Scalar's quasibound states in cosmological black hole background

被引：2

作者：

Senjaya, David ^{[1
]}

机构：

[1] Chulalongkorn Univ, Fac Sci, Dept Phys, High Energy Phys Theory Grp, 254 Phayathai Rd, Bangkok 10330, Thailand

来源：

JOURNAL OF HIGH ENERGY ASTROPHYSICS | 2024年 / 43卷

关键词：

Black hole; de-Sitter space-time; Klein-Gordon equation; Quasibound states; NORMAL-MODES; FREQUENCIES;

D O I：

10.1016/j.jheap.2024.07.004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this letter, we present in detail a novel exact solution of scalar quasibound states of a static spherically symmetric Schwarzschild de Sitter black hole. We investigate and work out the governing covariant scalar field wave equation, i.e., the Klein-Gordon equation and isolate the radial equation. In this letter, we show in detail, the derivation of the successfully obtained exact radial wave solutions which are expressed in terms of General Heun functions. Having the exact solutions in hand, the energy levels expression is obtained from special function's polynomial condition. In the last part, the Hawking radiation is investigated via the Damour-Ruffini method and the Hawking temperature is obtained from radiation distribution function.

引用

页码：132 / 139

页数：8

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