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Quasinormal Modes of Electromagnetic Perturbation around a Stringy Black Hole |
| ZHANG Yu;GUI Yuan-Xing;YU Fei;WANG Fu-Jun |
| School of Physics and Optoelectronic Technology, Dalian University of Technology, Dalian 116024 |
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| Cite this article: |
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ZHANG Yu, GUI Yuan-Xing, YU Fei et al 2007 Chin. Phys. Lett. 24 2749-2751 |
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Abstract We investigate the electromagnetic perturbation around a stringy black hole. A second-order differential equation is obtained for the perturbation. The variation of the effective potential with r is presented. The complex frequencies of the quasinormal modes of electromagnetic perturbation around a stringy black hole are computed by the third Wentzel--Kramers--Brillouin (WKB) approximation. The results show that the parameters resulted from the
compactification of higher dimensions can influence the quasinormal complex
frequencies, and the Maxwell field around a stringy black hole damps more
slowly than that around a Schwarzschild black hole.
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| Keywords:
04.30.Nk
04.70.Bw
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Received: 27 May 2007
Published: 20 September 2007
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| PACS: |
04.30.Nk
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(Wave propagation and interactions)
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04.70.Bw
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(Classical black holes)
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[1] Kokkotas K D and Schmidt B G 1999 Living Rev. Rel. 2 2
[2]Nollert H P 1999 Class. Quantum Grav. 16 R159
[3]Chandrasekhar S 1975 Proc. R. Soc. London A 343 289
[4]Konoplya R A 2005 Phys. Rev. D 71 024038
[5]Cardoso V and Lemos J P S 2001 Phys. Rev. D 64 084017
[6]Beri E, Cardoso V and Yoshida S 2004 Phys. Rev. D 69 124018
[7]Cardoso V, Lemos J P S and Yoshida S 2004 Phys. Rev. D 70 124032
[8]Jing J L and Pan Q Y 2005 Phys. Rev. D 71 124011
[9]Chen S B and Jing J L 2005 Class. Quantum Grav. 22 533
[10]Chen S B and Jing J L 2005 Class. Quantum Grav. 22 2159
[11]Liu H 1995 Class. Quantum Grav. 12 543
[12]Liu H and Mashhoon B 1996 Class. Quantum Grav. 13 233
[13]Wang B, Abdalla E and Mann R B 2002 Phys. Rev. D 65 084006
[14]Wang B, Lin C Y and Molina C 2004 Phys. Rev. D 70064025
[15]Konoplya R A and Zhidenko A 2006 Phys. Rev. D 73124040
[16]L\'{opez-Ortega A 2006 Gen. Rel. Grav. 38 743
[17]Zhang Y and Gui Y X 2006 Class. Quantum Grav. 23 6141
[18]Zhang Y, Gui Y X, Yu F and Li F L 2007 Gen. Rel. Grav. 39 1003
[19]Vishveshwara C V 1970 Nature 227 936
[20]Schutz B F and Will C M 1985 Astrophys. J. 291L33
[21]Iyer S and Will C M 1987 Phys. Rev. D 35 3621
[22]Konoplya R A 2003 Phys. Rev. D 68 024018
[23]Ferrari V and Mashhoon B 1984 Phys. Rev. D 30 295
[24]Leaver E W 1985 Proc. R. Soc. A 402 285
[25]Echeverria F 1989 Phys. Rev. D 40 3194
[26]Finn L S 1992 Phys. Rev. D 46 5236
[27]Witten E 1998 Adv. Theor. Math. Phys. 2 253
[28]Bekenstein J 1974 Lett. Nuovo Cimento 11 467
[29]Bekenstein J 1998 Cosmology and Gravitation ed Novello M(Atlasciences, France 2000) pp 1--85 gr-qc/9808028
[30]Hod S 1998 Phys. Rev. Lett. 81 4293
[31]Li X Z, Hao J G and Liu D J 2001 Phys. Lett. B 507 312
[32]McGuidan M D, Nappi C R and Yost S A 1992 Nucl. Phys. B 375 421
[33]Wheeler J A 1955 Phys. Rev. 97 511
[34]Cveti\v{c M and Youm D 1995 Phys. Rev. D 53 584
[35]Cveti\v{c M and Youm D 1996 Nucl. Phys. B 472 249
[36]Iyer S 1987 Phys. Rev. D 35 3632 |
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