Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2017, Vol. 41> Issue(4) : 045103 DOI: 10.1088/1674-1137/41/4/045103

Hawking radiation and entropy of a black hole in Lovelock-Born-Infeld gravity from the quantum tunneling approach

  • 1.

     Institute of Theoretical Physics, Lingnan Normal University, Zhanjiang 524048, China

  • The tunneling radiation of particles from black holes in Lovelock-Born-Infeld (LBI) gravity is studied by using the Parikh-Wilczek (PW) method, and the emission rate of a particle is calculated. It is shown that the emission spectrum deviates from the purely thermal spectrum but is consistent with an underlying unitary theory. Compared to the conventional tunneling rate related to the increment of black hole entropy, the entropy of the black hole in LBI gravity is obtained. The entropy does not obey the area law unless all the Lovelock coefficients equal zero, but it satisfies the first law of thermodynamics and is in accordance with earlier results. It is distinctly shown that the PW tunneling framework is related to the thermodynamic laws of the black hole.
      PCAS:
  • 加载中

  • References

    [1] S. W. Hawking, Commun. Math. Phys., 43:199 (1975)
    [2] G. W. Gibbons and S. W. Hawking, Phys. Rev. D, 15:2752 (1997)
    [3] J. Y. Zhang and Z. Zhao, Acta Phys. Sin., 51:2399 (2002) (in Chinese)
    [4] W. B. Liu and Z. Zhao, Chin. Phys. Lett., 18:310 (2001)
    [5] S. Z. Yang and L. B. Lin, Chin. Phys., 11:619 (2002)
    [6] J. L. Jing, Chin. Phys. Lett., 20:459 (2003)
    [7] S.W. Hawking, Phys. Rev. D, 72:084013 (2005)
    [8] P. Kraus and F. Wilczek, Nucl. Phys. B, 433:403 (1995)
    [9] M. K. Parikh and F. Wilczek, Phys. Rev. Lett., 85:5042 (2000)
    [10] M. K. Parikh, Int. J. Mod. Phys. D, 13:2351 (2004)
    [11] J. Y. Zhang and Z. Zhao, J. High Energy Phys., 10:55 (2005)
    [12] J. Y. Zhang and Z. Zhao, Nucl. Phys. B, 725:173 (2005)
    [13] Q. Q. Jiang, S. Z. Yang, and H. L. Li, Chin. Phys., 14:1736 (2005)
    [14] Y. W. Han and S. Z. Yang, Chin. Phys. Lett., 22:2769 (2005)
    [15] J. Ren, Z. Zhao and C. J. Gao, Chin. Phys. Lett., 22:2489 (2005)
    [16] J. Y. Zhang and Z. Zhao, Phys. Lett. B, 618:14 (2005)
    [17] J. Y. Zhang and Z. Zhao, Mod. Phys. Lett. A, 20:1673 (2005)
    [18] S. Z. Yang, Chin. Phys. Lett., 22:2492 (2005)
    [19] G. Q. Li, Europhys. Lett., 76:203 (2006)
    [20] J. Y. Zhang, J H. Fan, Phys. Lett. B, 648:133 (2007)
    [21] G. Q. Li, Europhys. Lett., 75:216 (2006)
    [22] G. Q. Li, J. Phys. A:Math. Gen., 39:11889 (2006)
    [23] G. Q. Li, Mod. Phys. Lett. A, 22:209 (2007)
    [24] G. Q. Li and J. X. Mo, Astrophys. Space Sci., 361:251 (2016)
    [25] J. Math. Phys. (N.Y.) 12:498 (1971)
    [26] D. G. Boulware and S. Deser, Phys. Rev. Lett., 55:2656 (1985)
    [27] M. H. Dehghani, N. Alinejadi, and S. H. Hendi, Phys. Rev. D, 77:104025 (2008)[arXiv:0802.2637]
    [28] J. X. Mo and W. B. Liu, Eur. Phys. J. C, 74:2836 (2014)[arXiv:1401.0785]
    [29] M. H. Dehghani and M. Shamirzaie, Phys. Rev. D, 72:124015 (2005)[arXiv:hep-th/0506227]
    [30] M. H. Dehghani and R. B. Mann, Phys. Rev. D, 73:104003 (2006)[arXiv:hep-th/0602243]
    [31] M. H. Dehghani and N. Farhangkhah, Phys. Rev. D, 78:064015 (2008)[arXiv:0806.1426]
    [32] M. H. Dehghani and R. Pourhasan, Phys. Rev. D, 79:064015 (2009)[arXiv:0903.4260]
    [33] M. H. Dehghani and R. B. Mann, JHEP, 1007:019 (2010)[arXiv:1004.4397]
    [34] M. H. Dehghani and Sh. Asnafi, Phys. Rev. D, 84:064038 (2011)[arXiv:1107.3354]
    [35] M. Aiello, R. Ferraro, and G. Giribet, Phys. Rev. D, 70:104014 (2004)[arXiv:gr-qc/0408078]
    [36] R. Banerjee and S. K. Modak, JHEP, 0911:073 (2009)[arXiv:0908.2346]
    [37] H. Maeda, M. Hassaine, and C. Martinez, Phys. Rev. D, 79:044012 (2009)[arXiv:0812.2038]
    [38] R. G. Cai, L. M. Cao, and N. Ohta, Phys. Rev. D, 81:024018 (2010)[arXiv:0911.0245]
    [39] D. Kastor, S. Ray, and J. Traschen, Class. Quant. Grav., 27:235014 (2010)[arXiv:1005.5053]
    [40] S. H. Mazharimousavi and M. Halilsoy, Phys. Lett. B, 694:54 (2010)[arXiv:1007.4888]
    [41] D. Zou, R. Yue and Z. Yang, Commun. Theor. Phys., 55:449 (2011)[arXiv:1011.2595]
    [42] P. Li, R. H. Yue and D. C. Zou, Commun. Theor. Phys., 56:845 (2011)[arXiv:1110.0064]
    [43] S. Sarkar and A. C. Wall, Phys. Rev. D, 83:124048 (2011)[arXiv:1011.4988]
    [44] J. de Boer, M. Kulaxizi, and A. Parnachev, JHEP, 1107:109 (2011)[arXiv:1101.5781]
    [45] Y. Bardoux, C. Charmousis, and T. Kolyvaris, Phys. Rev. D, 83:104020 (2011)[arXiv:1012.4390]
    [46] S. H. Hendi, S. Panahiyan, and H. Mohammadpour, Eur. Phys. J. C, 72:2184 (2012)
    [47] R. Yue, D. Zou, T. Yu, P. Li, and Z. Yang, Gen. Rel. Grav., 43:2103 (2011)[arXiv:1011.5293]
    [48] M. Cruz and E. Rojas, Class. Quant. Grav., 30:115012 (2013)[arXiv:1212.1704]
    [49] T. Padmanabhan and D. Kothawala, Phys. Rept., 531:115 (2013)[arXiv:1302.2151]
    [50] D. C. Zou, S. J. Zhang, and B. Wang, Phys. Rev. D, 87:084032 (2013)[arXiv:1302.0904]
    [51] B. Chen and J. J. Zhang, JHEP, 07:185 (2013)[arXiv:1305.6767]
    [52] M. B. Gaete and M. Hassaine, JHEP, 1311:177 (2013)[arXiv:1309.3338]
    [53] Z. Amirabi, Phys. Rev. D, 88:087503 (2013)[arXiv:1311.4911]
    [54] J. de Boer, M. Kulaxizi, and A. Parnachev, JHEP, 1006:008 (2010)[arXiv:0912.1877]
    [55] M. Born and L. Infeld, Proc. Roy. Soc. Lond. A, 144:425 (1934)
    [56] E. Keski-Vakkuri and P. Kraus, Nucl. Phys. B, 491:249 (1997)

  • Access

    加载中

Get Citation
Gu-Qiang Li. Hawking radiation and entropy of a black hole in Lovelock-Born-Infeld gravity from the quantum tunneling approach[J]. Chinese Physics C, 2017, 41(4): 045103. doi: 10.1088/1674-1137/41/4/045103
Gu-Qiang Li. Hawking radiation and entropy of a black hole in Lovelock-Born-Infeld gravity from the quantum tunneling approach[J]. Chinese Physics C, 2017, 41(4): 045103.  doi: 10.1088/1674-1137/41/4/045103 shu
Milestone
Received: 2016-08-29
Revised: 2016-10-19
Fund

    Supported by Guangdong Natural Science Foundation (2016A030307051, 2015A030313789)

Article Metric

Article Views(1588)
PDF Downloads(42)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Hawking radiation and entropy of a black hole in Lovelock-Born-Infeld gravity from the quantum tunneling approach

    Corresponding author: Gu-Qiang Li,
  • 1. Institute of Theoretical Physics, Lingnan Normal University, Zhanjiang 524048, China
  • Received Date: 2016-08-29
  • Accepted Date: 2016-10-19
  • Available Online: 2017-04-05
Fund Project:  Supported by Guangdong Natural Science Foundation (2016A030307051, 2015A030313789)

Abstract: The tunneling radiation of particles from black holes in Lovelock-Born-Infeld (LBI) gravity is studied by using the Parikh-Wilczek (PW) method, and the emission rate of a particle is calculated. It is shown that the emission spectrum deviates from the purely thermal spectrum but is consistent with an underlying unitary theory. Compared to the conventional tunneling rate related to the increment of black hole entropy, the entropy of the black hole in LBI gravity is obtained. The entropy does not obey the area law unless all the Lovelock coefficients equal zero, but it satisfies the first law of thermodynamics and is in accordance with earlier results. It is distinctly shown that the PW tunneling framework is related to the thermodynamic laws of the black hole.

    HTML

Reference (56)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return