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用Hamilton-Jacobi方法研究了动态球对称Einstein-Yang-Mills-Chern-Simons 黑洞事件视界处的隧穿辐射特征及其黑洞事件视界处的温度. 其结果表明,黑洞温度及隧穿率与黑洞的固有性质及其动态特征有关. 这对于进一步研究动态黑洞的热力学性质及其相关问题是有意义的. 其方法的重要意义在于研究这类动态黑洞的霍金辐射时, 不仅适用于标量场隧穿辐射的情形, 同时也适用于研究旋量场、矢量场以及引力波的隧穿辐射.Using Hamilton-Jacobi method, the Hawking tunneling radiation and temperature are investigated near the event horizon of the Einstein-Yang-Mills-Chern-Simons black hole. The results show that the temperature and tunneling rate depend on the charge and horizon of black holes, and the conclusion is significant for investigating other dynamical black holes. What is more, we also prove that this method can be used to study Hawking radiation in the scalar, vector, Dirac field and gravitational wave cases.
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Keywords:
- Einstein-Yang-Mills-Chern-Simons black hole /
- Hawking tunneling radiation /
- Hamilton-Jacobi equation
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[35] Lin K, Yang S Z 2009 Phys. Lett. B 674 127
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[37] Lin K, Yang S Z 2010 Chin. Phys. B 11 110403
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[40] Brihaye Y, Radu E, Tchrakian D H 2011 Phys. Rev. Lett. 106 071101
[41] Brihaye Y, Radu E, Tchrakian D H 2010 Phys. Rev. D 81 064005
[42] Zhao Z, Zhu J Y, Liu W B 1999 Chin. Phys. Lett. 16 698
[43] Flanagan E E, Hughes S A 2005 New J. Phys. 7 204
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[1] Hawking S W 1974 Nature 248 30
[2] Hawking S W 1975 Commun. Math. Phys. 43 199
[3] Robinson S P, Wilczek F 2005 Phys. Rev. Lett. 95 011303
[4] Iso S, Umetsu H, Wilczek F 2006 Phys. Rev. Lett. 96 151302
[5] Das S, Robinson S P, Vagenas E C 2008 Int. J. Mod. Phys. D 17 533
[6] Xu Z, Chen B 2007 Phys. Rev. D 75 024041
[7] Jiang Q Q, Wu S Q, Cai X 2007 Phys. Lett. B 651 58
[8] Murata K, Soda J 2006 Phys. Rev. D 74 044018
[9] Vagenas E C, Das S 2006 JHEP 0610 025
[10] Setare M R 2007 Eur. Phys. J. C 49 865
[11] Jiang Q Q, Wu S Q, Cai X, 2007 Phys. Rev. D 75 064029
[12] Jiang Q Q, Wu S Q 2007 Phys. Lett. B 647 200
[13] Iso S, Umetsu H, Wilczek F 2006 Phys. Rev. D 74 044017
[14] Iso S, Morita T, Umetsu H 2007 J. High. Energy Phys. 04 068
[15] Yang S Z, Li H L, Jiang Q Q, Liu M Q 2007 Sci. China G 50 249
[16] Yang S Z, Chen D Y 2007 Inter. J. Theor. Phys. 46 2923
[17] Chen D Y, Yang S Z 2007 New J. Phys. 9 252
[18] Parikh M K, Wilczek F 2000 Phys. Rev. Lett. 85 5042
[19] Vagenas E C 2001 Phys. Lett. B 503 399
[20] Vagenas E C 2002 Mod. Phys. Lett. A 17 609
[21] Vagenas E C 2002 Phys. Lett. B 533 302
[22] Medved A J M 2002 Class. Quant. Grav. 19 589
[23] Parikh M K 2002 Phys. Lett. B 546 189
[24] Medved A J M 2002 Phys. Rev. D 66 124009
[25] Vagenas E C 2003 Phys. Lett. B 559 65
[26] Parikh M K 2004 Energy Conservation and Hawking Radiation arXiv: 0402166[hep-th]
[27] Kerner R, Mann R B 2008 Class. Quant. Grav. 25 095014
[28] Kerner R, Mann R B 2008 Phys. Lett. B 665 277
[29] Li R, Ren J R, Wei S W 2008 Class. Quant. Grav. 25 125016
[30] Li R, Ren J R 2008 Phys. Lett. B 661 370
[31] Chen D Y, Jiang Q Q, Zu X T 2008 Class. Quant. Grav. 25 205022
[32] Chen D Y, Jiang Q Q, Zu X T 2008 Phys. Lett. B 665 106
[33] Zeng X X, Yang S Z 2008 Gen. Rel. Grav. 40 2107
[34] Lin K, Yang S Z 2009 Phys. Rev. D 79 064035
[35] Lin K, Yang S Z 2009 Phys. Lett. B 674 127
[36] Lin K, Yang S Z 2009 Phys. Lett. B 680 506
[37] Lin K, Yang S Z 2010 Chin. Phys. B 11 110403
[38] Yang S Z, Lin K 2010 Sci. China 40 507 (in Chinese) [杨树政,林恺 2010 中国科学 40 507]
[39] Yang S Z, Lin K 2010 Acta Phys. Sin. 59 5266 (in Chinese) [杨树政, 林恺 2010 59 5266]
[40] Brihaye Y, Radu E, Tchrakian D H 2011 Phys. Rev. Lett. 106 071101
[41] Brihaye Y, Radu E, Tchrakian D H 2010 Phys. Rev. D 81 064005
[42] Zhao Z, Zhu J Y, Liu W B 1999 Chin. Phys. Lett. 16 698
[43] Flanagan E E, Hughes S A 2005 New J. Phys. 7 204
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