Please wait a minute...
Frontiers of Physics

ISSN 2095-0462

ISSN 2095-0470(Online)

CN 11-5994/O4

邮发代号 80-965

2019 Impact Factor: 2.502

Frontiers of Physics  2009, Vol. 4 Issue (1): 94-96   https://doi.org/10.1007/s11467-009-0002-1
  本期目录
The thermodynamics in a dynamical black hole
The thermodynamics in a dynamical black hole
Bo LIU (刘博), Wen-biao LIU(刘文彪,)
Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing 100875, China
 全文: PDF(320 KB)   HTML
Abstract

Considering the back-reaction of emitting particles to the black hole, a “new” horizon is suggested where thermodynamics can be built in the dynamical black hole. It, at least, means that the thermodynamics of a dynamical black hole should not be constructed at the original event horizon any more. The temperature, “new” horizon position and radiating particles’ energy will be consistent again under the theory of equilibrium thermodynamical system.

Key wordsHawking radiation    black hole    information loss paradox    back-reaction    event horizon    thermodynamics
收稿日期: 2008-07-14      出版日期: 2009-03-05
Corresponding Author(s): null,Email:wbliu@bnu.edu.cn   
 引用本文:   
. The thermodynamics in a dynamical black hole[J]. Frontiers of Physics, 2009, 4(1): 94-96.
Bo LIU (刘博), Wen-biao LIU(刘文彪). The thermodynamics in a dynamical black hole. Front. Phys. , 2009, 4(1): 94-96.
 链接本文:  
https://academic.hep.com.cn/fop/CN/10.1007/s11467-009-0002-1
https://academic.hep.com.cn/fop/CN/Y2009/V4/I1/94
1 S. W. Hawking, Commun. Math. Phys. , 1975, 43: 199
doi: 10.1007/BF02345020
2 S. W. Hawking, Nature , 1974, 248: 30
doi: 10.1038/248030a0
3 J. D. Bekenstein, Phys. Rev. D , 1973, 7: 2333
doi: 10.1103/PhysRevD.7.2333
4 J. D. Bekenstein, Phys. Rev. D , 1974, 9: 3292
doi: 10.1103/PhysRevD.9.3292
5 J. M. Bardeen, B. Carter, and S. W. Hawking, Commun. Math. Phys. , 1973, 31: 161
doi: 10.1007/BF01645742
6 S. W. Hawking, Phys. Rev. D , 1976, 14: 2460
doi: 10.1103/PhysRevD.14.2460
7 S. W. Hawking, Phys. Rev. D , 2005, 72: 084013
doi: 10.1103/PhysRevD.72.084013
8 M. K. Parikh and F. Wilczek, Phys. Rev. Lett. , 2000, 85: 5042
doi: 10.1103/PhysRevLett.85.5042
9 M. K. Parikh, Int. J. Mod. Phys. D , 2004, 13: 2355
doi: 10.1142/S0218271804006498
10 M. K. Parikh, arXiv: hep-th/0402166, 2004
11 P. Kraus and F. Wilczek, Nucl. Phys. B , 1995, 433: 403
doi: 10.1016/0550-3213(94)00411-7
12 S. Hemming and E. Keski-Vakkuri, Phys. Rev. D , 2001, 64: 044006
doi: 10.1103/PhysRevD.64.044006
13 A. J. M. Medved, Phys. Rev. D , 2002, 66: 124009
doi: 10.1103/PhysRevD.66.124009
14 E. C. Vagenas, Phys. Lett. B , 2001, 503: 399
doi: 10.1016/S0370-2693(01)00242-8
15 E. C. Vagenas, Phys. Lett. B , 2004, 584: 127
doi: 10.1016/j.physletb.2004.01.039
16 J. Y. Zhang and Z. Zhao, Phys. Lett. B , 2005, 618: 14
doi: 10.1016/j.physletb.2005.05.024
17 J. Y. Zhang and Z. Zhao, Nucl. Phys. B , 2005, 725: 173
doi: 10.1016/j.nuclphysb.2005.07.024
18 J. Ren, J. Y. Zhang, and Z. Zhao, Chin. Phys. Lett ., 2006, 23: 2019
doi: 10.1088/0256-307X/23/8/016
19 W. B. Liu, Acta Physica Sinica , 2007, 56(10): 6164
20 X. K. He and W. B. Liu, Chin. Phys. Lett. , 2007, 24: 2448
doi: 10.1088/0256-307X/24/8/080
21 S. W. Zhou and W. B. Liu, Phys. Rev. D , 2008, 77(10): 104021
doi: 10.1103/PhysRevD.77.104021
22 T. Damour and R. Ruffini, Phys. Rev. D , 1976, 14: 332
doi: 10.1103/PhysRevD.14.332
23 G. Fodor, K. Nakamura, Y. Oshiro, and A. Tomimatsu, Phys. Rev. D , 1996, 54: 3882
doi: 10.1103/PhysRevD.54.3882
24 W. Collins, Phys. Rev. D , 1992, 45: 495
doi: 10.1103/PhysRevD.45.495
Viewed
Full text


Abstract

Cited

  Shared   
  Discussed