Abstract
Dilaton black hole solutions in low energy string theory (well known as GMGHS black holes) have analogue black holes with a cosmological constant derived by Gao and Zhang. Here, we study quasi normal modes of this dilaton-de Sitter black hole under neutral scalar field perturbations. We have employed the sixth order WKB analysis to compute the quasi normal mode frequencies. A detailed study is done for the quasi normal mode frequencies by varying the parameters in the theory such as the mass, cosmological constant, dilaton charge and the spherical harmonic index. For the massive scalar field we observed that the usual quasi resonance modes that exists for asymptotically flat black holes do not exist for this particular black hole. We have approximated the scalar field potential of the near-extreme dilaton de Sitter black hole with the Pöschl-Teller potential and have presented exact quasi normal frequencies.
Similar content being viewed by others
References
Perlmutter, S., et al.: Measurements of \(\Omega \) and \(\Lambda \) from 42 high-redshift supernovae. Astrophys. J. 517, 565 (1999)
Riess, A.G., et al.: Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116 1009 (1998); BVRI light curves for 22 type Ia supernovae. Astron. J. 117, 707 (1999)
Spergel, D.N., et al.: (WMAP Collaboration), Wilkinson microwave anisotropy probe (WMAP) three year results: implications for cosmology. Astrophys. J. Suppl. 170, 377 (2007)
Tegmark, M., et al.: (SDSS collaboration) cosmological parameters from SDSS and WMAP. Phys. Rev. D 69, 103501 (2004)
Seljak, U., et al.: Cosmological parameter analysis including SDSS Ly\(\alpha \) forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy. Phys. Rev. D 71, 103515 (2005)
Witten, E.: Quantum gravity in de Sitter space. arXiv:hep-th/0106109
Dasguptha, K., Gwyn, R., McDonough, E., Mia, M., Tatar, R.: de Sitter vacua in type II B string theory: classical solutions and quantum corrections. JHEP 054, 1407 (2014)
Danielsson, U.H., Haque, S.S., Shiu, G., van Riet, T.: Towards classical de Sitter solutions in string theory. JHEP 0909, 114 (2009)
Gibbons, G.W., Maeda, K.: Black holes and membranes in higher dimensional theories with dilaton fields. Nuclear Phys. B 298, 741 (1988)
Garfinkle, D., Horowitz, G.T., Strominger, A.: Charged black holes in string theory. Phys. Rev. D 43, 3140 (1991)
Poletti, S.J., Wiltshire, D.L.: Global properties of static spherically symmetric charged dilaton spacetimes with a Liouville potential. Phys. Rev. D 50, 7260 (1994)
Gao, C.J., Zhang, S.N.: Dilaton black holes in de Sitter or anti-de Sitter universe. Phys. Rev. D 70, 124019 (2004)
Gates, S.J., Zwiebach, B.: Gauged N\(=\)4 supergravity theory with a new scalar potential. Phys. Lett. B 123, 200 (1983)
Zwiebach, B.: The inequivalent gauges of SO(4) supergravities. Nuclear Phys. B 238, 367 (1984)
Easther, R.: Exact superstring motivated cosmological models. Classic Quantum Gravity 10, 2203 (1993)
Dehghani, M.H., Bazrafshan, A.: Asymptotically AdS magnetic branes in \((n+1)\) dimensional dilaton gravity. Can. J. Phys. 89, 1163 (2011)
Sheykhi, A., Riazi, N., Mahzoon, M.H.: Asymptotically non-flat Einstein-Born-Infeld-dilaton black holes with Liouville-type potentials. Phy. Rev. D 74, 044025 (2006)
Chan, K.C.K., Horne, J.H., Mann, R.B.: Charged dilaton black holes with unusual asymptotics. Nuclear Phys. B 447, 441 (1995)
Ferrari, V., Gualtieri, L.: Quasi-normal modes and gravitational wave astronomy. Gen. Relativ. Gravit. 40, 945 (2008)
Morgan, J., Miranda, A.S., Zanchin, V.T.: Electromagnetic quasinormal modes of rotating black strings and the AdS/CFT correspondence. JHEP 03, 169 (2013)
Hod, S.: Bohr’s correspondence principle and the area spectrum of quantum black holes. Phys. Rev. Lett. 81, 4293 (1998)
Fernando, S.: Spinning dilaton black holes in 2+1 dimensions: quasinormal modes and the area spectrum. Phys. Rev. D 79, 124026 (2009)
Kunstatter, G.: d-Dimensional black hole entropy spectrum from quasi-normal modes. Phys. Rev. Lett 90, 161301 (2003)
Konoplya, R.A., Zhidenko, A.: Quasinormal modes of black holes: from astrophysics to string theory. Rev. Mod. Phys. 83, 793 (2011)
Ferrari, V., Pauri, M., Piazza, F.: Quasi-normal modes of charged, dilaton black holes. Phy. Rev. D 63, 064009 (2001)
Fernando, S., Arnold, K.: Scalar perturbations of charged dilaton black holes. Gen. Relativ. Gravit. 36, 1805 (2004)
Konoplya, R.A.: Decay of charged scalar field around a black hole: quasinormal modes of R-N, R-N-AdS and dilaton black holes. Phys. Rev. D 66, 084007 (2002)
Konoplya, R.A.: Quasinormal modes of the electrically charged dilaton black hole. Gen. Rewl. 34, 329 (2002)
Shu, F., Shen, Y.: Quasinormal modes of charged black holes in string theory. Phys. Rev. D 70, 084046 (2004)
Kokkotas, K.D., Konoplya, R.A., Zhidenko, A.: Bifurcation of the quasinormal spectrum of zero damped modes for rotating dilatonic black holes. arXiv:1507.05649
Iyer, S., Will, C.M.: Black-hole normal modes: a WKB approach. I. Foundations and application of a higher-order WKB analysis of potential-barrier scattering. Phys. Rev. D 35, 3621 (1987)
Konoplya, R.A.: Quasinormal behavior of the D-dimensional Schwarzschild black hole and higher order WKB approach. Phys. Rev. D 68, 024018 (2003)
Fernando, S.: Decay of massless Dirac field around the Born-Infeld black hole. Int. J. Mod. Phys. A 25, 669 (2010)
Fernando, S., Correa, J.: Quasi-normal modes of the Bardeen black hole: scalar perturbations. Phys. Rev. D 86, 64039 (2012)
Fernando, S., Clark, T.: Black holes in massive gravity: quasinormal modes of scalar perturbations. Gen. Relativ. Gravit. 46, 1834 (2014)
Horowitz, G.T., Hubeny, V.E.: Quasinormal modes of AdS black holes and the approach to thermal equilibrium. Phys. Rev. D 62, 024027 (2000)
Brady, P.R., Chambers, C.M., Krivan, W., Laguna, P.: Telling tails in the presence of a cosmological constant. Phys. Rev. D 55, 7538 (1997)
Fernando, S.: Regular black holes in de Sitter universe: scalar field perturbations and quasinormal modes, to appear in Int. J. Mod. Phys. D. arXiv:1508.03581
Gundlach, C., Price, R.H., Pullin, J.: Late-time behavior of stellar collapse and explosions: I linearized perturbations. Phys. Rev. D 49, 883 (1994)
Bronnikov, K.A., Konoplya, R.A., Zhidenko, A.: Instabilities of wormholes and regular black holes supported by a phantom scalar field. Phy. Rev. D 86, 024028 (2012)
Konoplya, R.A., Zhidenko, A.V.: Decay of massive scalar field in a Schwarzschild background. Phys. Lett. B 609, 377 (2005)
Ohashi, A., Sakagami, M.: Massive quasi-normal modes. Classic Quantum Gravity 21, 3973 (2004)
Chang, J., Huang, J., Shen, Y.: Quasi-resonent modes of massive scalar fields in Schwarzschild–de Sitter space-time. Int. J. Theor. Phys. 46, 2617 (2007)
Podolsky, J.: The structure of the extreme Schwarzschild–de Sitter space-time. Gen. Relativ. Gravit. 31, 1703 (1999)
Fernando, S.: Cold, ultracold and Nariai black holes with quintessence. Gen. Relativ. Gravit. 45, 2053 (2013)
Fernando, S.: Nariai black holes with quintessence. Mod. Phys. Lett. A 28, 13550189 (2013)
Fernando, S.: Born-Infeld-de Sitter gravity: cold, ultracold and Nariai black holes. Int. J. Mod. Phys. D 22, 1350080 (2013)
Matyjasek, J., Sadurski, P., Tryniecki, D.: Inside the degenerate horizons of the regular black holes. Phys. Rev. D 87, 124025 (2013)
Ferrari, V., Mashhoon, B.: New approach to the quasinormal modes of a black hole. Phys. Rev. D 30, 295 (1984)
Cardoso, V., Lemos, J.P.S.: Quasinormal modes of the near extremal Schwarzschild–de Sitter black hole. Phys. Rev. D 67, 084020 (2003)
Molina, C.: Quasinormal modes of d-dimensional spherical black holes with a near extreme cosmological constant. Phys. Rev. D 68, 064007 (2003)
Acknowledgments
The author wish to thank R. A. Konoplya for providing the Mathematica file for WKB approximation.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Fernando, S. Quasinormal modes of dilaton-de Sitter black holes: scalar perturbations. Gen Relativ Gravit 48, 24 (2016). https://doi.org/10.1007/s10714-016-2020-y
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10714-016-2020-y