Author:
Avery Steven G.,Chowdhury Borun D.,Puhm Andrea
Abstract
Abstract
We investigate the recent black hole firewall argument. For a black hole in a typical state we argue that unitarity requires every quantum of radiation leaving the black hole to carry information about the initial state. An information-free horizon is thus inconsistent with unitary at every step of the evaporation process. The required horizon-scale structure is manifest in the fuzzball proposal which provides a mechanism for holding up the structure. In this context we want to address the experience of an infalling observer and discuss the recent fuzzball complementarity proposal. Unlike black hole complementarity and observer complementarity which postulate asymptotic observers experience a hot membrane while infalling ones pass freely through the horizon, fuzzball complementarity postulates that fine-grained operators experience the details of the fuzzball microstate and coarse-grained operators experience the black hole. In particular, this implies that an in-falling detector tuned to energy E ~ T
H
, where T
H
is the asymptotic Hawking temperature, does not experience free infall while one tuned to E ≫ T
H
does.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
Reference71 articles.
1. G. Gibbons, Birkhoff ’s invariant and Thorne’s hoop conjecture, arXiv:0903.1580 [INSPIRE].
2. S. Hawking, Particle creation by black holes, Commun. Math. Phys.
43 (1975) 199 [Erratum ibid.
46 (1976) 206] [INSPIRE].
3. L. Susskind, L. Thorlacius and J. Uglum, The stretched horizon and black hole complementarity, Phys. Rev.
D 48 (1993) 3743 [hep-th/9306069] [INSPIRE].
4. A. Almheiri, D. Marolf, J. Polchinski and J. Sully, Black holes: complementarity or firewalls?, JHEP
02 (2013) 062 [arXiv:1207.3123] [INSPIRE].
5. R. Bousso, Complementarity is not enough, Phys. Rev.
D 87 (2013) 124023 [arXiv:1207.5192] [INSPIRE].
Cited by
41 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献