Tortoise Coordinates and Hawking Radiation in a Dynamical Spherically Symmetric Spacetime
YANG Jian1, ZHAO Zheng2, TIAN Gui-Hua1, LIU Wen-Biao2
1School of Sciences, Beijing University of Posts and Telecommunications, Beijing 1008762Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing 100875
Tortoise Coordinates and Hawking Radiation in a Dynamical Spherically Symmetric Spacetime
YANG Jian1, ZHAO Zheng2, TIAN Gui-Hua1, LIU Wen-Biao2
1School of Sciences, Beijing University of Posts and Telecommunications, Beijing 1008762Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing 100875
摘要Hawking effect from dynamical spherical Vaidya black hole, Vaidya-Bonner black hole, and Vaidya-de Sitter black hole is investigated using the improved Damour-Ruffini method. After the new tortoise coordinate transformation in which the position r of event horizon is an undetermined function and the temperature parameter κ is an undetermined constant, the Klein-Gordon equation can be written as the standard form at the event horizon, and both r and κ can be determined automatically. Then extending the outgoing wave from outside to inside of the horizon analytically, the Hawking temperature can also be obtained automatically.
Abstract:Hawking effect from dynamical spherical Vaidya black hole, Vaidya-Bonner black hole, and Vaidya-de Sitter black hole is investigated using the improved Damour-Ruffini method. After the new tortoise coordinate transformation in which the position r of event horizon is an undetermined function and the temperature parameter κ is an undetermined constant, the Klein-Gordon equation can be written as the standard form at the event horizon, and both r and κ can be determined automatically. Then extending the outgoing wave from outside to inside of the horizon analytically, the Hawking temperature can also be obtained automatically.
YANG Jian;ZHAO Zheng;TIAN Gui-Hua;LIU Wen-Biao. Tortoise Coordinates and Hawking Radiation in a Dynamical Spherically Symmetric Spacetime[J]. 中国物理快报, 2009, 26(12): 120401-120401.
YANG Jian, ZHAO Zheng, TIAN Gui-Hua, LIU Wen-Biao. Tortoise Coordinates and Hawking Radiation in a Dynamical Spherically Symmetric Spacetime. Chin. Phys. Lett., 2009, 26(12): 120401-120401.
[1] Hawking S W 1975 Commun. Math. Phys. 43 199 [2] Hawking S W 1974 Nature 248 458 [3] Bekenstein J D 1973 Phys. Rev. D 7 2333 [4] Bardeen J M, Carter B and Hawking S W 1973 Commun.Math. Phys. 31 161 [5] Damour T and Ruffini R 1976 Phys. Rev. D 14332 [6] Sannan S 1988 Gen. Rel. Grav. 20 239 [7] Liu L and Xu D Y 1980 Acta Phys. Sin. 29 1617(in Chinese) [8] Zhao Z, Gui Y X and Liu L 1981 J. Astrophys. 1141 [9] Zhao Z and Dai X X 1991 Chin. Phys. Lett. 8548 [10] Zhao Z, Luo Z Q and Dai X X 1994 Il Nuovo Cimento B 109 483 [11] Chen D Y and Yang S Z 2007 New J. Phys. 9 252 [12] Li X and Zhao Z 2000 Phys. Rev. D 62 104001 [13] Ren J and Zhao Z 2006 Chin. Phys. Lett. 150292 [14] Ren J, Zhang J Y and Zhao Z 2006 Chin. Phys. Lett. 23 2019 [15] Zhang Y P and Liu W B 2007 Astrophys. Space Sci. 312 315 [16] Liu B and Liu W B 2009 Front. Phys. Chin. 494 [17] Fodor G, Nakamura K, Oshiro Y and Tomimatsu A 1996 Phys. Rev. D 54 3882 [18] Zhao Z 1999 The Thermal Nature of Black Holes andThe Singularity of the Spacetime (Beijing: Beijing NormalUniversity Press) [19] Dai X X and Zhao Z 1992 Acta Phys. Sin. 41869 (in Chinese) [20] Dai X X, Zhao Z and Liu L 1993 Sci. Chin. A 23 69