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Lecture 31 - Supernovae and Cosmic Rays
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Astronomy and Astrophysics - An Introductory Survey, A lecture series by Prof. G. Srinivasan - Lecture 31 - Supernovae and Cosmic Rays

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What you'll learn

Analyze data using Python pandas and NumPy libraries
Build responsive web interfaces with React and Tailwind CSS
Implement user authentication with JWT and OAuth 2.0
Deploy containerized applications using Docker and Kubernetes

This course includes

  • 47 hours of video
  • Certificate of completion
  • Access on mobile and TV

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AstroPHYSICS with Srini (https://www.youtube.com/@astrophysicswithsrini1094) The newly launched youtube channel of Prof. Srinivasan. WATCH it, SUBSCRIBE to it, and bring it to the attention of your friends! And here is why. The present course of introductory lectures will end with the 41st lecture. There are many topics in basic physics, as well as astrophysics, that you encountered in this course that deserves a 'revisit'. Prof. Srinivasan plans to make new videos on these topics and upload them to this channel. This will start to happen after the last lecture of this series has been released. Meanwhile, this channel is up. Currently, the PLAYLIST contains the 40 lectures that he delivered at the International Centre for Theoretical Sciences, a few years ago. You are welcome to contact Prof. Srinivasan at [email protected] if you have suggestions for topics, or if you have questions. -------------------------------------------------------------------------------- Cosmic rays were first observed by Victor Hess in the early 20th century. A century later, the first direct evidence that galactic cosmic rays are accelerated within supernova remnants has been provided by observations by the Fermi Large Area Telescope collaboration. ABOUT THE LECTURE Supernovae are explosions of stars. Broadly speaking, there are two types of supernovae, (i) Explosions of massive stars, and (ii) Explosions of White Dwarfs. The classification of supernovae into various ‘types’ is based on their “light curves”, as well as the elemental abundance in the ejecta. In this lecture, I explain why a massive star explodes, and the presently accepted mechanism of the explosion. We will also discuss the explosion of a white dwarf star when it accretes mass and is pushed over the Chandrasekhar limiting mass. Supernovae and their remnants are important ‘accelerators’ of cosmic ray particles. We shall discuss this also. ABOUT THE LECTURE SERIES This lecture series is organized by the Astronomical Society of India as a part of its Golden Jubilee celebrations. Aimed at undergraduate and graduate students, this series of talks by renowned astrophysicist and teacher, Prof G. Srinivasan, starts from the first principles of Physics and builds up the subject rigorously to the present state of our understanding. Series website: https://astron-soc.in/srini-ana The website hosts a question bank as well as a list of suggested reading for each lecture (prepared by Dr. Sushan Konar) ABOUT THE SPEAKER Professor G. Srinivasan In a research career spanning more than five decades, his interests have spanned many aspects of physics and astrophysics. He is a passionate teacher and has authored two outstanding Astronomy texts titled ‘What Are The Stars?’ and ‘Can Stars Find Peace?’ He is a Past President of the Astronomical Society of India, and a Past President of the Division on Space and High Energy Astrophysics of the International Astronomical Union. In his distinguished career he has worked at the University of Chicago, USA; the IBM Research Laboratory in Zurich, Switzerland; Chalmers University of Technology, Goteborg, Sweden; the Cavendish Laboratory, University of Cambridge, England and the Raman Research Institute, Bengaluru Follow us on social media at https://twitter.com/asipoec https://www.facebook.com/asi.poec/ This series is also supported by the IAU OAE Centre in India https://twitter.com/astro4edu_India https://www.facebook.com/OAE-Center-India-105698322030674

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