首页|Quasinormal modes and ringdown waveforms of a Frolov black hole

Quasinormal modes and ringdown waveforms of a Frolov black hole

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In this paper we investigate scalar perturbation over a Frolov black hole(BH),which is a regular BH induced by the quantum gravity effect.The quasinormal frequencies of a scalar field always consistently reside in the lower half-plane,and the time-domain evolution of the field demonstrates a decaying behavior,with the late-time tail exhibiting a power-law pattern.These observations collectively suggest the stability of a Frolov BH against scalar perturbation.Additionally,our study reveals that the quantum gravity effect leads to slower decay modes.For the case of the angular quantum number l=0,the oscillation exhibits non-monotonic behavior with the quantum gravity parameter α0.However,once l≥1,the angular quantum number surpasses the influence of the quantum gravity effect.

quasinormal modesblack holeFrolov black holequantum gravity effects

Zhijun Song、Huajie Gong、Hai-Li Li、Guoyang Fu、Li-Gang Zhu、Jian-Pin Wu

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Center for Gravitation and Cosmology,College of Physical Science and Technology,Yangzhou University,Yangzhou 225009,China

Basic Teaching Department,Shenyang Institute of Engineering,Shenyang 110136,China

Department of Physics and Astronomy,Shanghai Jiao Tong University,Shanghai 200240,China

National Key R&D Program of ChinaNatural Science Foundation of ChinaNatural Science Foundation of ChinaNatural Science Foundation of ChinaPostgraduate Research & Practice Innovation Program of Jiangsu ProvinceScientific Research Funding Project of the Education Department of Liaoning ProvinceNatural Science Foundation of Liaoning Province of China

2020YFC2201400123750551234715912305068KYCX22_3451JYTQN20230902023-BSBA-229

2024

理论物理通讯(英文版)
中国科学院理论物理研究所 中国物理学会

理论物理通讯(英文版)

CSTPCD
影响因子:0.333
ISSN:0253-6102
年,卷(期):2024.76(10)