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Degenerate Bose Gas
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Classroom Contents
Maximum Mass of Neutron Stars - Lecture 8
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- 1 AM
- 2 Neutron Stars and Black Holes Lecture - 8: Maximum mass of Neutron Stars
- 3 Lev Landau
- 4 Landau invents neutron stars in 1938
- 5 Neutronization of matter at high density
- 6 J. Robert Oppenheimer
- 7 The maximum mass of neutron stars
- 8 A fully relativistic WD has no radius! But it has a unique mass!
- 9 The Maximum Mass for Neutron Stars
- 10 Tolman, Oppenheimer, Volkoff equation
- 11 Oppenheimer - Volkoff Equation of State
- 12 Oppenheimer and Volkoff, 1938
- 13 Limiting Mass for Neutron Stars
- 14 Ideal Fermi Gas
- 15 Why are there only two classes of 'cold stars'?
- 16 Stability of Matter
- 17 HW: Harrison - Wheeler Equation of State OV: Oppenheimer - Volkoff Equation of State
- 18 Minimum mass of neutron stars
- 19 Why is there a minimum mass?!
- 20 There are only two types of cold stars in nature!
- 21 Upper limit to the mass
- 22 Uniformly rotating stars
- 23 Exotic states near the centre?
- 24 Bose - Einstein Statistics
- 25 Bose-Einstein Condensation
- 26 Degenerate Bose Gas
- 27 Bose-Einstein Distribution
- 28 Quark - Gluon soup?!
- 29 Gravitational Mass versus Central Density.
- 30 Harland Snyder - a very special student!
- 31 Implosion of a star in General Relativity
- 32 The implosion of a star
- 33 Inside the Black Hole?
- 34 Next Lecture - Neutron stars in Binary Systems
- 35 Q&A
