Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime

doi:10.1088/1674-1056/19/6/060401

中国物理B ›› 2010, Vol. 19 ›› Issue (6): 60401-060401.doi: 10.1088/1674-1056/19/6/060401

Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime

陈菊华, 王永久

College of Physics and Information Science, Hunan Normal University, Changsha 410081, China

收稿日期:2009-08-08 出版日期:2010-06-15 发布日期:2010-06-15
基金资助:
Project supported by the National Natural Science Foundation of China (Grant No.~10873004), the Key Project of the National Natural Science Foundation of China (Grant No.~10935013), the Scientific Research Fund of the Educational Department of Hunan Pro

Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime

Chen Ju-Hua(陈菊华)^† and Wang Yong-Jiu(王永久)

College of Physics and Information Science, Hunan Normal University, Changsha 410081, China

Received:2009-08-08 Online:2010-06-15 Published:2010-06-15
Supported by:
Project supported by the National Natural Science Foundation of China (Grant No.~10873004), the Key Project of the National Natural Science Foundation of China (Grant No.~10935013), the Scientific Research Fund of the Educational Department of Hunan Pro

摘要/Abstract

摘要： In this paper, using the third-order WKB approximation, we investigate the quasinormal frequencies of the scalar field in the background of a five-dimensional Lovelock black hole. We find that the ultraviolet correction to Einstein theory in the Lovelock theory makes the scalar field decay more slowly and oscillate more quickly, and the cosmological constant makes the scalar field decay more slowly and oscillate more slowly in the Lovelock black hole background.

Abstract: In this paper, using the third-order WKB approximation, we investigate the quasinormal frequencies of the scalar field in the background of a five-dimensional Lovelock black hole. We find that the ultraviolet correction to Einstein theory in the Lovelock theory makes the scalar field decay more slowly and oscillate more quickly, and the cosmological constant makes the scalar field decay more slowly and oscillate more slowly in the Lovelock black hole background.

Key words: quasinormal modes, third-order WKB approximation, Lovelock black hole

中图分类号: (Quantum aspects of black holes, evaporation, thermodynamics)

04.70.Dy

98.80.Jk (Mathematical and relativistic aspects of cosmology) 04.60.-m (Quantum gravity)

陈菊华, 王永久. Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime[J]. 中国物理B, 2010, 19(6): 60401-060401.

Chen Ju-Hua(陈菊华) and Wang Yong-Jiu(王永久). Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime[J]. Chin. Phys. B, 2010, 19(6): 60401-060401.

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Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime

Quasinormal modes of the scalar field in five-dimensional Lovelock black hole spacetime

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