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球对称动态黑洞视界附近的瞬时辐射能通量及瞬时辐射功率

孟庆苗 蒋继建 李传安

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球对称动态黑洞视界附近的瞬时辐射能通量及瞬时辐射功率

孟庆苗, 蒋继建, 李传安

Instantaneous radiation energy flux and instantaneous radiation power of dynamic spherically symmetric black holes

Meng Qing-Miao, Jiang Ji-Jian, Li Chuan-An
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  • 采用黑洞的薄膜模型和局域热平衡的假定,研究球对称动态黑洞视界附近的瞬时辐射能通量和瞬时辐射功率,得到了当截断距离η取定后,Vaidya黑洞视界附近标量场的瞬时辐射能通量与黑洞的质量和视界变化率有关,其瞬时辐射功率仅与黑洞的视界变化率有关.Vaidya-Bonner黑洞的瞬时辐射能通量和瞬时辐射功率与黑洞的质量、电荷和视界变化率有关.表明黑洞周围的引力场、电磁场以及视界的变化均对黑洞的热辐射产生影响.
    By the thin film model and the local thermal equilibrium assumption, the instantaneous radiation power and instantaneous radiation energy flux near the event horizon of the dynamic spherically symmetric black hole have been studied. When the cut-off distance η takes a fixed value, the following results can be obtained. For Vaidya black hole, its instantaneous radiation energy flux of the scalar field near the event horizon is related to both the black hole mass and the change rate of the event horizon. But its instantaneous radiation power is only related to the change rate of the horizon. For Vaidya-Bonner black hole, the instantaneous radiation power and instantaneous radiation energy flux are all related to the mass, the charge of the black hole and the change rate of the event horizon. These results show that the gravitational field, electromagnetic field and the change of the horizon will all affect the thermal radiation of the black hole.
    • 基金项目: 国家自然科学基金(批准号:10773002)和山东省教育厅科技计划项目(批准号:J07WJ49)资助的课题.
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    [27]Meng Q M, Jiang J J,Liu J L, Deng D L 2009 Acta Phys.Sin. 58 78 (in Chinese)[孟庆苗、蒋继建、刘景伦、邓德力 2009 58 78]

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    [28]Jiang J J ,Meng Q M, Wang S 2009 Chin.Phys.B 18 456

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    [29]Meng Q M, Jiang J J,Wang S 2009 Acta Phys. Sin. 58 7486(in Chinese)[孟庆苗、蒋继建、王帅 2009 58 7486]

    [30]

    [30]Zhang J H,Meng Q M,Li C A 1996 Acta Phys.Sin. 45 177 (in Chinese)[张建华、孟庆苗、李传安 1996 45 177]

    [31]

    [31]Zhao Z 2000 Black holes and curved space-time(Taiyuan:Shanxi Science and Technology Press) p204, 246(in Chinese)[赵峥 2000 黑洞与弯曲的时空(太原:山西科学技术出版社)第204,246页)]

  • [1]

    [1]Hawking S W 1974 Nature 248 30

    [2]

    [2]Hawking S W 1975 Commun. Math. Phys. 43 199

    [3]

    [3] ’ t Hooft G 1985 Nucl. Phys. B 256 727

    [4]

    [4]Parikh M K , Wilczek F 2000 Phys. Rev. Lett. 85 5024

    [5]

    [5]Zhao Z 1999 Black Hole Thermodynamics and Singularity of Spacetime (Beijing:Beijing Nomal University Press) p70, 256(in Chinese)[赵峥 1999 黑洞的热性质与时空的奇异性 (北京:北京师范大学出版社) 第70,256页]

    [6]

    [6]Gao C J,Shen Y G 2003 Sic. China G 33 561(in Chinese)[高长军、沈有根 2003 中国科学 G 33 561]

    [7]

    [7]Liu C Z 2007 Sic. China G 37 146(in Chinese)[刘成周 2007 中国科学 G 37 146]

    [8]

    [8]Li C A, Su J Q , Jiang J J,Meng Q M 2009 Sic. China G 39 280(in Chinese)[李传安、苏九清、蒋继建、孟庆苗. 2009 中国科学 G 39 280]

    [9]

    [9]Liu W B,Zhao Z 2001 Chin. Phys. Lett. 18 310

    [10]

    [10]Li X,Zhao Z 2001 Chin. Phys. Lett. 18 463

    [11]

    [11]Li C A, Wei X Q,Meng Q M, Liu J L 2002 Acta Phys. Sin. 51 2173 (in Chinese)[李传安、魏显起、孟庆苗、刘景伦 2002 51 2173]

    [12]

    [12]Li C A, Meng Q M, Su J Q 2002 Acta Phys. Sin. 51 1897 (in Chinese)[李传安、孟庆苗、苏九清 2002 51 1897]

    [13]

    [13]Meng Q M, Su J Q , Li C A 2003 Acta Phys.Sin. 52 1822 (in Chinese)[孟庆苗、苏九清、李传安 2003 52 1822]

    [14]

    [14]Niu Z F, Liu W B 2005 Acta Phys. Sin. 54 457 (in Chinese)[牛振风、刘文彪 2005 54 475]

    [15]

    [15]Yang B 2008 Acta Phys. Sin. 57 2614 (in Chinese)[杨波 2008 57 2614]

    [16]

    [16]Gibbons G W, Hawking S W 1977 Phys. Rev. D 15 2752

    [17]

    [17]Yang S Z,Li H L,Jiang Q Q,Liu M Q 2007 Sic. China G 37 66(in Chinese)[杨树政、李慧玲、蒋青权、刘门全 2007 中国科学 G 37 66]

    [18]

    [18]Zhang J Y,Zhao Z 2006 Acta Phys. Sin. 55 3796(in Chinese)[张靖仪、赵峥 2006 55 3796]

    [19]

    [19]Han Y W 2007 Chin. Phys. 16 923

    [20]

    [20]Meng Q M,Su J Q ,Jiang J J 2007 Acta Phys.Sin. 56 3723 (in Chinese)[孟庆苗、苏九清、蒋继建 2007 56 3723]

    [21]

    [21]He T M, Fan J H, Wang Y J 2008 Chin. Phys. B 17 2321

    [22]

    [22]Meng Q M 2003 Acta Phys.Sin. 52 2102 (in Chinese)[孟庆苗 2003 52 2102]

    [23]

    [23]Meng Q M 2005 Acta Phys.Sin. 54 471 (in Chinese)[孟庆苗 2005 54 471]

    [24]

    [24]Meng Q M, Su J Q, Jiang J J 2007 Acta Phys.Sin. 56 5077 (in Chinese)[孟庆苗、苏九清、蒋继建2007 56 5077]

    [25]

    [25]Meng Q M, Jiang J J 2008 Sic. China G 38 171(in Chinese)[孟庆苗、蒋继建 2008 中国科学 G 38 171]

    [26]

    [26]Meng Q M, Wang S,Jiang J J ,Deng D L 2008 Chin.Phys.B 17 2811

    [27]

    [27]Meng Q M, Jiang J J,Liu J L, Deng D L 2009 Acta Phys.Sin. 58 78 (in Chinese)[孟庆苗、蒋继建、刘景伦、邓德力 2009 58 78]

    [28]

    [28]Jiang J J ,Meng Q M, Wang S 2009 Chin.Phys.B 18 456

    [29]

    [29]Meng Q M, Jiang J J,Wang S 2009 Acta Phys. Sin. 58 7486(in Chinese)[孟庆苗、蒋继建、王帅 2009 58 7486]

    [30]

    [30]Zhang J H,Meng Q M,Li C A 1996 Acta Phys.Sin. 45 177 (in Chinese)[张建华、孟庆苗、李传安 1996 45 177]

    [31]

    [31]Zhao Z 2000 Black holes and curved space-time(Taiyuan:Shanxi Science and Technology Press) p204, 246(in Chinese)[赵峥 2000 黑洞与弯曲的时空(太原:山西科学技术出版社)第204,246页)]

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出版历程
  • 收稿日期:  2009-05-17
  • 修回日期:  2009-06-25
  • 刊出日期:  2010-03-15

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