Quantum Aspects of Black Holes - Lecture 1

Quantum Aspects of Black Holes - Lecture 1

International Centre for Theoretical Sciences via YouTube Direct link

Entropy

3 of 28

3 of 28

Entropy

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Quantum Aspects of Black Holes - Lecture 1

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

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