Scalar field quasinormal frequencies of Reissner-Nordstrom black hole surrounded by quintessence by using the continued fraction method

被引：3

作者：

Wu, Chen ^{[1
]}

机构：

[1] Chinese Acad Sci, Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2017年 / 26卷 / 10期

关键词：

Scalar perturbation; dark energy; quasinormal modes; NORMAL MODES;

D O I：

10.1142/S0218271817501115

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We evaluate the quasinormal modes of massless scalar field around Reissner-Nordstrom black hole surrounded by a static and spherically symmetric quintessence using the continued fraction method. The appropriate Frobenius series for three special cases of the quintessence parameter is an element of = -1/3,-2/3 and -1 are derived successfully. We show the variation of quasinormal frequencies with charge of the black hole and the quintessential parameters. The numerical results show that quintessence field decreases oscillation frequencies of all angular momentum l modes and increases the damping time of l > 0 modes.

引用

页数：10

共 21 条

[1] Observation of Gravitational Waves from a Binary Black Hole Merger [J].

Abbott, B. P. ;

Abbott, R. ;

Abbott, T. D. ;

Abernathy, M. R. ;

Acernese, F. ;

Ackley, K. ;

Adams, C. ;

Adams, T. ;

Addesso, P. ;

Adhikari, R. X. ;

Adya, V. B. ;

Affeldt, C. ;

Agathos, M. ;

Agatsuma, K. ;

Aggarwal, N. ;

Aguiar, O. D. ;

Aiello, L. ;

Ain, A. ;

Ajith, P. ;

Allen, B. ;

Allocca, A. ;

Altin, P. A. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arai, K. ;

Arain, M. A. ;

Araya, M. C. ;

Arceneaux, C. C. ;

Areeda, J. S. ;

Arnaud, N. ;

Arun, K. G. ;

Ascenzi, S. ;

Ashton, G. ;

Ast, M. ;

Aston, S. M. ;

Astone, P. ;

Aufmuth, P. ;

Aulbert, C. ;

Babak, S. ;

Bacon, P. ;

Bader, M. K. M. ;

Baker, P. T. ;

Baldaccini, F. ;

Ballardin, G. ;

Ballmer, S. W. ;

Barayoga, J. C. ;

Barclay, S. E. ;

Barish, B. C. ;

Barker, D. ;

Barone, F. .

PHYSICAL REVIEW LETTERS, 2016, 116 (06)

[2]

[Anonymous], J HIGH ENERGY PHYS

[3] Cosmological imprint of an energy component with general equation of state [J].

Caldwell, RR ;

Dave, R ;

Steinhardt, PJ .

PHYSICAL REVIEW LETTERS, 1998, 80 (08) :1582-1585

[4] Quasinormal modes of a black hole surrounded by quintessence [J].

Chen, SB ;

Jing, JL .

CLASSICAL AND QUANTUM GRAVITY, 2005, 22 (21) :4651-4657

[5] A flat Universe from high-resolution maps of the cosmic microwave background radiation [J].

de Bernardis, P ;

Ade, PAR ;

Bock, JJ ;

Bond, JR ;

Borrill, J ;

Boscaleri, A ;

Coble, K ;

Crill, BP ;

De Gasperis, G ;

Farese, PC ;

Ferreira, PG ;

Ganga, K ;

Giacometti, M ;

Hivon, E ;

Hristov, VV ;

Iacoangeli, A ;

Jaffe, AH ;

Lange, AE ;

Martinis, L ;

Masi, S ;

Mason, PV ;

Mauskopf, PD ;

Melchiorri, A ;

Miglio, L ;

Montroy, T ;

Netterfield, CB ;

Pascale, E ;

Piacentini, F ;

Pogosyan, D ;

Prunet, S ;

Rao, S ;

Romeo, G ;

Ruhl, JE ;

Scaramuzzi, F ;

Sforna, D ;

Vittorio, N .

NATURE, 2000, 404 (6781) :955-959

[6]

Frolov V. P., 1998, Black hole physics: basic concepts and new developments

[7] Massless scalar field quasi-normal frequencies of Schwarzschild black hole in the quintessence background [J].

Guo, Guanghai .

EUROPEAN PHYSICAL JOURNAL C, 2013, 73 (09) :1-8

[8] Testing the interaction between dark energy and dark matter via the latest observations [J].

He, Jian-Hua ;

Wang, Bin ;

Abdalla, Elcio .

PHYSICAL REVIEW D, 2011, 83 (06)

[9] Quintessence and black holes [J].

Kiselev, VV .

CLASSICAL AND QUANTUM GRAVITY, 2003, 20 (06) :1187-1197

[10] Quasi-normal modes of stars and black holes [J].

Kokkotas K.D. ;

Schmidt B.G. .

Living Reviews in Relativity, 1999, 2 (1)

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