scholarly journals Toy model for decoherence in the black hole information problem

2020 ◽  
Vol 102 (8) ◽  
Author(s):  
Kartiek Agarwal ◽  
Ning Bao
2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
Daniel Harlow ◽  
Edgar Shaghoulian

Abstract In this paper we argue for a close connection between the non-existence of global symmetries in quantum gravity and a unitary resolution of the black hole information problem. In particular we show how the essential ingredients of recent calculations of the Page curve of an evaporating black hole can be used to generalize a recent argument against global symmetries beyond the AdS/CFT correspondence to more realistic theories of quantum gravity. We also give several low-dimensional examples of quantum gravity theories which do not have a unitary resolution of the black hole information problem in the usual sense, and which therefore can and do have global symmetries. Motivated by this discussion, we conjecture that in a certain sense Euclidean quantum gravity is equivalent to holography.


2018 ◽  
Vol 57 (6) ◽  
pp. 1763-1773 ◽  
Author(s):  
Merab Gogberashvili ◽  
Lasha Pantskhava

2020 ◽  
Vol 2020 (8) ◽  
Author(s):  
Cesar A. Agón ◽  
Sagar F. Lokhande ◽  
Juan F. Pedraza

Abstract Quantum corrections to the entanglement entropy of matter fields interacting with dynamical gravity have proven to be very important in the study of the black hole information problem. We consider a one-particle excited state of a massive scalar field infalling in a pure AdS3 geometry and compute these corrections for bulk subregions anchored on the AdS boundary. In the dual CFT2, the state is given by the insertion of a local primary operator and its evolution thereafter. We calculate the area and bulk entanglement entropy corrections at order $$ \mathcal{O}\left({N}^0\right), $$ O N 0 , both in AdS and its CFT dual. The two calculations match, thus providing a non-trivial check of the FLM formula in a dynamical setting. Further, we observe that the bulk entanglement entropy follows a Page curve. We explain the precise sense in which our setup can be interpreted as a simple model of black hole evaporation and comment on the implications for the information problem.


2012 ◽  
Vol 2012 (9) ◽  
Author(s):  
Markus P. Müller ◽  
Jonathan Oppenheim ◽  
Oscar C.O. Dahlsten

2007 ◽  
Vol 379 (2) ◽  
pp. 629-640 ◽  
Author(s):  
F. J. Tipler ◽  
J. Graber ◽  
M. McGinley ◽  
J. Nichols-Barrer ◽  
C. Staecker

2012 ◽  
Vol 2012 (9) ◽  
Author(s):  
Markus P. Müller ◽  
Jonathan Oppenheim ◽  
Oscar C.O. Dahlsten

2006 ◽  
Vol 73 (10) ◽  
Author(s):  
David A. Lowe ◽  
Lárus Thorlacius

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