. Himanshu S. Mazumdar
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Androids and autonomous robots in popular films and fictions are far too smarter than the ones being developed in most advanced research labs. Most of us grew up watching “C3Po” and “R2D2” robots of “Star Wars”. General expectation from robot poses greatest challenge for researchers. Robotics research is evolving as one of the key science discipline of the 21st century. Complex robotic hardware is rapidly evolving with the availability of greater computational power, variety of integrated monolithic smart sensors and actuators. These advances in hardware, however, do not fulfill the expectation of desired intelligent performance without the matching advances in software like computer vision, natural language processing and computational intelligence. Disciplines like artificial life, cognitive science,neural networks, rule-based systems, behavior based control, genetic algorithms and other forms of evolutionary computation are being applied to evolutionary robotics to bridge the gap between hardware and software. The integration of mechatronics with computational power and artificial intelligence has created human- like androids, autonomous vehicles and planetary rovers. The techniques of mechatronics and robotics are being applied to other areas of engineering, sciences and medical applications, creating vast opportunities of new products. In recent past we have witnessed the real - life application of such devices like Da Vinci the surgical-robot in Britain, drones in Afghanistan,war-robots used in Iraq war. NASA’s Robotic Refueling Mission (RRM) is coming up with the capabilities of repairing and refueling dead satellites in space. Multi legged robots are being designed to explore terrains and hostile landscapes. Robotics is most popular among university students and hobbyists. It is one of the best sources of learning many technologies like mechanics, electronics, mathematics, control, software, computer vision and artificial intelligence. This colloquium will give an overview of the historical development of robotics highlighting few case studies and results.

Its time for time domain astronomy

Date
2013-02-20
Speaker
Dr. Ashish Mahabal
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Astronomy has come a long way from small-area focused observations of a small set of objects to panoramic, deep, multi-wavelength survey and has opened floodgates of discovery. This revolution has been enabled by faster computers, by the availability of larger and cheaper storage devices, and even more so by the advance in observing technology. Astronomy has moved from taking static pictures of the sky to digital movies that can be data-mined in a variety of ways. We present an overview of the field with a special emphasis on open surveys like Catalina Real-time Transient Survey (CRTS), modes of communicating information about transient events so that rapid follow-up becomes possible. Given the large number of transients we will soon be witnessing per unit time, deciding which transients are worth following up in detail for rarity or new physics is an important question. We present a few classification methods that can make this happen. Finally, we speculate on the crucial role that Indian observatories and institutes can play.

The Nitrogen Paradox

Date
2013-02-06
Speaker
Dr. Sanjeev Kumar
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Nitrogen is one of the most important elements for the sustenance of life. But as the saying goes, excess of anything is bad. This maxim appears to be particularly true for nitrogen as nutrient source in our ecosystems. In pre-human world, the dominant means by which nitrogen was accessible to living organisms in bio-available form was biological nitrogen fixation, where small number of microorganisms could fix atmospheric nitrogen. However, the script changed after the invention of the Haber-Bosch process (~1913), which enabled us to produce a rtificial fertilizer on commercial scale. Although this product of the Haber -Bosch process turned out to be the life saver for the ever increasing population of the world, it also led to degradation of the natural ecosystems due to excess nitrogenous nutri ents. During this colloquium, this basic paradox of nitrogen and related examples from the aquatic and terrestrial ecosystems will be discussed.

Low - dimensional Physics and Ordering in Nano - structured Materials

Date
2013-01-30
Speaker
Prof. Milan K. Sanyal
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Fascinating physical properties evolve in materials when it gets confined in any of the three physical directions. Ordering of materials and associated structures of electrons and spins can now be probed with desired accuracy to test theoretically predicted properties of one -and two-dimensional physics.We shall discuss here results of a series of synchrotron x -ray, neutron scattering and electronic transport property studies of nano -structured materials to understand these ordering processes. Inparticular we shall discuss long range ordering and crystallization of CuS during formation at Toluene-water interface and reversible crystallization of monolayer of Polyhedral Oligomeric SilSesquioxane (POSS) on bare water surface. We shall also discuss spin-ordering in two dimensional systems with vortex formation and electron ordering in one-dimensional nanowires that give rise to novel resistance-switching transition properties.

Charge Particle Nanotechnology [CHARPAN] - The New Frontier

Date
2013-01-23
Speaker
Professor Girijesh Kumar Mehta
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Nuclear accelerators provided the breakthrough to Si industry by introducing ionimplanters, and are providing ways to reduce the size of the transistor to nm range. Nano ion beams are opening new horizons in the nano-scale world and leading the industry towards futuristic technologies through Charge Particle Nanotechnology [CHARPAN]. The Proton Induced X-Ray Emission [PIXE] technique for Trace Element Analysis used in many disciplines is now being used for medical studies in human cells. Material is modified by ion-matter interaction. We can control the modification to the extent that either we change its property to the level we want or to the extent that we can destroy the material as done in ion- therapy to cure cancer. Ions of controlled energies and sizes are now opening up new horizon. It is possible to fabricate nanostructures by drilling/cutting with nano size ions or use bottom up approach by depositing nanosize particles. It is demonstrated that with ions we can make material with negative refractive index, make glass which can transmit light but not heat and other smart/intelligent materials.

Infrared Spectroscopy of Protostars with Spitzer & Herschel: Probing the earliest stages of stellar birth

Date
2013-01-16
Speaker
Dr. Manoj Puravankara
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Protostars are new born stars and represent the earliest stages of star formation. The protostellar phase is of fundamental importance as it is during this phase that the final stellar mass is determined and the protoplanetary disks, the birth places of planetary systems, are formed. And yet, protostellar evolution remains the least understood phase of star formation. The early evolution of protostars is driven by the competition between infall, accretion and outflows, processes that can heat up the surrounding gas to temperatures of several 100 K to several 1000 K. Many of the important cooling lines of the warm and hot circumstellar gas fall in the mid- and far-infrared wavelengths. These lines provide valuable diagnostics of the physical conditions (density & temperature), elemental abundance and spatial extent of the emitting gas, and, thereby offer vital clues on the heating mechanisms. Infrared spectroscopy, thus, is a powerful tool to study the energetic processes that shape protostellar evolution. We have analyzed 5-200 micron spectra of some 100 protostars from the nearby star forming regions, obtained with the Spitzer and Herschel space telescopes. The protostars in our sample span three orders of magnitude in luminosity and are in various stages of evolution; this is the largest such sample of protostars to date, for which mid- and far-infrared spectra have been obtained and analyzed. I will present our analysis and discuss our main results, which provide new insights into our understanding of the earliest stages of star formation.

Isotope tracing of contemporary and paleo-oceanographic processes in the Indian Ocean

Date
2013-01-09
Speaker
Dr. Sunil Kumar Singh
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Global ocean circulation controls the global climate and ocean productivity by transporting heat from equator to pole and by redistributing nutrient among different oceanic basins. Past ocean circulation has been influenced by tectonics and climate variability. As a part of GEOTRACES programme, efforts are being made to study the ocean circulation pattern, both contemporary and paleo, in the Indian Ocean using isotope proxies. In addition, suitability of these isotope proxies are also being tested and calibrated to study these processes. Studies carried in the Indian Ocean till now in this direction reveal few interesting facts which will be discussed in colloquium.

Structure of Sunspot

Date
2013-01-02
Speaker
Dr. Debi Prasad Choudhary
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Are the sunspots monolithic magnetic plasma tubes or collection of smaller tubes that would have gaps of field free material? This has been a question for more than 30 years. With the high spatial resolution images of the sunspots from ground and from space observatories, we can now attempt to answer this question. As sunspots are the sites of large explosive events that influence the near earth space weather it is important to understand their magnetic structure that govern their stability and decay process. In this lecture, the anatomy of sunspots derived using the observations with Hinode Solar Optical Telescope, a 50 cm optical telescope in space platform for solar observations, will be discussed.

Higgs Boson - Have we seen it?

Date
2012-12-26
Speaker
Prof. Sunanda Banerjee
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

The Standard Model of particle physics has been extremely successful in explaining all the precision data collected during the past few decades. The model, however, is incomplete with one of the key particles still not experimentally observed. This particle is predicted by the theory in the context of providing mass to the fundamental constituents as well as the exchange particles W and Z bosons. In the recent past, two experiments, ATLAS and CMS operating at the Large Hadron Collider, CERN have observed the evidence of a new state. Search signal of this object has been motivated by the Higgs boson within the Standard Model. Meanwhile, in the ~20 years since the inception of these experiments there has been a growing conviction that the Standard Model is not the end of the story. In this lecture the LHC physics program and some of the most important recent results including the discovery of a new Higgs-like particle will be presented.

The search for new light weakly-interacting particles

Date
2012-12-19
Speaker
Prof. E. Masso
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

New light particles that couple very weakly are a common feature of theoretical extensions beyond the Standard Model. This talk will review the current constraints (astrophysical, cosmological and from laboratory experiments) on such particles. It will also present the intense activity there is now on the experimental front in the searches for light weakly-coupled particles, with emphasis on the several laboratory experiments being either in progress or proposed.

Aerosols, Clouds and Rainfall

Date
2012-12-12
Speaker
Dr. S. Ramachandran
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Atmospheric aerosols can exert a cooling and warming on the Earth's climate through direct (scattering and absorption of solar and long wave radiation), semi-direct (evaporation of cloud droplets due to solar absorption), and indirect (modify the cloud optical properties, lifetime and albedo) effects. The concentration, size and composition of aerosols that can act as cloud condensation nuclei determine the cloud properties, evolution and development of precipitation. The indirect radiative effects of aerosols are more uncertain than the direct radiative effects of aerosols. The combined effects of aerosols produced by local and non-local (long-range transport) sources may alter the large-scale heating and induce changes in the general circulation of the atmosphere, thereby affecting the processes of cloud formation and rainfall. The inter-annual and spatial variations in aerosols and cloud characteristics, and their relation to rainfall in summer monsoon over India during the last decade which witnessed normal, drought and excess rainfall are examined. Results obtained on the aerosol-cloud-rainfall linkages over India and observational evidence for aerosol indirect radiative effects will be presented.

Is Interstellar Space Travel Possible?

Date
2012-12-05
Speaker
Prof. Ashok Singal
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Recently, India had successfully launched Chandrayaan - a mission to the Moon. A second mission to the Moon is already in the offing and there are plans for sending probes to other planets, e.g., Mars. Perhaps in a decade or so we may have a man landing on the moon. A few countries have already achieved this. After that one could imagine manned trips to other planets in the solar system. Pioneer 10 and 11, and Voyager 1 and 2 have already crossed the boundary of our planetary system and are still moving away. This begs the pertinent question: Could man possibly ever travel to distant stars? Of course the distances involved are immense. The nearest star (Proxima Centauri) is as many times farther (a hundred million times) than the moon, as the latter is compared to distance between adjacent rooms (4 m) in a building. Thus planning a voyage to a star will be “asking for the moon”, repeated 100 million times. With the maximum speeds achieved so far by space probes within the solar system, it will require about 85,000 years to reach Proxima Centauri, roughly equivalent to the time the homo-sapiens (humans) have been on the scene. Thus it may not look possible to reach even nearby stars within a human lifetime. To speed up, even just by an order of magnitude, by using conventional chemical propellants, would require fuel mass equivalent to that of a whole galaxy like our dear Milky-way. Various other alternatives and possibilities for interstellar space travel will be examined and discussed.

Multiscale Phenomena of the Earth’s Magnetosphere

Date
2012-11-21
Speaker
Prof. A. Surjalal Sharma
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

The Earth’s magnetosphere exhibits multiscale behavior, spanning a wide range of scales from the electron skin depth (~ km) to the global scale (200 RE ~105 km). On the largest scale the global simulations using the MHD model provide the dominant features of the macro-scale features. On the shortest scale the electron-MHD and PIC simulations provide the details of the processes, such as magnetic reconnection, that initiate the meso- and macro-scale phenomena. An integrated approach based on the two-fluid plasma model can provide a seamless description of the multiscale phenomena on the micro-, meso- and macro-scales, and can be a framework for the understanding of ESA/Cluster and NASA/MMS missions. On the other hand the recent approach of data-enabled modeling, based on the nonlinear dynamical systems theory, yields models which are independent of modeling assumptions and complements the numerical simulations. The capabilities of numerical simulations to yield physical insights and of the data-enabled approach to yield dynamical and statistical behavior complement each other and provide a framework for the understanding of multiscale phenomena in general.

Form and function of proteins. Historical background and the Indian effort

Date
2012-11-07
Speaker
Prof. M. Vijayan
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

The function and biological role of proteins, and indeed those of other biomolecules, depend upon their structure. The method of choice for determining the structure of biological macromolecules like proteins is macromolecular crystallography. Macromolecular crystallography had its origin when J.D. Bernal and Dorothy Crowfoot (subsequently Hodgkin) recorded the X-ray diffraction pattern from the crystals of pepsin. However, the first structures of proteins were determined only by around 1960. Since then the area progressed rapidly and the three-dimensional structures of thousands of proteins have been now determined. India had a head start in protein structural studies, with emphasis on computational biology, modelling and what we now call bioinformatics, thanks to the efforts of G.N. Ramachandran and his colleagues. The structure determination of the fibrous protein collagen, using modeling and fibre diffraction, and the construction of the Ramachandran map are the best known contributions of the Ramachandran group. However, experimental macromolecular crystallographic studies got off the ground in India, with the Molecular Biophysics Unit of the Indian Institute of Science, Bangalore as a national nucleus, only in the 1980s. Since then the work in the area in the country has grown to encompass thirty institutions and hundreds of research workers. It is now an important component of modern biological research in the country. The systems being addressed using macromolecular crystallography in India encompass a wide spectrum. The studies include a concerted effort on proteins from microbial pathogens, particularly TB proteins. The area is now poised to scale new heights and expand into activities such as structure-based inhibitor design directed towards drug development.

Nuclear Energy: Problems and Prospects

Date
2012-10-17
Speaker
Prof. R. Rajaraman
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Nuclear Energy has had a roller coaster history since its inception over 65 years ago, enjoying periodic revivals followed by setbacks – the most recent being the reactor disaster in Japan. In India too, our government’s ambitious nuclear program, while significantly boosted by the Indo-US nuclear Deal, has since run into some stumbling blocks. Questions persist among the lay public on whether nuclear energy is desirable. Unfortunately, an educated judgment on this is not easy. Issues of public concern—reactor safety, radiation hazards, disaster liability, the economics etc --- together with a minimal appreciation of the underlying science and technology, cover a wide spectrum of expertise, making the subject immensely complicated. In this lecture we will sketch the history and prospects of nuclear energy globally and in India and throw some light on its different facets.

Modelling proportionate growth

Date
2012-10-10
Speaker
Prof. Deepak Dhar
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

It is fascinating to see baby animals grow into adults. Understanding the development of different organs from a single egg cell has been the central problem in developmental biology for over a hundred years. However, there is a considerably simpler problem of understanding how a small baby animal grows to a much larger size. In the case of humans, the body weight increases by a factor of 30 or so. In the case of elephants, this factor is about 100. As the baby grows, different parts of the body grow at same rate. This is called proportionate growth. The recent work on a simple sandpile model where this feature comes out quite naturally from local rules, without fine tuning any parameter will be discussed. The patterns produced are composed of large distinguishable structures with sharp boundaries, all of which grow at the same rate, keeping their overall shapes unchanged. FIGURE: Proportionate growth shown in patterns formed in the growing sandpile by adding N particles at a single site on a background with all sites with height 2, for N = 4 X 104, 2X105, and 4X 105. Color code 0, 1, 2, 3 = R, B, G, Y

Infrared Studies of Recent Outbursts of Recurrent Novae

Date
2012-10-03
Speaker
Prof. N. M. Ashok
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Cataclysmic Variables with multiple outbursts in a human lifetime are known as Recurrent Novae (RNe). These outbursts are the product of thermonuclear runaway in the accreted material from the companion star on the surface of the white dwarf (WD). The outburst mechanism is identical to that of classical novae, but the presence of a high-mass WD (mass  1.3 Msun) and a high accretion rate result in short recurrence timescale. RNe, of which only 10 are known in our galaxy, are special because they are strong progenitor candidates of a class of objects which are vitally important cosmologically viz. Type Ia supernovae. The short recurrence time of RNe make them well suited to provide observational inputs and constraints to nova trigger theories. In recent years 3 recurrent novae have undergone outbursts : RS Oph in 1986, U Sco in 2010 and T Pyx in 2011. These outbursts were extensively observed from Mt.Abu Infrared Observatory. Some of the interesting results obtained from these campaigns will be presented.

Formation, structure and fragmentation dynamics of CO2q+ (q ≤ 3) ions due to impact of 12 keV electrons

Date
2012-09-26
Speaker
Prof. R. Shanker
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

The processes of dissociation of multiply charged molecules play important role in our planetary atmosphere and interstellar space. Such processes can be studied in greater detail by employing an ion momentum imaging spectrometer (IMIS). Recently, we have developed IMIS in our atomic physics laboratory at BHU and have used it to study the formation, structure and fragmentation dynamics of CO2q+ (q ≤ 3) ions due to impact of 12 keV electrons. In this talk, a brief account of fabrication of IMIS and its working principle will be presented. The absolute partial ionization cross sections of CO2 molecule are measured for impact of 10-26 keV electrons as well as the complete and incomplete Coulomb explosion pathways for CO22+ and CO23+ ions are identified and discussed. The kinetic energy release distributions of these precursor ions are determined. Also, the angular correlation studies are performed to infer the geometrical structure of the excited states involved. These studies yield the bent structures of the involved states for both precursor ions. The concerted and/or sequential nature of all the dissociation pathways is assigned.

Science and Exploration of Mars

Date
2012-09-19
Speaker
Prof. S. A. Haider, FASc.
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Mars has been explored by several spacecrafts such as Mariners, Vikings, Phobos, Mars Odyssey, Mars Reconnaissance, Mars Global Surveyor and Mars Express. We have been able to understand atmosphere, ionosphere and magnetic field of Mars from these missions in detail. However, there are several questions which are not known in the Martian aeronomy. ISRO and NASA are planning to explore aeronomy/atmospheric missions to Mars in November 2013. The objectives of these missions are to address key science questions on Mars’ upper atmosphere, ionosphere, solar wind interaction and escape to outer space. These missions will be helpful for the study of several key issues concerning the current atmosphere, ionosphere and their escape, existence of methane, planetary neutral corona and solar wind/ solar EUV interaction with Mars. This talk will present the science of future Mars missions highlighting the above points as well as unsolved problems in the Martian atmosphere.

Matter under extreme conditions

Date
2012-09-12
Speaker
Dr. Hiranmaya Mishra
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

Important progress in understanding the behaviour of hadronic matter under extreme conditions of temperature, pressure as well as external fields has been achieved by adapting techniques of condensed matter theory. Such extreme conditions existed during the evolution of our universe around microseconds after the big bang. Such conditions are also expected to exist in the interior of ultra compact astrophysical objects like neutron stars. Further, such conditions are also created in the laboratory during the experiments on relativistic heavy ion collisions. In the present colloquium I shall discuss our current understanding of such extreme matter regarding superconductivity in quark matter, hydrodynamics of hot matter following a heavy ion collision as well as phase structure of hot and dense matter in presence of strong magnetic field.

Geomagnetic storms, substorms and their effects on low latitude ionosphere

Date
2012-09-05
Speaker
Dr. Dibyendu Chakrabarty
Venue
K.R.Ramanathan Auditorium, PRL

Abstract

In the presence of suitable polarity of interplanetary magnetic field (IMF Bz), solar wind can break apart the terrestrial magnetic shield. This leads to perturbations in the magnetospheric and ionospheric electric field & current systems resulting into what is known as a geomagnetic storm. During geomagnetic storms, energy gets stored in the nightside magnetosphere and is released during or after the main phase of the storm. This also brings in modifications in the ionospheric currents and electric fields on a global scale. This is known as magnetospheric substorm. The polarity reversals in the IMF Bz, drastic changes in the solar wind ram pressure, etc. can trigger substorms. The relationship between storm and substorm is complex and one of the poorly understood areas in the field of space weather. While the electric field and current perturbations during storms and substorms are direct in the high latitude ionosphere, these are often indirect and delayed over low latitudes. However, there are circumstances when these effects reach low latitude ionosphere almost instantaneously as that in the polar ionosphere. Evidences will be shown that the signatures of these perturbations can be captured using thermospheric airglow emissions. In addition, it will be shown that these perturbations can alter the low latitude ionosphere significantly. These findings advance our understanding of low latitude ionosphere-thermosphere system.

Peculiar motion of the solar system from the sky brightness anisotropy

Date
2011-12-21
Speaker
Ashok K. Singal,
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

New aspects of solar coronal rotation

Date
2011-08-10
Speaker
Hari Om Vats,
Venue
K.R. Ramanathan Auditorium, PRL

Abstract

A principle of partial coherence in a synchrotron source

Date
2011-03-16
Speaker
Ashok K. Singal,
Venue
K.R. Ramanathan Auditorium, PRL

Abstract