Late-time tails in a stationary axisymmetric EMDA black hole geometry

doi:10.1088/1009-1963/14/2/009

中国物理B ›› 2005, Vol. 14 ›› Issue (2): 268-273.doi: 10.1088/1009-1963/14/2/009

Late-time tails in a stationary axisymmetric EMDA black hole geometry

潘启沅, 荆继良

Institute of Physics, Hunan Normal University, Changsha 410081, China

收稿日期:2004-05-20 修回日期:2004-07-14 出版日期:2005-03-02 发布日期:2005-03-02
基金资助:
Project supported by the National Natural Science Foundation of China (Grant No 10275024); the FANEDD (Grant No 200317); and the Hunan Provincial Natural Science Foundation of China (Grant No 04JJ3019).

Late-time tails in a stationary axisymmetric EMDA black hole geometry

Pan Qi-Yuan (潘启沅), Jing Ji-Liang (荆继良)

Institute of Physics, Hunan Normal University, Changsha 410081, China

Received:2004-05-20 Revised:2004-07-14 Online:2005-03-02 Published:2005-03-02
Supported by:
Project supported by the National Natural Science Foundation of China (Grant No 10275024); the FANEDD (Grant No 200317); and the Hunan Provincial Natural Science Foundation of China (Grant No 04JJ3019).

摘要/Abstract

摘要： The late-time tails of massless and self-interacting (SI) (massive) scalar fields are investigated analytically in a stationary axisymmetric Einstein—Maxwell dilaton-axion (EMDA) black hole geometry. It is shown that the asymptotic behaviour of massless perturbations is dominated by an inverse power-law decaying tail and the intermediate asymptotic behaviour of SI (massive) perturbations is dominated by an oscillatory one.

Abstract: The late-time tails of massless and self-interacting (SI) (massive) scalar fields are investigated analytically in a stationary axisymmetric Einstein—Maxwell dilaton-axion (EMDA) black hole geometry. It is shown that the asymptotic behaviour of massless perturbations is dominated by an inverse power-law decaying tail and the intermediate asymptotic behaviour of SI (massive) perturbations is dominated by an oscillatory one.

Key words: late-time tail, stationary axisymmetric EMDA black hole, inverse power-law decaying tail

中图分类号: (Black holes)

97.60.Lf

04.70.-s (Physics of black holes)

潘启沅, 荆继良. Late-time tails in a stationary axisymmetric EMDA black hole geometry[J]. 中国物理B, 2005, 14(2): 268-273.

Pan Qi-Yuan (潘启沅), Jing Ji-Liang (荆继良). Late-time tails in a stationary axisymmetric EMDA black hole geometry[J]. Chinese Physics, 2005, 14(2): 268-273.

[1]	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.
[2]	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.
[3]	汪志云, 陈培杰, 张良英. Resonant behavior of stochastic oscillations of general relativistic disks driven by a memory-damped friction[J]. 中国物理B, 2015, 24(5): 59801-059801.
[4]	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.
[5]	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.
[6]	李慧玲. Area spectrum of the three-dimensional Gödel black hole[J]. Chin. Phys. B, 2012, 21(12): 120401-120401.
[7]	刘彤, 薛力. Jet precession in neutrino-cooled disks for gamma-ray bursts: The effects of the mass and spin of a black hole[J]. 中国物理B, 2012, 21(6): 69801-069801.
[8]	邵建舟,王永久. [J]. 中国物理B, 2012, 21(4): 40404-040404.
[9]	林恺, 杨树政. A simpler method for researching fermions tunneling from black holes[J]. 中国物理B, 2011, 20(11): 110403-110403.
[10]	潘伟珍, 杨学军, 谢志堃. Hawking effect and quantum nonthermal radiation of an arbitrarily accelerating charged black hole using a new tortoise coordinate transformation[J]. 中国物理B, 2011, 20(4): 49701-049701.
[11]	李慧玲. Fermion tunneling from squashed black holes in the Gödel universe and charged Kaluza–Klein space–time[J]. 中国物理B, 2011, 20(3): 30402-030402.
[12]	曾晓雄, 李强. On particles tunneling from the Taub-NUT-AdS black hole[J]. 中国物理B, 2009, 18(11): 4716-4720.
[13]	刘成周, 朱建阳. Asymptotic quasinormal modes of scalar field in a gravity's rainbow[J]. 中国物理B, 2009, 18(10): 4161-4168.
[14]	邓熙浩, 高思杰. Reversible Carnot cycle outside a black hole[J]. 中国物理B, 2009, 18(3): 927-932.
[15]	魏益焕. Effective first law of thermodynamics of black holes with two horizons[J]. 中国物理B, 2009, 18(2): 821-824.

Late-time tails in a stationary axisymmetric EMDA black hole geometry

Late-time tails in a stationary axisymmetric EMDA black hole geometry

PDF (PC)

赞

可视化

摘要/Abstract

引用本文

使用本文

参考文献

相关文章 15

Metrics

本文评价

推荐阅读 0