Massive Scalar Field Evolution in the Dyadosphere Spacetime of Charged Black Hole

Scalar field quasinormal modes in the dyadosphere spacetime of charged black hole are studied by using the third-order WKB approximation. From numerical results obtained, we find that the scalar field mass u plays an important role in studying the quasinormal frequencies. With the scalar field mass...

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Published inCommunications in theoretical physics Vol. 59; no. 4; pp. 517 - 520
Main Author 王春艳 高亚军
Format Journal Article
LanguageEnglish
Published 01.04.2013
Subjects
WKB近似
带电黑洞
拟正规
数值结果
时空
标量场
正规模
演化
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ISSN0253-6102
DOI10.1088/0253-6102/59/4/22

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Abstract Scalar field quasinormal modes in the dyadosphere spacetime of charged black hole are studied by using the third-order WKB approximation. From numerical results obtained, we find that the scalar field mass u plays an important role in studying the quasinormal frequencies. With the scalar field mass increases, the real parts increase and the magnitudes of the imaginary parts decrease. Partieulary, these change are almost linearly.
AbstractList Scalar field quasinormal modes in the dyadosphere spacetime of charged black hole are studied by using the third-order WKB approximation. From numerical results obtained, we find that the scalar field mass u plays an important role in studying the quasinormal frequencies. With the scalar field mass increases, the real parts increase and the magnitudes of the imaginary parts decrease. Partieulary, these change are almost linearly.
Author 王春艳 高亚军
AuthorAffiliation Department of Physics, School of Mathematics and Physics, Bohai University, Jinzhou 121013, China
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10.12942/lrr-1999-2
10.1088/0264-9381/9/4/012
10.1098/rspa.1975.0112
10.4310/ATMP.1998.v2.n2.a2
10.1103/PhysRevD.58.064014
10.1103/PhysRevLett.90.081301
10.1051/0004-6361:20010089
10.1103/PhysRevD.66.044009
10.1088/0264-9381/16/12/201
10.1088/0264-9381/26/16/163001
10.1007/s10509-009-0160-1
10.1016/j.physletb.2010.03.013
10.1103/PhysRevD.30.295
10.4310/ATMP.1998.v2.n2.a1
10.1103/PhysRevLett.24.737
10.1103/PhysRevD.68.024003
10.1103/PhysRevD.74.104020
10.1103/PhysRev.108.1063
10.1103/PhysRevD.47.5253
10.1142/S0217732399002777
10.1086/184453
10.1103/PhysRevD.70.124032
10.1103/PhysRevLett.81.4293
10.1103/PhysRevD.83.064020
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Notes dyadosphere spacetime, WKB approximation, quasinormal frequencies
Scalar field quasinormal modes in the dyadosphere spacetime of charged black hole are studied by using the third-order WKB approximation. From numerical results obtained, we find that the scalar field mass u plays an important role in studying the quasinormal frequencies. With the scalar field mass increases, the real parts increase and the magnitudes of the imaginary parts decrease. Partieulary, these change are almost linearly.
11-2592/O3
WANG Chun-Yan , GAO Ya-Jun
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References 22
23
G. Preparata (24) 1998; 338
E. Berti (13) 2009; 26
26
27
29
L.E. Simone (28) 1992; 9
H.P. Nollert (6) 1999; 16
10
11
12
14
J. Maldacena (18) 1998; 2
15
16
Y.S. Myung (17) 2012
H.P. Nollert (8) 1999; 16
1
2
E. Witten (19) 1998; 2
3
4
5
7
9
R. Ruffini (25) 1998; 338
20
21
References_xml – ident: 4
  doi: 10.1038/227936a0
– volume: 338
  start-page: L87
  year: 1998
  ident: 24
  publication-title: Astro. Astrophys. Lett.
– ident: 5
  doi: 10.12942/lrr-1999-2
– volume: 9
  start-page: 963
  issn: 0264-9381
  year: 1992
  ident: 28
  publication-title: Class. Quantum Grav.
  doi: 10.1088/0264-9381/9/4/012
– ident: 1
  doi: 10.1098/rspa.1975.0112
– volume: 2
  start-page: 253
  year: 1998
  ident: 19
  publication-title: Adv. Theor. Math. Phys.
  doi: 10.4310/ATMP.1998.v2.n2.a2
– ident: 27
  doi: 10.1103/PhysRevD.58.064014
– ident: 22
  doi: 10.1103/PhysRevLett.90.081301
– year: 2012
  ident: 17
– ident: 23
  doi: 10.1051/0004-6361:20010089
– ident: 9
  doi: 10.1103/PhysRevD.66.044009
– volume: 16
  start-page: R159
  issn: 0264-9381
  year: 1999
  ident: 8
  publication-title: Class. Quant. Grav.
  doi: 10.1088/0264-9381/16/12/201
– volume: 26
  start-page: 163001
  issn: 0264-9381
  year: 2009
  ident: 13
  publication-title: Class. Quant. Grav.
  doi: 10.1088/0264-9381/26/16/163001
– ident: 15
  doi: 10.1007/s10509-009-0160-1
– ident: 14
  doi: 10.1016/j.physletb.2010.03.013
– ident: 26
  doi: 10.1103/PhysRevD.30.295
– volume: 2
  start-page: 231
  year: 1998
  ident: 18
  publication-title: Adv. Theor. Math. Phys.
  doi: 10.4310/ATMP.1998.v2.n2.a1
– ident: 3
  doi: 10.1103/PhysRevLett.24.737
– ident: 10
  doi: 10.1103/PhysRevD.68.024003
– volume: 16
  start-page: R159
  issn: 0264-9381
  year: 1999
  ident: 6
  publication-title: Class. Quant. Grav.
  doi: 10.1088/0264-9381/16/12/201
– ident: 12
  doi: 10.1103/PhysRevD.74.104020
– ident: 2
  doi: 10.1103/PhysRev.108.1063
– ident: 7
  doi: 10.1103/PhysRevD.47.5253
– ident: 20
  doi: 10.1142/S0217732399002777
– volume: 338
  start-page: L87
  year: 1998
  ident: 25
  publication-title: Astro. Astrophys. Lett.
– ident: 29
  doi: 10.1086/184453
– ident: 11
  doi: 10.1103/PhysRevD.70.124032
– ident: 21
  doi: 10.1103/PhysRevLett.81.4293
– ident: 16
  doi: 10.1103/PhysRevD.83.064020
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SubjectTerms WKB近似
带电黑洞
拟正规
数值结果
时空
标量场
正规模
演化
Title Massive Scalar Field Evolution in the Dyadosphere Spacetime of Charged Black Hole
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