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Chin. Phys. B, 2017, Vol. 26(6): 060401    DOI: 10.1088/1674-1056/26/6/060401
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Gravitational quasi-normal modes of static R2 Anti-de Sitter black holes

Hong Ma(马洪), Jin Li(李瑾)
Department of Physics, Chongqing University, Chongqing 401331, China
Abstract  In this paper, we study the gravitational quasi-normal modes (QNMs) for a static R2 black hole (BH) in Anti-de Sitter (AdS) spacetime. The corresponding master equation of odd parity is derived and the QNMs are evaluated by the Horowitz and Hubeny method. Meanwhile the stability of such BH is also discussed through the temporal evolution of the perturbation field. Here we mainly consider the coefficient λ, which is related to the radius of AdS black hole, on the QNMs of the R2 AdS BH. The results show that the Re(ω) and |Im(ω)| of the QNMs increase together as |λ| increases for a given angular momentum number l. That indicates with a larger value of |λ| the corresponding R2 AdS BH returns to stable much more quickly. The dynamic evolution of the perturbation field is consistent with the results derived by the Horowitz and Hubeny method. Since in the conformal field theory the QNMs can reflect its approach to equilibrium, so our related results could be referential to studies of the AdS/CFT conjecture. The relationship between λ and the properties of the static R2 BH might be helpful for the development of R2 gravitational theory.
Keywords:  static R2 AdS black hole      gravitational perturbation      quasi-normal modes  
Received:  27 December 2016      Revised:  11 February 2017      Accepted manuscript online: 
PACS:  04.70.Bw (Classical black holes)  
  04.62.+v (Quantum fields in curved spacetime)  
  04.70.-s (Physics of black holes)  
Fund: Project supported by the National Natural Science Foundation of China (Grant Nos. 11205254, 11178018, 11375279, and 11605015), the Fundamental Research Funds for the Central Universities, China (Grant Nos. 106112016CDJXY300002 and CDJRC10300003), the Chinese State Scholarship Fund, FAPESP (Grant No. 2012/08934-0), and the Natural Science Foundation Project of CQ CSTC (Grant No. 2011BB0052).
Corresponding Authors:  Jin Li     E-mail:  cqujinli1983@cqu.edu.cn

Cite this article: 

Hong Ma(马洪), Jin Li(李瑾) Gravitational quasi-normal modes of static R2 Anti-de Sitter black holes 2017 Chin. Phys. B 26 060401

[1] Perlmutter S, Aldering G, Goldhaber G, et al. 1999 Astrophys. J. 517 565
[2] Brian P, Nicholas B, Phillips M, et al. 1998 Astrophys. J. 507 46
[3] Adam G, Alexei V, Peter Challis, et al. 1998 Astron. J. 116 1009
[4] Riess A G, Strolger L G, John T, et al. 2004 Astrophys. J. 116 665
[5] Riess A G, Nugent P E, Gillil R L, et al. 2001 Astrophys. J. 560 49
[6] Perlmutter S, Turner M S and White M 1999 Phys. Rev. Lett. 83 670
[7] Bennett C L, Hill R, Hinshaw G, et al. 2003 Astrophys. J. 148 1
[8] Hinshaw G, Spergel D N, Verde L, et al. 2003 Astrophys. J. 148 135
[9] Cecotti S 1987 Phys. Lett. B 190 86
[10] Starobinsky A A 1980 Phys. Lett. B 91 99
[11] Stelle K S 1978 Gen. Rel. Grav. 9 353
[12] Guth A H 1981 Phys. Rev. D 23 347
[13] Mukhanov V 2005 Physical Foundations of Cosmology (London: Cambridge University Press) p. 42
[14] Stelle K S 1977 Phys. Rev. D 16 953
[15] Berti E, Cardoso V and Starinets A O 2009 Class. Quantum Grav. 26 163001
[16] Konoplya R A and Zhidenko A 2011 Rev. Mod. Phys. 83 793
[17] Berti E, Cardoso V and Will C M 2006 Phys. Rev. D 73 064030
[18] Regge T and Wheeler J A 1957 Phys. Rev. 108 1063
[19] Vishveshwara C V 1970 Nature 227 936
[20] Chandrasekhar S 1983 The Mathematical Theory of Black Holes (London: Oxford University Press) pp. 135-204
[21] Flachi A and Lemos J P S 2013 Phys. Rev. D 87 936024034
[22] Bronnikov K A and Konoplya R A 2012 Phys. Rev. D 86 024028
[23] Musiri S, Ness S and Siopsis G 2006 Phys. Rev. D 73 064001
[24] Cardoso V and Jose P S Lemos 2001 Class. Quantum Grav. 18 5257
[25] Cardoso V and Jose P S Lemos 2001 Phys. Rev. D 63 124015
[26] Moona T, Myungb Y S and Edwin J S 2011 arXiv: 1104.1908v2 [gr-qc]
[27] Myung Y S, Moon T and Edwin J S 2011 Phys. Rev. D 83 124009
[28] Li J, Ma H and Lin K 2013 Phys. Rev. D 88 064001
[29] Chen S B, Jing J L 2005 Chin. Phys. B 14 683
[30] Sharmanthie F 2005 Gen. Rel. Grav. 37 585
[31] Abbott B P, Abbott R, Abbott T D, et al. 2016 Phys. Rev. Lett. 116 061102
[32] Abbott B P, Abbott R, Abbott T D, et al. 2016 Phys. Rev. Lett. 116 241103
[33] Abbott B P, Abbott R, Abbott T D, et al. 2016 Phys. Rev. Lett. 116 221101
[34] Santos Oliván D and Sopuerta Carlos F 2016 Phys. Rev. Lett. 116 041101
[35] Lin K, Qian W L and Pavan A B 2016 Phys. Rev. D 94 064050
[36] Gary T H and Veronika E H 2000 Phys. Rev. D 62 024027
[37] Horowitz G T 2000 Class. Quantum Grav. D 17 1107
[38] Gundlach C, Richard H P and Pullin J 1994 Phys. Rev. D 49 883
[39] Gundlach C, Richard H P and Pullin J 1994 Phys. Rev. D 49 890
[40] Barth N H 1985 Class. Quantum Grav. 2 497
[41] Kounnas C, Lüst D and Toumbas N 2014 arXiv: 1409.7076 [hep-th]
[42] Stephani H, Kramer D, MacCallum M A H, Hoenselaers C and Herlt E 2003 Exact Solutions of Einstein's Field Equations (London: Cambridge University Press) p. 701
[43] Kehagias A, Kounnas C and Lust D 2015 arXiv: 1502.04192v2 [hep-th]
[44] Gundlach C, priee R H and Pullin J 1994 Phys. Rev. D 49 890
[45] Gundlach C, priee R H and Pullin J 1994 Phys. Rev. D 49 883
[46] Cardoso V, Jose' P S Lemos 2001 Phys. Rev. D 64 084017
[47] Pavan A B, Lima R S and Luís Filipe de Almeida Roque 2015 arXiv: 1510.04060 [hep-th]
[48] Li J and Zhong Y H 2013 Int. J. Theor. Phys. 52 1583
[49] Lin K, Li J and Yang N 2011 Gen. Relativ. Grav. 43 1889
[50] Gundlach C, Price R H and Pullin J 1994 Phys. Rev. D 49 883
[51] Maldacena J 1998 Adv. Theor. Math. Phys. 2 231
[52] Witten E 1998 Adv. Theor. Math. Phys. 2 253
[53] Gubser S S, Klebanov I R and Polyakov A M 1998 Phys. Lett. B 428 105
[54] Aharony O, Gubser S S and Maldacena J 2000 Phys. Rep. 323 183
[55] Gary T H and Veronika E H 2000 Phys. Rev. D 62 024027
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