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首页> 外文期刊>Astrophysics and Space Science >Massive scalar field quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle
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Massive scalar field quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle

机译：具有典型现象和缺陷立体角的黑洞的质量标量场拟正态模

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Using the third-order WKB approximation, we evaluate the quasinormal frequencies of massive scalar field perturbation around a black hole with quintessence-like matter and a deficit solid angle. The mass u of the scalar field plays an important role in studying the quasinormal frequencies. We find that as the scalar field mass increases when the other parameters are fixed, so do the real parts and the magnitudes of the imaginary parts of the quasinormal frequencies decrease. The imaginary parts are almost linearly related to the real parts. Keywords Quasinormal frequencies - WKB approximation - Quintessence - Deficit solid angle PACS 04.30.-w - 97.60.Lf - 04.62.+v
机译：使用三阶WKB逼近，我们评估了具有典型现象和缺陷立体角的黑洞周围大质量标量场摄动的准正规频率。标量场的质量u在研究准法向频率中起着重要作用。我们发现，当其他参数固定时，随着标量场质量的增加，准法向频率的实部和虚部的量级也会减小。虚部几乎与实部线性相关。准准频率-WKB近似-精粹-赤字立体角PACS 04.30.-w-97.60.Lf-04.62。+ v

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