Quantum Aspects of Black Holes - Lecture 2

Quantum Aspects of Black Holes - Lecture 2

International Centre for Theoretical Sciences via YouTube Direct link

ER = EPR

4 of 34

4 of 34

ER = EPR

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Quantum Aspects of Black Holes - Lecture 2

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  1. 1 Full Schwarzschild solution
  2. 2 What should we make of these?
  3. 3 Full Schwarzschild solution = entangled Sta Juan Maldace.
  4. 4 ER = EPR
  5. 5 Some interesting lessons
  6. 6 AMPS paradox
  7. 7 A side comment
  8. 8 Simple models
  9. 9 A particularly simple 2d theory of gravity
  10. 10 Nearly AdS2 gravity
  11. 11 Infinite number of other configurations with the same
  12. 12 A particularly simple 2d theory of gravity
  13. 13 Dynamics
  14. 14 Perturbative quantum gravity
  15. 15 This includes al perturbative gravity corrections.
  16. 16 End of lecture 1
  17. 17 Dynamics
  18. 18 [Demo]
  19. 19 Is this relevant
  20. 20 Gravitational interactions between highly boosted particles in flat space.
  21. 21 The main effect is a time delay.
  22. 22 There is an interaction between the infalling particles and the outgoing particles.
  23. 23 Chaos in classical systems
  24. 24 If we look at a thermal state,
  25. 25 Quantum mechanical system
  26. 26 Out of time order correlator
  27. 27 Operator growth picture
  28. 28 OTOC as the overlap between two states
  29. 29 OTOC = Scattering amplitude
  30. 30 Black holes are maximally chaotic
  31. 31 Q&A
  32. 32 Thinking about black holes inspiration for a bound that applies to any many body quantum system
  33. 33 Chaos in the S-matrix
  34. 34 Longer times

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