Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

doi:10.1088/1674-1056/22/3/039701

中国物理B ›› 2013, Vol. 22 ›› Issue (3): 39701-039701.doi: 10.1088/1674-1056/22/3/039701

• GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS • 上一篇

Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

谢志堃, 潘伟珍, 杨学军

Department of Physics and Electronic Information, Shaoxing University, Shaoxing 312000, China

收稿日期:2012-05-31 修回日期:2012-08-17 出版日期:2013-02-01 发布日期:2013-02-01
基金资助:
Project supported by the National Natural Science Foundation of China (Grant Nos. 10873003 and 11045005) and the Natural Science Foundation of Zhejiang Province, China (Grant No. Y6090739).

Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

Xie Zhi-Kun (谢志堃), Pan Wei-Zhen (潘伟珍), Yang Xue-Jun (杨学军)

Department of Physics and Electronic Information, Shaoxing University, Shaoxing 312000, China

Received:2012-05-31 Revised:2012-08-17 Online:2013-02-01 Published:2013-02-01
Contact: Pan Wei-Zhen E-mail:panwz8@usx.edu.cn
Supported by:
Project supported by the National Natural Science Foundation of China (Grant Nos. 10873003 and 11045005) and the Natural Science Foundation of Zhejiang Province, China (Grant No. Y6090739).

摘要/Abstract

摘要： With a new tortoise coordinate transformation, we discussed the quantum nonthermal radiation characteristics near the event horizon by studying the Hamilton-Jacobi equation of a scalar particle in the curve space-time, and obtained the event horizon surface gravity and the Hawking temperature on the event horizon. The results showed that there is a crossing of particle energy near the event horizon. We derived the maximum overlap of the positive and negative energy levels. It was also found that the Hawking temperature of a black hole depends on not only the time, but also the angle. There is a problem of dimension in the usual tortoise coordinate, so the present results obtained by using a correct-dimension new tortoise coordinate transformation may be more reasonable.

关键词: tortoise coordinate transformation, black hole, quantum nonthermal radiation, event horizon surface gravity

Abstract: With a new tortoise coordinate transformation, we discussed the quantum nonthermal radiation characteristics near the event horizon by studying the Hamilton–Jacobi equation of a scalar particle in the curve space–time, and obtained the event horizon surface gravity and the Hawking temperature on the event horizon. The results showed that there is a crossing of particle energy near the event horizon. We derived the maximum overlap of the positive and negative energy levels. It was also found that the Hawking temperature of a black hole depends on not only the time, but also the angle. There is a problem of dimension in the usual tortoise coordinate, so the present results obtained by using a correct-dimension new tortoise coordinate transformation may be more reasonable.

Key words: tortoise coordinate transformation, black hole, quantum nonthermal radiation, event horizon surface gravity

中图分类号: (Black holes)

97.60.Lf

04.70.-s (Physics of black holes)

谢志堃, 潘伟珍, 杨学军. Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge[J]. 中国物理B, 2013, 22(3): 39701-039701.

Xie Zhi-Kun (谢志堃), Pan Wei-Zhen (潘伟珍), Yang Xue-Jun (杨学军). Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge[J]. Chin. Phys. B, 2013, 22(3): 39701-039701.

参考文献 25

[1]	Hawking S W 1974 Nature 248 30
[2]	Hawking S W 1975 Commun. Math. Phys. 43 199
[3]	Li H L 2011 Chin. Phys. B 20 030402
[4]	Pan W Z, Yang X J and Luo J C 2011 Acta Phys. Sin. 60 109701 (in Chinese)
[5]	Zhao Z 1981 Acta Phys. Sin. 30 1508 (in Chinese)
[6]	Zhao R, Zhang S L 2006 Phys. Lett. B 641 318
[7]	Jiang Q Q, Wu S Q and Cai X 2007 Phys. Rev. D 75 064029
[8]	Robinson S P and Wilczek F 2005 Phys. Rev. Lett. 95 011303
[9]	Zhao Z 1999 Thermal Properties of Black Holes and Singularities of Space-times (Beijing: Beijing Normal University Press) (in Chinese)
[10]	Qiang L E, Gao X Q and Zhao Z 2004 Acta Phys. Sin. 53 3619 (in Chinese)
[11]	Zhang J Y and Zhao Z 2005 Phys. Lett. B 618 14
[12]	Liu W B 2007 Acta Phys. Sin. 56 6164 (in Chinese)
[13]	Li H L, Yang S Z and Qi D J 2006 Commun. Theor. Phys. 46 991
[14]	Zhao R, Zhang L C and Li H F 2010 Acta Phys. Sin. 59 2982 (in Chinese)
[15]	Han Y W, Bao Z Q and Hong Y 2009 Chin. Phys. B 18 62
[16]	Lin K, Yang S Z and Zeng X X 2008 Chin. Phys. B 17 2804
[17]	Zeng X X and Yang S Z 2009 Chin. Phys. B 18 462
[18]	Starobinsky A A 1973 JETP 37 28
[19]	Unruh W G 1974 Phys. Rev. D 10 3194
[20]	Lu J L 2002 Acta Phys. Sin. 51 973 (in Chinese)
[21]	Yang S Z and Lin L B 2002 Chin. Phys. 11 619
[22]	Yang S Z 2004 Acta Phys. Sin. 53 4007 (in Chinese)
[23]	Jiang Q Q, Yang S Z and Li H L 2005 Chin. Phys. 14 1736
[24]	Meng Q M, Jiang J J and Li C A 2010 Acta Phys. Sin. 59 778 (in Chinese)
[25]	Zhao Z, Yang J and Liu W B 2010 J. Beijing Normal University (Natural Science) 46 32 (in Chinese)

Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

Quantum nonthermal radiation and horizon surface gravity of an arbitrarily accelerating black hole with electric charge and magnetic charge

PDF (PC)

赞

可视化

摘要/Abstract

引用本文

使用本文

参考文献 25

相关文章 15

Metrics

本文评价

推荐阅读 0

[1]	Xuan-Ran Zhu(朱轩然), Yun-Xian Chen(陈芸仙), Ping-Hui Mou(牟平辉), and Ke-Jian He(何柯腱). The shadow and observation appearance of black hole surrounded by the dust field in Rastall theory[J]. 中国物理B, 2023, 32(1): 10401-010401.
[2]	Jianwei Zhang(张见微), Chengmin Zhang(张承民), Di Li(李菂), Xianghan Cui(崔翔翰), Wuming Yang(杨伍明), Dehua Wang(王德华), Yiyan Yang(杨佚沿), Shaolan Bi(毕少兰), and Xianfei Zhang(张先飞). Simulation of the gravitational wave frequency distribution of neutron star-black hole mergers[J]. 中国物理B, 2021, 30(12): 120401-120401.
[3]	Wei Sun(孙威) and Xian-Hui Ge(葛先辉). Holographic heat engine efficiency of hyperbolic charged black holes[J]. 中国物理B, 2021, 30(10): 109501-109501.
[4]	胡馨匀, 何柯健, 李中华, 李国平. Thermodynamics and weak cosmic censorship conjecture of charged AdS black hole in the Rastall gravity with pressure[J]. 中国物理B, 2020, 29(5): 50401-050401.
[5]	魏益焕. Thermal properties of regular black hole with electric charge in Einstein gravity coupled to nonlinear electrodynamics[J]. 中国物理B, 2019, 28(12): 120401-120401.
[6]	宋宇, 唐浩, 邹德成, 孙成一, 岳瑞宏. Destroying MTZ black holes with test particles[J]. 中国物理B, 2018, 27(2): 20401-020401.
[7]	叶伯兵, 陈菊华, 王永久. Geometry and thermodynamics of smeared Reissner-Nordström black holes in d-dimensional AdS spacetime[J]. 中国物理B, 2017, 26(9): 90202-090202.
[8]	马洪, 李瑾. Gravitational quasi-normal modes of static R² Anti-de Sitter black holes[J]. 中国物理B, 2017, 26(6): 60401-060401.
[9]	景艺德, 彭俊金. A note on the mass of Kerr-AdS black holes in the off-shell generalized ADT formalism[J]. 中国物理B, 2017, 26(10): 100401-100401.
[10]	T. Ibungochouba Singh. Hawking radiation of stationary and non-stationary Kerr–de Sitter black holes[J]. 中国物理B, 2015, 24(7): 70401-070401.
[11]	陈斯纳, 张靖仪. Concrete quantum tunneling spectrum of Schwarzschild black holes[J]. 中国物理B, 2015, 24(2): 20401-020401.
[12]	韩亦文, 洪云. Thermodynamics of a two-dimensional charged black holein the geometric framework[J]. , 2014, 23(10): 100401-100401.
[13]	李慧玲, 林榕, 程丽英. Spectroscopy via adiabatic covariant action for the Bañados-Teitelboim-Zanelli (BTZ) black hole[J]. 中国物理B, 2013, 22(5): 50402-050402.
[14]	魏益焕, 任军. Thermodynamic properties of Reissner–Nordström–de Sitter quintessence black holes[J]. 中国物理B, 2013, 22(3): 30402-030402.
[15]	曾晓雄, 周史薇, 刘文彪. Non-equilibrium Landauer transport model for Hawking radiation from a Reissner–Nordstrom black hole[J]. 中国物理B, 2012, 21(9): 90402-090402.