the black hole interior in ads cft
play

The black hole interior in AdS/CFT Kyriakos Papadodimas CERN and - PowerPoint PPT Presentation

The black hole interior in AdS/CFT Kyriakos Papadodimas CERN and University of Groningen Strings 2014 Princeton based on work with Suvrat Raju: 1211.6767, 1310.6334, 1310.6335 + work in progress, with Souvik Banerjee (postdoc at University of


  1. The black hole interior in AdS/CFT Kyriakos Papadodimas CERN and University of Groningen Strings 2014 Princeton

  2. based on work with Suvrat Raju: 1211.6767, 1310.6334, 1310.6335 + work in progress, with Souvik Banerjee (postdoc at University of Groningen) Prashant Samantray (postdoc at ICTS Bangalore) and S. Raju First Part: I will give overview of our proposal Second Part: Suvrat Raju , Wednesday at 16:00, will address Joe’s objections

  3. Black Hole interior in AdS/CFT Does a big black hole in AdS have an interior and can the CFT describe it? ? Smooth BH interior ⇒ harder to resolve the information paradox

  4. Black Hole information paradox A c B Quantum cloning on nice slices Strong subadditivity paradox [Mathur], [Almheiri, Marolf, Polchinski, Sully (AMPS)]

  5. Black Hole information paradox Should we give up smooth interior? Firewall, fuzzball,... ? Alternative: limitations of locality In Quantum Gravity locality is emergent (large N , strong coupling) ⇒ it cannot be exact Cloning/entanglement paradoxes rely on unnecessarily strong assumptions about locality

  6. Resolution: Complementarity The Hilbert space of Quantum Gravity does not factorize into interior × exterior [’t Hooft, Susskind, Thorlacius, Uglum, Bousso, Nomura, Varela, Weinberg, Verlinde × 2 , Maldacena...] BH interior is a scrambled copy of exterior This would resolve cloning/subadditivity paradoxes Questions: 1. Is there a precise mathematical realization of complementarity? 2. Is complementarity consistent with locality in effective field theory?

  7. Resolution: Complementarity The Hilbert space of Quantum Gravity does not factorize into interior × exterior [’t Hooft, Susskind, Thorlacius, Uglum, Bousso, Nomura, Varela, Weinberg, Verlinde × 2 , Maldacena...] BH interior is a scrambled copy of exterior This would resolve cloning/subadditivity paradoxes Questions: 1. Is there a precise mathematical realization of complementarity? 2. Is complementarity consistent with locality in effective field theory? Our work: 1. Progress towards a mathematical framework for complementarity 2. Evidence that complementarity is consistent with locality in EFT

  8. Setup Consider the N = 4 SYM on S 3 × time , at large N , large λ . and typical pure state | Ψ � with energy of O ( N 2 ) . What is experience of infalling observer? ⇒ Need local bulk observables

  9. Reconstructing local observables in empty AdS Large N factorization allows us to write local ∗ observables in empty AdS as non-local observables in CFT (smeared operators) � � � dω d� O ω,� φ CFT ( t, � x, z ) = k k f ω,� k ( t, � x, z ) + h . c . ω> 0 where φ CFT obeys EOMs in AdS, and [ φ CFT ( P 1 ) , φ CFT ( P 2 )] = 0 , if points P 1 , P 2 spacelike with respect to AdS metric (based on earlier works: Banks, Douglas, Horowitz, Martinec, Bena, Balasubramanian, Giddings, Lawrence, Kraus, Trivedi, Susskind, Freivogel Hamilton, Kabat, Lifschytz, Lowe, Heemskerk, Marolf, Polchinski, Sully...) ∗ Locality is approximate: 1. (Plausibly) true in 1 /N perturbation theory Unlikely that [ φ CFT ( P 1 ) , φ CFT ( P 2 )] = 0 to e − N 2 accuracy 2. 3. Locality may break down for high-point functions (perhaps no bulk spacetime interpretation)

  10. Black hole in AdS Consider typical QGP pure state | Ψ � (energy O ( N 2 )) . Single trace correlators still factorize at large N � Ψ |O ( x 1 ) ... O ( x n ) | Ψ � = � Ψ |O ( x 1 ) O ( x 2 ) | Ψ � ... � Ψ |O ( x n − 1 ) O ( x n ) | Ψ � + ... The 2-point function in which they factorize is the thermal 2-point function, which is hard to compute, but obeys KMS condition G β ( − ω, k ) = e − βω G β ( ω, k )

  11. Black hole in AdS Local bulk field outside horizon of AdS black hole ∗ � ∞ � dω O ω,m f β φ CFT ( t, Ω , z ) = ω,m ( t, Ω , z ) + h . c . 0 m At large N (and late times) the correlators � Ψ | φ CFT ( t 1 , Ω 1 , z 1 ) ...φ CFT ( t n , Ω n , z n ) | Ψ � reproduce those of semiclassical QFT on the BH background (in AdS-Hartle-Hawking state). ∗ We have clarified confusions about the convergence of the sum/integral

  12. Behind the horizon Need new modes For free infall we expect � ∞ � � O ω,m e − iωt Y m (Ω) g (1) φ CFT ( t, Ω , z ) = dω ω,m ( z ) + h . c . 0 m � O ω,m e − iωt Y m (Ω) g (2) + � ω,m ( z ) + h . c . where the modes � O ω,m must satisfy certain conditions

  13. Conditions for � O ω,m The � O ω,m ’s ( mirror or tilde operators) must obey the following conditions, in order to have smooth interior: For every O there is a � O 1. The algebra of � O ’s is isomorphic to that of the O ’s 2. The � O ’s commute with the O ’s 3. The � O ’s are “correctly entangled” with the O ’s 4. Equivalently: Correlators of all these operators on | Ψ � must reproduce (at large N ) those of the thermofield-double state � e − βE i / 2 | E i , � | TFD � = √ E i � Z i � � O ( t k ) .. O ( t n ) | Ψ � ≈ 1 O ( t 1 ) ... O ( t n ) O ( t k + iβ 2 ) ... O ( t m + iβ � Ψ |O ( t 1 ) ... � Z Tr 2 )

  14. MAIN QUESTION: does a single CFT contain operators � O with the desired properties? If so, then black hole has smooth interior, and interior is visible in the CFT.

  15. Construction of the mirror operators Exterior of AdS black hole ⇒ Described by “algebra of (products of) single trace operators O ” Why do we get a second commuting copy � O ?

  16. Construction of the mirror operators Exterior of AdS black hole ⇒ Described by “algebra of (products of) single trace operators O ” Why do we get a second commuting copy � O ? The doubling of the observables is a general phenomenon whenever we have: • A large (chaotic) quantum system in a typical state | Ψ � • We are probing it with a small algebra A of observables Under these conditions, the small algebra A is effectively “doubled”.

  17. Construction of the mirror operators T For us, | Ψ � = BH microstate (typical QGP state of E ∼ O ( N 2 ) A = “algebra” of small (i.e. O ( N 0 ) ) products of single trace operators A = span of {O ( t 1 , � x 1 ) , O ( t 1 , � x 1 ) O ( t 2 , � x 2 ) , ... } Here T is a long time scale and also need some UV regularization.

  18. The Hilbert space H Ψ For any given microstate | Ψ � consider the linear subspace H Ψ of the full Hilbert space H of the CFT H Ψ = A| Ψ � = { span of : O ( t 1 , � x 1 ) ... O ( t n , � x n )) | Ψ �}

  19. The Hilbert space H Ψ • H Ψ depends on | Ψ � • H Ψ ⇒ Contains states of higher and lower energies than | Ψ � • Bulk EFT experiments around BH | Ψ � take place within H Ψ (bulk observer cannot easily see outside H Ψ )

  20. Reducibility of representation of A The “doubling” follows from the important property : A | Ψ � � = 0 A � = 0 , ∀ A ∈ A if (we cannot annihilate the QGP microstate by the action of a few single trace operators) Physical interpretation of this property: “The state | Ψ � appears to be entangled when probed by the algebra A ”.

  21. Example: two spins Two spins, small algebra A ≡ operators acting on the first spin. 1. If no entanglement: | Ψ � = | ↑↑� s (1) s (1) + | Ψ � = 0 while + � = 0 2. If state is entangled: 1 √ | Ψ � = 2( | ↑↑� + | ↓↓� ) can check that A (1) � = 0 A (1) | Ψ � � = 0

  22. Example: Relativistic QFT in ground state t t D D x x Reeh-Schlieder theorem: Minkowski vacuum | 0 � M cannot be annihilated by acting with local operators in D . ⇒ In | 0 � M local operator algebras are entangled — (though, no proper factorization of Hilbert space due to UV divergences)

  23. Why doubling? Remember the important condition A | Ψ � � = 0 for A � = 0 (1) Suppose that dim A = n Then from (1) follows that dim H Ψ = dim (span A| Ψ � ) = n However the algebra L ( H Ψ ) of all operators that can act on H Ψ has dimensionality dim L ( H Ψ ) = n 2 while the original algebra A had only dim A = n . This suggests that L ( H Ψ ) = A ⊗ � A where � A is a “second copy” of A . We can choose basis so that [ A, � A ] = 0

  24. Summary of the problem • | Ψ � = BH microstate (QGP microstate) • A = “algebra” of small products of single trace operators Black Hole interior operators � • O must commute with A ⇒ They are elements of the “commutant” A ′ of the algebra. What is A ′ for the algebra of single trace operators A acting on a typical QGP state?

  25. Mathematical aspects of the problem Consider a von-Neumann algebra A acting on a Hilbert space H . Question: what is the commutant A ′ ? In general, question is difficult. A ′ could be trivial. However, if ∃ a state | Ψ � in H for which i) States A| Ψ � span H ii) A | Ψ � � = 0 for all A � = 0 then Theorem: (Tomita-Takesaki) The commutant A ′ is isomorphic to A ( doubling !). There is a canonical isomorphism J acting on H such that � O = J O J

  26. Constructing the mirror operators On the subspace H Ψ we define the antilinear map S by SA | Ψ � = A † | Ψ � This is well defined because of the condition A | Ψ � � = 0 for A � = 0 . We manifestly have S | Ψ � = | Ψ � and S 2 = 1 For any operator A ∈ A acting on H Ψ we define a new operator acting on the same space by ˆ A = SAS

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend