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arXiv 2102.06303hep-thgr-qc
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Bumblebee引力模型中类Kerr黑洞的灰体辐射和拟正规模

Greybody Radiation and Quasinormal Modes of Kerr-like Black Hole in Bumblebee Gravity Model

Sara Kanzi, İzzet Sakallı

摘要:

在Lorentz对称性破缺(LSB)框架下,研究了由大黄蜂引力模型得到的类Kerr黑洞时空的准正规模(QNM)和灰体因子(GF).特别地,我们在半解析WKB方法和时域方法的框架内分析了黑洞的标量和费米子扰动。详细研究了LSB对类Kerr黑洞玻色子/费米子QNM和GFs的影响。所得结果以图形方式描绘和讨论。

英文摘要:

In the framework of the Lorentz symmetry breaking (LSB), we investigate the quasinormal modes (QNMs) and the greybody factors (GFs) of the Kerr-like black hole spacetime obtained from the bumblebee gravity model. In particular, we analyze the scalar and fermionic perturbations of the black hole within the framework of both semi-analytic WKB method and the time domain approach. The impacts of the LSB on the bosonic/fermionic QNMs and GFs of the Kerr-like black hole are investigated in detail. The obtained results are graphically depicted and discussed.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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