Supernovae and Neutron Stars Lecture 06 by G Srinivasan

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Time: 10:00 AM • Venue: Ramanujan Lecture Hall / Madhava Lecture Hall, ICTS Campus, Bangalore • This summer course aims to give a broad perspective on gravity, astrophysics and cosmology and is suitable for advanced undergraduates and graduate students in physics and astronomy. Professor G Srinivasan is a specialist in Condensed matter Physics and Astrophysics and is an excellent teacher. After acquiring his PhD from the University of Chicago in 1970, he had a distinguished career as a scientist and teacher at the IBM Research Laboratory, Chalmers University of Technology, University of Cambridge, and Raman Research Institute. He has done pioneering work in condensed matter physics and astrophysics, and is the author of the best selling popular science books “What Are The Stars?” and “Can Stars Find Peace?”. • Topics: • L1 : Einstein's Theory of Relativity • L 2 : Principles of Radiative Transfer • L 3 : What are the stars? • L 4 : The solar neutrino puzzle. • L 5 : White Dwarfs as Quantum stars. • L 6 : Neutron Stars. • L 7 : Pulsars • L 8 : Black Holes I • L 9 : Black Holes II • L 10 : Between the stars. • L 11 : Supernovae • L 12 : Contemporary Cosmology I • L 13 : Contemporary Cosmology II • URL: https://www.icts.res.in/courses/summe... • Table of Contents (powered by https://videoken.com) • 0:00:00 A Journey through the Universe • 0:00:08 Supernovae and Neutron Stars (Lecture - 06) • 0:00:42 Guest Stars • 0:12:03 Supernova Explosion • 0:14:32 Between 1932 and 1937: • 0:15:18 Lev Landau • 0:18:37 Landau invents neutron stars in 1938 • 0:20:24 Protons + electrons • 0:23:07 Dynamical instability • 0:26:36 Stability of Matter • 0:32:26 J. Robert Oppenheimer • 0:33:57 The Maximum Mass for Neutron Stars • 0:37:25 Tolman, Oppenheimer, Volkoff equation • 0:40:36 OV: Oppenheimer - Volkoff Equation of State • 0:40:57 Oppenheimer and Volkoff, 1938 • 0:45:43 The Maximum Mass for Neutron Stars • 0:47:30 Oppenheimer and Volkoff, 1938 • 0:49:56 The fate of massive stars • 0:51:13 Condition for degeneracy • 0:58:01 Radiation pressure and Degeneracy • 1:08:56 Chandrasekhar, 1932 • 1:13:20 Oppenheimer - Volkoff Equation of State • 1:14:54 Stability of Matter • 1:15:20 HW: Harrison - Wheeler Equation of state OV: Oppenheimer - Volkoff Equation of State • 1:16:37 There are only two types of cold stars in nature! • 1:18:21 Q A

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