An archive of all the talks conducted by the NAC.
Shapes, Structures and Randomness
November 11, 2023
Dr. Pravabati Chingangbam
Professor, Indian Institute of Astrophysics
Abstract
The talk will introduce morphological descriptors known as scalar and tensorial Minkowski functionals, and Betti numbers. They are geometrical and topological quantities that quantify the morphological information of structures. We will connect these quantities to random fields and discuss how they reveal the statistical nature of the fields. Lastly, some physical applications will be discussed.
Hunting low-frequency gravitational waves through Pulsar Timing Arrays: The role of Indian Pulsar Timing Array
July 29, 2023
Dr. Manjari Bagchi
Astrophysicist, IMSc, Chennai
We know that gravity is just the curvature of the spacetime. A mass curves the spacetime around it, and both massive and massless particles follow the curvature of the spacetime. Motion (translational, rotational or vibrational) of massive particles generate ripples in the spacetime or gravitational waves. Like electromagnetic waves, gravitational waves also have a wide range of frequencies. Gravitational waves of different frequencies are created by different sources āand we need different types of detectors to detect them. There is an innovative āmethod to detect low-frequency gravitational waves by using a number of undead stars as the detectors. These low-frequency gravitational waves are caused by mergers of supermassive black holes, and not only one mergers, many mergers resulting a summed-up background wave. As pulsars are the special type of undead star used for this purpose, we call such experiments as Pulsar Timing Array experiments. Presently, there are multiple Pulsar Timing Array experiments ongoing in various continents. These groups recently declared their results revealing a hint of the low-frequency gravitational waves. Indian Pulsar Timing Array (InPTA) is an Indo-Japanese collaboration performing PTA experiment using Indian telescope, the upgraded Giant Metrewave Radio Telescope. In the present talk, I will briefly discuss low-frequency gravitational waves, the basics of a PTA experiment, and the contribution of InPTA in this field.
Introduction to Solar Astrophysics
September 21, 2024
SriUma M Vittal
PhD Scholar (SEPS), NISER
Solar Astrophysics is a major discipline in Astronomy, where a lot of foundational physics concepts are applied to solve problems, and understand the star that makes our existence possible. This talk will attempt to introduce the flavour of the field, by giving a brief look at the Sun, how it is studied, and the kind of problems and active areas currently being worked on.
Huge Radio Telescopes and Where to Find Them
Vasanth Kashyap
Int. MSc. (Batch 19), SPS, NISER
This is a story that started as a casual tea table conversation in December 2023 and led to an oppurtunity to do some interesting observations using the latest upgraded GMRT radio telescope couple of weeks ago. This is a state of the art facility, comprising of 30 radio antennae, each 45 m in size spread over 25 kms at Khodad, Pune. I was at the facility for a few days and in this talk, I will discuss how exactly it all went about. The proposals, technical details, actual observations and the future of this project. This, I believe is just a step towards a bigger global project to build a "Faraday Telescope".
Formation of Giant Planets: Insights from Pebble Accretion
September 06, 2024
Anuja Raorone
Integrated M.Sc., IISER Pune
The formation history of Jupiter has been of interest due to its ability to shape the solar system's history. Yet little attention has been paid to the formation and growth of Saturn and the other giant planets. Through N-body simulations on a simple disk, we have explored the formation of these planets via pebble accretion. We conducted a statistical survey of different disc parameters and initial conditions of the protoplanetary disc to establish which combination best reproduces the present outer solar system. This talk will highlight key findings on the eccentricity and semi-major axis distribution of the giant planets and provide insights into their formation timelines.
Zooming in on Planetary birthplaces with ALMA
August 10, 2024
Parashmoni Kashyap
The origin of our solar system and the structure of planetary systems across the cosmos is a fundamental question in astrophysics. With over 5,000 exoplanetary systems discovered, none perfectly mirrors our solar system. In this talk, I will explore the journey of planetary system formation, focusing on the protoplanetary disk stage, where planets acquire their unique characteristics. I will highlight how molecular line observations using the Atacama Large Millimeter/submillimeter Array (ALMA) provide invaluable insights into these early stages, advancing our understanding of planetary origins.
Beyond the Visible: Exploring the Universe with Neutral Hydrogen
August 3, 2024
Tanya Tripty
Int. Msc. (Batch 23) (SPS), NISER
The formation history of Jupiter has been of interest due to its ability to shape the solar system's history. Yet little attention has been paid to the formation and growth of Saturn and the other giant planets. Through N-body simulations on a simple disc, we have explored the formation of these planets via pebble accretion. We conducted a statistical survey of different disc parameters and initial conditions of the protoplanetary disc to establish which combination best reproduces the present outer solar system. This talk will highlight key findings on the eccentricity and semi-major axis distribution of the giant planets and provide insights into their formation timelines.
My Research Experience during a Master's Project
April 6, 2024
Abha Vishwakarma
Int. M.Sc. (B19), SPS, NISER
For those of us who wish to continue down a path towards academia, somewhere along the way, we most certainly have to do a PhD. But do we have the right idea of what research feels like? That is the question I set out to answer when I chose to take a break for a year, not apply anywhere, and spend all of my time on one thing - my thesis. I had to re-evaluate my choices of being an academic. I worked on a thesis that was new in many aspects for my supervisor too, similar to a PhD. I learned many things, from how to think and approach a problem, how to deal with setbacks, how to organise my research, and so much more, and I believe I should talk about it. Personally for me, I was not aware of most of the things I will be talking about, so perhaps this discussion might be helpful to others too. A disclaimer is that it is my individual experience and might be a bit specific to Astrophysics-related research, but I will try to be as general as possible.
Navigating the Mysteries of the Sun through Physics
January 20, 2024
N Sneha
Int. M.Sc. (B21), SPS, NISER
The Sun, a celestial powerhouse, not only dictates the rhythm of our days but also holds the key to profound mysteries. Understanding its workings unlocks a treasure of scientific insights. This talk will cover: 1. Motivation to study this massive celestial object. 2. Brief introduction to solar observations. 3. An account of the Coronal Heating Problem. 4. Introduction to hydrodynamics (HD) and Magnetohydrodynamics (MHD). 5. Emphasis on two particular solutions to the Coronal Heating Problem: (a) Magnetohydrodynamics-wave driven Kelvin-Helmholtz Instability in Coronal Loops. (b) Ambipolar Diffusion in Solar Winds. 6. Simulations conducted and some results presented.
The Rise and Fall of Pluto!
January 13, 2024
Aniketh Nath
Int. M.Sc. (B20), SPS, NISER
We all have heard that Pluto was considered the ninth planet of the solar system, but now it is no longer a planet. The story of Pluto from its discovery to its enlistment under the category of a dwarf planet is an interesting one. I shall try to cover some aspects of this story backed by the theoretical notions that were at play at different events of this story.
Introduction to Cosmology
October 20, 2023
Abhinav Roy
Cosmology is the study of the physical universe and due to both theoretical and observational developments, it has made enormous strides in the past 100 years. Cosmology has answered age-old questions involving the universe's age, geometry, and composition. In this talk, we will see the journey of cosmology as a science, learn more about our universe, and discuss the efforts of a few to answer the questions of many.
Orbital Dynamics near Lagrange Points
October 14, 2023
Sri Uma Maheshwari
Int. M.Sc. (B22), SPS, NISER
Many satellites, such as Aditya L1 and JWST, are seated at specific vantage points in space called Lagrange points. This talk will go step by step through the process of finding a numerical solution to an analytically unsolvable physical problem and also discuss the orbits of known astronomical objects around these points.
Introductory Talk: An Introduction to Positional Astronomy
October 9, 2023
Gayatri P
When you look at the night sky, you are greeted with the familiar sparkling points of light situated on the surface of a vast sphere of which you are at the centre. But to make any astronomical observation, you need to know precisely where to look, that is, the location of celestial objects in our night sky. Spherical or positional astronomy is a sub-field of astronomy that deals with the directions in which these celestial objects are viewed and predicts how they vary over space and time. One of the most ancient forms of science, here we learn how to locate objects on the celestial sphere — as seen at a particular date, time, and location on Earth — just as we measure positions on Earth's surface by Latitude and Longitude. Along the way, we also will encounter certain astronomical phenomena observed on Earth.
Introductory Talk: An introduction to Astrophotography and the photo of the moon
Vishal Meena
Int. M.Sc. (B22), SCS, NISER
This talk will introduce the basics of astrophotography, with a focus on a photo of the moon that our club recently took. We will discuss the equipment and techniques that we used to capture the photo, as well as the challenges and rewards of astrophotography. The photo of the moon that we will be discussing is a high-resolution image that was taken using a telescope and a specialized sensor. The photo shows the moon in stunning detail, including its craters, mountains, and valleys. We will discuss how we captured the photo and how we processed the data to achieve such high quality.
Introductory Talk: Search for water in the Universe
Asmi Nandy
For the longest time, we have been curious about the existence of life beyond Earth. Are we really alone in the Universe? This is a question we have been asking ourselves for quite some time. Water is supposed to be the a priori requirement that enabled life to evolve on our planet. It makes sense thus that we look for it elsewhere in the search for our brethren in space. How do we look for water, then? What are the processes used to detect its presence someplace millions of light years away from us? And how successful have we been in our search until now? Join us for the discussion session to find out!
Laboratory astrochemistry techniques for investigating kinetics of reactions in space
September 9, 2023
Aditi Pradhan
Int. M.Sc. (Batch 19), SCS, NISER
Over 200 species have been detected in the cold, neutral regions of the ISM over the past 80 years. The existence of such a rich and diverse range of chemistry even at very low temperatures and densities, raises several interesting questions about the origin of these species and how the energy barrier for reactions is surpassed at such low temperatures. The hunt for answers has led to the highly interdisciplinary field of Astrochemistry. Astrochemistry proceeds on 3 interlinked fronts, namely - observations, modelling and laboratory experiments. Laboratory astrochemistry is central to enhancing our understanding of the present composition of ISM, as well as the chemical origins of the universe. Laboratory spectroscopy aids observations in confirming the detection of new species in space. On the modelling front, parameters such as rate constants and branching ratios are required and can only be measured experimentally. The measurement of these parameters in a laboratory while mimicking the conditions in space, is a multi-fold challenge. This has led to the development of several novel experimental techniques, and innovative combinations of existing methods. The aim of this talk is therefore, to highlight the various experimental techniques involved in laboratory astrochemistry. More specifically, I will be discussing the novel CRESUCHIRP apparatus developed by Dr. Ian Sims and his group at the University of Rennes, where I worked over the summer.
X-Ray Binaries and Use of MESA
September 2, 2023
Pulkit Ojha
Research Assistant, IMSc, Chennai (B18 Alumni)
Binary stars, comprising more than 90% of the stars we see in our night sky, play a significant role in all kinds of astrophysical research. A peculiarly interesting category is x-ray binary, which happens to have compact stellar remnants, specifically a neutron star as one of their components. X-ray binaries act as space-based laboratories, allowing us to study the physics of accretion and the neutron star with good proximity observations. They also serve as progenitor systems to some exotic objects like millisecond pulsars and ultra-compact binaries releasing gravitational waves. For more than a year now, I've been working on modelling a class of such X-ray binaries using tools like MESA(Modules of Experiments in Stellar Astrophysics), the state-of-the-art Fortran-based 1D stellar simulation package. In the talk, I plan to start with a discussion about different classes of X-ray binaries and their wide applicability in astrophysics in the first part. Secondly, I'll present a small overview of my thesis work and the significance of such theoretical studies. I'll conclude the talk by talking about MESA, why it is important for anyone interested in working in astrophysics and how to use it as a beginner.
Magnetic Field of Stars
August 19, 2023
Monu Kumar Choubey
Int. M.Sc. (Batch 20)
In this talk, I will introduce the study of magnetic field of stellar bodies, including their origin, modeling, observation and interpretation. There's a special focus on Sun and sun-like stars, extending to white dwarfs and other stellar bodies. Lastly, there's brief mention of exotic bodies like neutron stars and magnetars.
The Ballet of the Medicean Stars
August 12, 2023
Shreya Jay & Samarth Mohan Nanjannavar
The main aim is to find out the time-period of 4 bright moons of Jupiter (IO, Callisto, Ganymede, and Europa) on pure experimental background i.e., without using any theoretical knowledge. We present to you the first experiment that the NAC Experimental team undertook. This was first done by Galileo. The problems encountered during the data analysis were versatile. The logic and method of solving the problems encountered is especially emphasised upon. Further we also used the data to find the mass of Jupiter using some basic literature on the topic.
A Misty Mystery: Unraveling Cloud Formation in Alien Skies
April 22, 2023
Rahul Arora
Int. MSc. (Batch 18), SEPS, NISER
Cloud formation plays a key role in the atmospheric dynamics of exoplanets, which can significantly impact their overall climate and habitability. This makes understanding of cloud formation and evolution in exoplanetary atmospheres very critical for interpreting observational data and characterizing these faraway worlds. In this talk, we will explore the various physical and chemical processes that contribute to cloud formation on exoplanets, such as condensation, nucleation, and growth. We will also discuss how cloud properties such as composition, size, and distribution can vary depending on the specific environmental conditions of the exoplanetary atmosphere, such as temperature, pressure, and atmospheric composition. In the end, we will review the current theoretical approaches for studying cloud formation in exoplanets and their impacts on observational interpretation and highlight some of the key challenges and open questions in this rapidly-evolving field of research.
Thinking Prebiotically: The study of Chemical Origin of Life and its Astronomical Implications
March 25, 2023
Adesh Natthuji Thawale
Int. MSc. (Batch 18), SCS, NISER
One of the leading theories for the origin of life is the Chemical Origin of Life, which involves mixing and matching simple molecules to form complex ones. Think of it like a giant chemistry experiment, but instead of baking a cake, we are trying to create life. But if you're feeling adventurous and want to explore more before the talk, we've got some papers at the end that will give you a deeper dive into the topic. Who knows, you might even find your calling in life (pun intended) and become a Chemical Origin of Life researcher. So, join us for a discussion that will be equal parts informative and entertaining. Let's get to the bottom of how life began!
Keep Calm and Let The Planets Form
January 28, 2023
Baibhav Srivastava
IISER Berhampur, Batch 18
By now you all surely know that planets form in disk-like structures, called protoplanetary disks, around young stars. But how exactly?
How did our Earth and Solar system form?
January 21, 2023
Prathap Rayalacheruvu
Our Solar System is believed to have been formed about 4.6 billion years ago in a cold molecular cloud. Its origin and evolution are still a mystery. The present state of planetary bodies, including our own Earth and the life on it are the direct result of various evolutionary processes that these planetary objects have gone through during these many years. Now the question is “Can we trace down the evolutionary processes of the planetary bodies and understand how life came about on planets like our Earth?” In this talk I will introduce you to some astrochemical tools which go a long way in addressing the above question.
Alien worlds in the JWST era: No more a Science fiction
January 14, 2023
Priyankush Ghosh
Ever since humanity has existed, it has looked into the night sky and wondered “Is there life elsewhere in the universe?” and “How did our Earth and other planets form and evolve?” Exoplanetary science, a new interdisciplinary field that emerged 25 years ago has the capability to answer just that. This talk involves basic introduction to the far away alien worlds, why are they so interesting, how to find them, what are the current research works going on in the field and what future beholds. I will also discuss how to decode an exoplanet spectrum to search for signs of alien life and its implication with respect to current research.
Surfing through Exoplanets
November 12th, 2022
Chandan Kumar Sahu
Int. M.Sc. B19 SPS, NISER
In this vast universe, it is inappropriate to think that Earth is the only planet sustaining life. So, are there really planets outside our solar system that can host life? Billions are spent every year on detection and study of planets which can possibly host life. This talk will be an introduction to the basic methods that are used in the modern era for detection of exoplanets and studying them. I will also hover over the different types of exoplanets and some of their properties. At the end, I will briefly mention current research in the field of exoplanetary systems.
Determination of Solar offset using Cepheids
November 5th, 2022
Swaroop R Averesekar
The sun's galactocentric radius (RGC) is previously calculated and known. It has also been established that our sun is not located precisely on the galactic plane but is slightly displaced. Previous estimates have calculated this solar offset (z) using sources such as OB stars, young open clusters (YOCs), pulsars, Etc. The right ascension and declination of Cepheids, obtained from The Optical Gravitational Lensing Experiment (OGLE) catalog cross-matched with the GAIA mission's - DR3, provides a way to calculate the z. This talk will give a quick tour into Cepheids, the data, and visualize the sun's coordinates in the milky way galaxy.
Introduction to Cosmology: A chronology of the Universe
October 15th, 2022
Soham Bannerjee
PhD, SPS, NISER
Observational Cosmology has come a long way. The Cosmological Principle states that the Universe is spatially homogeneous and isotropic on the largest scales. Hubble's data indirectly proved this principle when he found the relation between the speed and distance of galaxies. The Big Bang model has been widely accepted, which claims that the Universe evolved from a fireball that eventually cools to the structures we see today. Peebles suggested radiation from the early Universe, which was discovered by Penzias and Wilson, as the cosmic microwave background, which gives a compelling foundation for this model. In this talk, the speaker gave an overview of the formation of light nuclei(big bang nucleo-synthesis), recombination(formation of first atoms), the radiation from the early Universe(CMB), and large-scale structure formation.
Introduction to Cosmology: Why is the night sky dark?
September 4th, 2022
Int. M.Sc., B19 SPS, NISER
The night sky appears very different from the earth or the solar system. At a very large scale, large enough to contain many, many galaxy clusters, our universe looks and behaves very differently compared to solar systems, individual galaxies or even clusters of galaxies. Gravity doesn't seem to work according to Newtonian principles. A new theory of gravity, the General Theory of Relativity, formulated by Albert Einstein, sheds light on our understanding of the large-scale universe. In this talk, I will take you through the history that led to the birth of Cosmology, the study of the nature of our universe. I will then develop the notion of 'curvature of the universe', discuss how it can be measured and discuss its implications on the notion of distance between any two points in the universe. This talk covers the prerequisites required to understand the Friedmann equations and the governing equations of the universe's evolution, which will be covered in the next talk. The goal at the end will be to have an interactive talk, where I will simulate universes with different densities of matter, radiation etc. using python and see how it evolves with time.
Stellar Astrophysics II: Classification and Evolution of stars
August 27th, 2022
Vasanth Kashyap, Pulkit Ojha
Int. M.Sc. B19, SPS, NISER, Int. M.Sc., B18 SPS, NISER
In the last talk on stellar astrophysics, the basics of stellar structure and the origin of stars was covered by Vasanth. In the upcoming talk, the classification of stars based upon their spectral luminosity will be discussed and if time permits, we'll also try to present a basic overview of stellar evolution. This talk may be followed by a demonstration of stellar evolution using MESA.
Stellar Astrophysics: Origin, Structure and Classification
August 20th, 2022
This is the second talk in the 'Stellar Physics Triad'. In this talk I hope to glance over the fundamentals of stellar astrophysics. Topics of star formation, stellar structure and spectral classification shall be discussed along with their underlying principles with sufficient mathematical detail. It will be followed by brief discussions on Hertzsprung Diagram and Morgan Keenan Luminosity Classes.
The Solar Cycle, Magnets, and More
August 13th, 2022
Ratul Das
Int. M.Sc., B20 SPS, NISER
The Babcock-Leighton model of the solar dynamo is often noted as the most accurate qualitative mechanism for explaining the Solar cycle, despite being initially formulated about 70 years ago, when only terrestrial data from the Sun was available. It successfully explained how and why sunspots form, along with the relation between the oscillatory 22-year Solar cycle and the evolution of the magnetic field (basically, a whole backflip) of the Sun.
Birth of Cosmology
April 23rd, 2022
Int. M.Sc. B20 SPS, NISER
Cosmology is the study of the physical universe and due to both theoretical and observational developments, it has made enormous strides in the past 100 years. Cosmology has answered age-old questions involving the universe's age, geometry, and composition. In this talk, we will see the journey of cosmology as a science and the efforts of a few to answer the questions of many.
Solar Storms
December 24th, 2021
Monu Kumar
A solar storm is a blanket term for events of solar disturbance, emanating outwards from the heliosphere, leading to various effects. I will talk about the origin of these events at the sun, shedding some light on our understanding of them and how we have come to such an understanding. We will also explore why these events are interesting and important, in various contexts. Lastly, I will try to give some insight into its effects on the earth and future frontiers.
Sun : The Literal Star of our Solar system
October 23rd, 2021
Swosti Prakash Sarangi
More often than not, we are ignorant to things that are closer to us. One such thing is the Sun. No matter how much we know about it already, it never fails to surprise us. In this talk, I will try to present the different shades of the Sun, explain the physics behind them and use the Sun as a subject to gain some useful insights into stellar astronomy. Also, I shall share some of the mythical tales surrounding the Sun. Towards the end, I shall discuss some paradoxes and open problems in the field of solar physics.
A brief Overview of Digital Imaging
June 12th, 2021
Int. M.Sc. B18 SCS, NISER
Image sensors are probably one of the most commonly used sensors in the entire world, yet very few people realise the complex process that goes into creating the image that they see after pressing the sensor button in the camera app of their smartphones. In the first session of the Image Processing Workshop, attendees will be taught about the characteristics of image Sensors and Images. The goal of session 1 is to familiarize the attendees with the process that goes into creating a digital image from modern sensors, so that they will better understand the processes that go into image processing. At the end of the session the attendees will be taught how to create star trails using just their phones and a simple software (StarStaX).
Diving into the surreal field of Exoplanets
Akshay Priyadarshi
Int. M.Sc. B16 SPS, NISER
Being a common occurrence in pop-sci and also at the home of crazy theories, the field of exoplanets does enjoy quite some attention. But have we ever looked at their importance beyond the wow factor? How "studying others to understand ourselves" could really be a thing!? In this talk, we'll start with an introductory know-how of the field, understanding the motivation and how exoplanets can be studied in exquisite detail despite being so small and so far! And the huge range of interdisciplinary research possibilities that lie ahead.
Perseverance; a big leap towards MARS
March 19th, 2021
Aheesh Chandrakant Hegde & Chandan Kumar Sahoo
In this talk, we will "explore" the Mars 2020 mission, the Perseverance rover and some of its onboard instruments it will be using for Mars exploration and also have a short but detailed description of 'Ingenuity - the Mars helicopter'; to entertain ourselves with the joy of knowing the latest probe on the red planet and the technicalities involved in the mission.
Ancient Astronomical Calculations
March 1st, 2021
Nisarg Vyas
Int. M.Sc. B17 SPS, NISER
Sure, you would have heard of Jantar Mantar. Ever peeked into the details of what instruments do they house, and what did it mean at the time of their inception to have such instruments? As a fun read, I would like you to look up about the Jantar Mantar at Jaipur. The image attached with the mail shows a model of the same, try finding out what's what. From Greek astronomer and mathematician, Ptolemy, to the Rajput king Sawai Jai Singh II, we will cover a wide period of the history of astronomy of our Sun. We will explore how the ancients calculated the Sun's rising times without the aid of spherical trigonometry. In this talk, I will try to get you started to do basic calculations in astronomy.
Evolution of our models of the Universe
September 5th, 2020
Sagar Shrivastava
(B11 SMS, NISER), Ph.D. student at TIFR, Mumbai
Humans have been fascinated by the twinkling lights in the night sky, and have been trying to give a reason for why they are there. Whether it's the ancient Mayan with their flat earth theory or the Greeks with their geocentric theory of the universe, there have been many models of the universe, and as we are able to understand more about the fundamental forces of our universe, we have been able to get a clearer picture. This would be an introductory talk with more focus on how progress in science was able to change our view of the universe.
Mapping the Universe using Sky Surveys
August 29th, 2020
Biprateep Dey
(B13 SPS, NISER), PhD student at University of Pittsburgh.
Astronomical surveys are used to map the universe along with discovering new phenomena. Past surveys like the Sloan Digital Sky Survey have significantly improved our understanding of the universe. We will talk about some upcoming sky surveys like the Dark Energy Spectroscopic Instrument (DESI) and the Rubin Observatory Legacy Survey of Space and Time (LSST). We will explore the wide range of science that can be done with these instruments and why and how you may consider doing PhD research in Astronomy.
Inflation, Quantum Fluctuations, and Primordial Black Holes
August 22rd, 2020
Swagat Saurav Mishra
(Batch 08, SPS, NISER), SRF at IUCAA, Pune
Black Holes are extremely dense gravitationally bound objects that are usually formed via the gravitational collapse of matter during the end stages of big stars. Such black holes, which are end products of stellar evolution, are known as Astrophysical BHs. Scientists have directly and indirectly established the existence of many astrophysical BHs of mass ranging from 10 solar mass to about several Billion solar masses. There are other types of black holes, known as the Primordial Black Holes (PBHs) that are formed in the early universe, during the hot Big Bang plasma state, long before the formation of any stars. We can refer to them as BHs from the Big Bang. Their masses could be as small as the mass of stone, unlike the astrophysical BHs. The speaker will discuss the significance of PBHs in addressing several issues in Cosmology, from Dark Matter to the existence of supermassive BHs to Hawking Radiation.
CMB Temperature Power Spectrum
May 8th, 2020
R Vasanth Kashyap
Int. M.Sc. B19, NISER
In this talk, I would like to take the audience into an understanding of the methods that enable us to move from the high uncertainties of cosmology to that of precision cosmology. All from the cosmic microwave background radiation. Understanding the CMB is possible by knowing what happened since the big bang to the creation of the CMB. How do we know the composition of the universe? How do we extract information from the fuzzy-looking cosmic microwave background? What information does this earliest snapshot of the universe contain? We would start with a brief introduction to The Big Bang model and inflation and how inflation explains the isotropy in the universe, which is observable in its current state. Later we would indulge ourselves in understanding the first notes of music in the universe, called the baryon acoustic oscillations. Further getting into the details of the CMB, a particular plot of the cosmic microwave background called the Power Spectrum is obtained, revealing all the secrets of the CMB. This eventually leads us to the results that are widely seen today about the constituents of the universe as 70% Dark Energy, 25% Dark Matter, and 4% Matter that we normally interact with.
Orbital Mechanics
April 23rd, 2020
Karan
Things in orbit don't behave in the most intuitive manner. In this talk, we will go over the basics of the rocket equation and how to calculate delta-v budgets. We will intuitively see how rockets launch and manoeuvre in orbit. All this will be done using the legendary video game 'Kerbal Space Program'.
The History of Measurement of the Speed of Light
February 15th, 2020
Abhipsa Mishra
Int. M.Sc. B18 SPS, NISER
With the values of myriads of fundamental constants of the Universe at a click away we sometimes lose contact from Newton's wise words, "We are standing on the shoulders of giants". So, on February 15, 6:30 pm, 2020, we shall pause to look down at those strong shoulders and try understanding the roots and tips of the quest for measuring the speed of light, a param fundamental constant. We shall have our humble beginnings at the naïve insights of the olden days and carry on to notice how the progress of technology and polishing of the human mind has helped us chase the value of speed of light to what we believe to be it's truest value.
Cosmological expansion and You
February 1st, 2020
Akshay Priyadarshi and Karan
Int. M.Sc. B16, B17 SPS, NISER
Taking off from the topic of curvature, we delve into its implications in the real universe. Then, using a simple Newtonian approach, we derive the Friedmann equation, which relates the expansion to the energy and curvature of the universe. The equation is further used to model different versions of the universe, which gives us a perspective on the current observations. Finally, we introduce the mysterious Lambda to get an even more consistent model of the universe.
Straight Paths in Curved Spaces.
January 15th, 2020
Pushpak Pandey and Renu Raman Sahu
Int. M.Sc. B15 SPS, NISER
We know that light travels along a straight path, but is 'straight' what we know it to be? What does the space-time being flat or curved mean? We shall explore these questions and discuss the notion of distance and curvature in a few simple geometries. We shall apply these ideas to find out the type of geometry we live in.
Tic Tac Toe Cosmology
January 18th, 2020
Nisarg Vyas & Chandranathan
Questions regarding our place in this vast object called universe are known to have invoked serious considerations about our understanding of it. We explore some of the school of thoughts in the talk. Translating the ideas of the talk in the language of mathematics flavoured with some infinities and observations, the talk, in itself, is complete! Borrowing rigour, contemplation and aesthetic from philosophy and science alike, we, sitting on the shoulders of giants, embark on a journey to the centre of the universe.
The Story Behind the First Image of a Black Hole
January 11th, 2020
Dripto Biswas
Last year, the scientific community was shown the first image of a black hole. In this talk, we will review the basic physics of a black hole, and why it is difficult to capture one using standard imaging techniques. We will also take a quick look at Very Long Baseline Interferometry (VLBI), which was the principle behind the Event Horizon Telescope. Finally, we will compare the image with the existing models of a black hole , and try to identify various components of the same.
Life on Mars
August 25th, 2019
Kanishk Kumar
Int. M.Sc., SBS, NISER
Life on other planets has always been a fascinating endeavour for humans. But it doesn't necessarily mean extraterrestrial life or as we fondly call them, aliens. It also means exploring the possibility of settling human life on other planets. Our best possible candidate for this is Mars. This planet has been well explored, with respect to other planets and will be at the focus of several missions in the future as well. I will explain the current understanding of the situation of establishing life there, as well as future possibilities. Hopefully, it won't break marriages of the Indians who settle there ;-).
Climbing the ladder of cosmos
August 24th, 2019
Chandranathan and Nisarg Vyas
This elegant universe instils awe in all of us. Inquiring minds often ponder about their place in this big "mess". In this talk we will, step by step, climb the ladder of the cosmic distances. For a start, using only a ruler and a protractor we will see how far we can go. Then with the understanding of light, we will climb a step further and fathom the cosmic 'depths'.
Virtual Astronomical Observatories
February 2nd, 2019
Satyam Chandra Mishra and Anshuman Padhi
Int. M.Sc. B15 & B18 SPS, NISER
In an extension to the last week's NAC series talk, this time we will learn how to analyze the data collected from the telescopes. For this, we will use Virtual Educational Observatory (VIREO) which is a simulated observatory and can access a huge database of astronomical information, both through a set of dedicated catalogues and via online databases. It also simulates a very large and diverse sample of the observable astronomical sky, as seen with optical and radio telescopes, and thus can be used to carry out a wide variety of realistic observing projects. We will start by discussing Kepler's Laws and see how we can use them to predict the mass of the Jupiter, by observing its moons. I'll then present the basics of pulsar observation and explain the signal extraction technique from simulated noisy data.
The theory of Special Relativity
October 6th, 2018
Ashish Mishra and Debaiudh Das
The Continuous Spectrum of Light
September 3rd, 2018
Dhanush S
The Cosmic Distance Ladder
August 18th, 2018
Karan and Manabputra
Int. M.Sc. B17 & B16 SPS, NISER
The Celestial Sphere
August 10th, 2018
Akshay Priyadarshi and Nisarg Vyas
Int. M.Sc. B16 & B17 SPS, NISER