Scalar radiation emitted by a source around a spherically symmetric black hole

被引：1

作者：

Bernar, Rafael P. ^{[1
]}

机构：

[1] Univ Fed Para, Fac Fis, BR-66075110 Belem, Para, Brazil

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2020年 / 29卷 / 11期

关键词：

Gravitational wares; static spacetime; circular motion; QUASI-NORMAL MODES; SCHWARZSCHILD;

D O I：

10.1142/S0218271820410084

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We analyze the scalar radiation emitted by a source in a circular geodesic orbit around a spherically symmetric black hole. The black hole (BH) spacetime considered is quite general, in the sense that it encompasses the solutions of Schwarzschild and ReissnerNordstrom, and also the Bardeen solution of a regular BH. We use the framework of quantum field theory in curved spaces to compute the one-particle emission amplitude of scalar particles and related quantities.

引用

页数：15

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