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Kerr-Newman黑洞的辐射谱

赵仁 张丽春 李怀繁

Kerr-Newman黑洞的辐射谱

赵仁, 张丽春, 李怀繁
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  • 运用Damour-Ruffini方法研究Kerr-Newman黑洞粒子的Hawking辐射.在保持时空中总能量,总角动量和总电荷守恒的条件下,考虑辐射粒子对时空的反作用后,得到黑洞辐射谱不再是严格的纯热谱. 在该结论中,不但含有辐射粒子能量的影响项,而且含有辐射粒子角动量对黑洞角动量的影响项. 所给表达式与用隧穿方法得到的表达式一致.满足量子力学的幺正性原理.
    • 基金项目: 山西省自然科学基金(批准号: 2006011012)和山西大同大学博士科研启动基金资助的课题.
    [1]

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

    [2]

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

    [3]

    [3]Hawking S W, Penrose R 1996 The Nature of Space and Time (Princeton. Princeton University Press)

    [4]

    [4]Thorne K 1994 Black Hole and Time Warps (New York. Norton Company)

    [5]

    [5]Hawking S W 2005 Phys. Rev. D 72 084013

    [6]

    Hawking S W 2002 Hawking’s talk at 17th International Conference on General Relativity and Gravition in Dublin. ArXiv: hep-th/0204107

    [7]

    [6]Parikh M K, Wilczek F 2000 Phys. Rev. Lett. 85 5042

    [8]

    [7]Kerner R, Mann R B 2006 Phys. Rev. D 73 104010

    [9]

    [8]Cai R G, Cao L M, Hu Y P 2008 Class. Quant. Grav. 26 155018

    [10]

    [9]Banerjee R, Majhi B R 2008 JHEP 06 095

    [11]

    Banerjee R, Majhi B R 2008 Phys. Lett. B 662 62

    [12]

    ]Kerner R, Mann R B 2007 Phys. Rev. D 75 084022

    [13]

    ]Kerner R, Mann R B 2008 Phys. Lett. B 665 277

    [14]

    ]Zhao R, Li H F, Hu S Q 2007 Chinese Journal of Physics. 45 32

    [15]

    ]Arzano M, Medved A J M, Vagenas E C 2005 JHEP 09 037

    [16]

    ]Zhang J Y, Zhao Z 2005 Phys. Lett. B 618 14

    [17]

    ]Jiang Q Q, Wu S Q, Cai X 2007 Phys. Rev. D 75 064029

    [18]

    ]Zhang J Y, Fan J H 2007 Phys. Lett. B 648 133

    [19]

    ]Li R, Ren J R 2008 Phys. Lett. B 661 370

    [20]

    ]Peng J J, Wu S Q 2008 Phys. Lett. B 661 300

    [21]

    ]Li H L, Jiang Q Q, Yang S Z 2006 Acta Phys. Sin. 55 539 (in Chinese) [李慧玲、蒋青权、 杨树政 2006 物理学报 55 539]

    [22]

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

    [23]

    ]Jiang Q Q, Wu S Q, Cai X 2007 Acta Phys. Sin. 56 3083 (in Chinese) [蒋青权、吴双清、蔡勖2007物理学报 56 3083]

    [24]

    ]Liu W B 2007 Acta Phys. Sin. 56 6164 (in Chinese) [刘文彪 2007 物理学报 56 6164]

    [25]

    ]He X K, Liu W B 2007 Phys. Lett. B 653 330

    [26]

    ]Zhou S W, Liu W B 2008 Phys. Rev. D 77 104021

    [27]

    ]Damour T, Ruffini R 1976 Phys. Rev. D 14 332

    [28]

    ]Sannan S 1988 Gen. Rel. Grav. 20 239

    [29]

    ]Vagenas E C 2008 JHEP 0811 073

    [30]

    ]Medved A J M 2008 Class. Quant. Grav. 25 205014[29]Wu S Q, Cai X 2000 Int. J. Theor. Phys. 39 2215

    [31]

    ]Wu S Q, Cai X 2000 IL Nuovo Cimento B 115 143

    [32]

    ]Bardeen J M, Carter B, Hawking S W 1973 Commun. Math. Phys. 31 161

    [33]

    ]Wald R M 1984 General Relativity (Chicago and London: the university of Chicago press)

  • [1]

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

    [2]

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

    [3]

    [3]Hawking S W, Penrose R 1996 The Nature of Space and Time (Princeton. Princeton University Press)

    [4]

    [4]Thorne K 1994 Black Hole and Time Warps (New York. Norton Company)

    [5]

    [5]Hawking S W 2005 Phys. Rev. D 72 084013

    [6]

    Hawking S W 2002 Hawking’s talk at 17th International Conference on General Relativity and Gravition in Dublin. ArXiv: hep-th/0204107

    [7]

    [6]Parikh M K, Wilczek F 2000 Phys. Rev. Lett. 85 5042

    [8]

    [7]Kerner R, Mann R B 2006 Phys. Rev. D 73 104010

    [9]

    [8]Cai R G, Cao L M, Hu Y P 2008 Class. Quant. Grav. 26 155018

    [10]

    [9]Banerjee R, Majhi B R 2008 JHEP 06 095

    [11]

    Banerjee R, Majhi B R 2008 Phys. Lett. B 662 62

    [12]

    ]Kerner R, Mann R B 2007 Phys. Rev. D 75 084022

    [13]

    ]Kerner R, Mann R B 2008 Phys. Lett. B 665 277

    [14]

    ]Zhao R, Li H F, Hu S Q 2007 Chinese Journal of Physics. 45 32

    [15]

    ]Arzano M, Medved A J M, Vagenas E C 2005 JHEP 09 037

    [16]

    ]Zhang J Y, Zhao Z 2005 Phys. Lett. B 618 14

    [17]

    ]Jiang Q Q, Wu S Q, Cai X 2007 Phys. Rev. D 75 064029

    [18]

    ]Zhang J Y, Fan J H 2007 Phys. Lett. B 648 133

    [19]

    ]Li R, Ren J R 2008 Phys. Lett. B 661 370

    [20]

    ]Peng J J, Wu S Q 2008 Phys. Lett. B 661 300

    [21]

    ]Li H L, Jiang Q Q, Yang S Z 2006 Acta Phys. Sin. 55 539 (in Chinese) [李慧玲、蒋青权、 杨树政 2006 物理学报 55 539]

    [22]

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

    [23]

    ]Jiang Q Q, Wu S Q, Cai X 2007 Acta Phys. Sin. 56 3083 (in Chinese) [蒋青权、吴双清、蔡勖2007物理学报 56 3083]

    [24]

    ]Liu W B 2007 Acta Phys. Sin. 56 6164 (in Chinese) [刘文彪 2007 物理学报 56 6164]

    [25]

    ]He X K, Liu W B 2007 Phys. Lett. B 653 330

    [26]

    ]Zhou S W, Liu W B 2008 Phys. Rev. D 77 104021

    [27]

    ]Damour T, Ruffini R 1976 Phys. Rev. D 14 332

    [28]

    ]Sannan S 1988 Gen. Rel. Grav. 20 239

    [29]

    ]Vagenas E C 2008 JHEP 0811 073

    [30]

    ]Medved A J M 2008 Class. Quant. Grav. 25 205014[29]Wu S Q, Cai X 2000 Int. J. Theor. Phys. 39 2215

    [31]

    ]Wu S Q, Cai X 2000 IL Nuovo Cimento B 115 143

    [32]

    ]Bardeen J M, Carter B, Hawking S W 1973 Commun. Math. Phys. 31 161

    [33]

    ]Wald R M 1984 General Relativity (Chicago and London: the university of Chicago press)

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    Citation:
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出版历程
  • 收稿日期:  2008-10-06
  • 修回日期:  2009-09-03
  • 刊出日期:  2010-05-15

Kerr-Newman黑洞的辐射谱

  • 1. 山西大同大学物理系,理论物理研究所,大同 037009
    基金项目: 

    山西省自然科学基金(批准号: 2006011012)和山西大同大学博士科研启动基金资助的课题.

摘要: 运用Damour-Ruffini方法研究Kerr-Newman黑洞粒子的Hawking辐射.在保持时空中总能量,总角动量和总电荷守恒的条件下,考虑辐射粒子对时空的反作用后,得到黑洞辐射谱不再是严格的纯热谱. 在该结论中,不但含有辐射粒子能量的影响项,而且含有辐射粒子角动量对黑洞角动量的影响项. 所给表达式与用隧穿方法得到的表达式一致.满足量子力学的幺正性原理.

English Abstract

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