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首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >Quasinormal modes of black holes in Einstein-power-Maxwell theory
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Quasinormal modes of black holes in Einstein-power-Maxwell theory

机译:爱因斯坦 - 力量 - 麦克斯韦理论中的黑洞的新势在量

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In the present work, we compute the spectrum of quasinormal frequencies of four-dimensional (4D) charged black holes (BHs) in Einstein-power-Maxwell (EpM) theory. In particular, we study scalar perturbations adopting the sixth-order WKB approximation. We analyze in detail, the behavior of the spectrum depending on the charge of the BH, the quantum number of angular momentum and the overtone number. In addition, a comparison is made between the results obtained here and the results valid for charged BHs in other theories as well as for the Reissner-Nordstrom BH. Finally, we have provided an analytical expression for the quasinormal spectrum in the eikonal limit.
机译:在本作工作中,我们在爱因斯坦 - Power-Maxwell(EPM)理论中计算四维(4D)带电黑洞(BHS)的四维频率的谱。 特别是,我们研究采用第六阶WKB近似的标量扰动。 我们详细分析,频谱的行为取决于BH的电荷,量子数的角动量和隆起数。 此外,在此获得的结果之间进行了比较,结果对于其他理论中的带电BHS有效,以及Reissner-Nordstrom BH。 最后,我们已经为eikonal极限的Quasinormal频谱提供了分析表达。

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