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Simple remarks on the entropy
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Classroom Contents
Quantum Aspects of Black Holes - Lecture 1
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- 1 Start
- 2 Black holes are hot
- 3 Entropy
- 4 De Sitter temperature and us
- 5 Even though Hawking radiation has not been seen for black holes,
- 6 Area is decreasing. The and law ?...
- 7 Central Hypothesis
- 8 No statement about the interior. So far, just a statement about the exterior.
- 9 AMPS paradox
- 10 Why would we insist on the "central dogma" given the arguments against it?
- 11 Evidence in favor
- 12 If it is true, can we understand why it is true directly by following the rules of gravity in the bulk?
- 13 Black holes vs de Sitter
- 14 Geometry of an evaporating black hole made from collapse
- 15 Black holes and thermalization
- 16 Black hole as a "mesoscopic" object
- 17 Why it is tricky?
- 18 Can we test that the radiation is pure?
- 19 There are things that are more complicated
- 20 Much more difficult than evolving backwards in time!
- 21 A very important tool for recent developments
- 22 Fine grained gravitational entropy
- 23 Entanglement wedge
- 24 Tom Hartman will discuss this in more detail in his lectures...
- 25 Simple remarks on the entropy
- 26 The message is in the Hawking radiate
- 27 Entropy of quantum fields around the hori
- 28 Let's go back to the Schwarzschild solution
