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Quasinormal Modes of Massless Scalar Field Perturbation in Reissner-Nordström-de Sitter Quintessence Spacetime

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Abstract

Using the WKB approximation method, the massless scalar quasinormal modes are studied in Reissner-Nordström-de Sitter quintessence spacetime. We analyze the effective potential and QNMs frequencies by varying angular harmonic index l, mass M, charge Q, quintessence energy b and cosmological constant L 2. The results show the effective potential and QNMs frequency are related to l, M, Q, b and L 2. Moreover, the b and L 2 can make the effective potential and QNMs frequency reduces.

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Acknowledgements

This work is supported in part by the Natural Science Foundation of China (Grant No. 11178018 ).

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  1. School of Physical Electronics, University of Electronic Science and Technology of China, Chengdu, People’s Republic of China

    Zhong-Wen Feng, Guo-Ping Li & Xiao-Tao Zu

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  1. Zhong-Wen Feng
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Correspondence to Zhong-Wen Feng.

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Feng, ZW., Li, GP. & Zu, XT. Quasinormal Modes of Massless Scalar Field Perturbation in Reissner-Nordström-de Sitter Quintessence Spacetime. Int J Theor Phys 55, 367–379 (2016). https://doi.org/10.1007/s10773-015-2669-0

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