Cold black holes in the Harlow-Hayden approach to firewalls

被引:13
作者
Ong, Yen Chin [1 ,2 ,3 ,4 ]
McInnes, Brett [5 ]
Chen, Pisin [6 ,7 ,8 ,9 ]
机构
[1] KTH Royal Inst Technol, NORDITA, SE-10691 Stockholm, Sweden
[2] Stockholm Univ, SE-10691 Stockholm, Sweden
[3] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan
[4] Natl Taiwan Univ, Grad Inst Astrophys, Taipei 10617, Taiwan
[5] Natl Univ Singapore, Dept Math, Singapore 119076, Singapore
[6] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan
[7] Natl Taiwan Univ, Grad Inst Astrophys, Taipei 10617, Taiwan
[8] Natl Taiwan Univ, Dept Phys, Taipei 10617, Taiwan
[9] Stanford Univ, SLAG Natl Accelerator Lab, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
关键词
RADIATION; PROSPECTS; CHARGE;
D O I
10.1016/j.nuclphysb.2014.12.024
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Firewalls are controversial principally because they seem to imply departures from general relativistic expectations in regions of spacetime where the curvature need not be particularly large. One of the virtues of the Harlow-Hayden approach to the firewall paradox, concerning the time available for decoding of Hawking radiation emanating from charged AdS black holes, is precisely that it operates in the context of cold black holes, which are not strongly curved outside the event horizon. Here we clarify this point. The approach is based on ideas borrowed from applications of the AdS/CFT correspondence to the quark-gluon plasma. Firewalls aside, our work presents a detailed analysis of the thermodynamics and evolution of evaporating charged AdS black holes with flat event horizons. We show that, in one way or another, these black holes are always eventually destroyed in a time which, while long by normal standards, is short relative to the decoding time of Hawking radiation. (C) 2014 The Authors. Published by Elsevier B.V.
引用
收藏
页码:627 / 654
页数:28
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