Gravitational axial perturbations and quasinormal modes of loop quantum black holes

被引：26

作者：

Cruz, M. B. ^{[1
]}

Silva, C. A. S. ^{[2
]}

Brito, F. A. ^{[1
,3
]}

机构：

[1] Univ Fed Paraiba, Dept Fis, BR-58051970 Joao Pessoa, Paraiba, Brazil

[2] Inst Fed Educ Ciencia & Tecnol Paraiba IFPB, Campus Campina Grande, Joao Pessoa, Paraiba, Brazil

[3] Univ Fed Campina Grande, Dept Fis, Caixa Postal 10071, BR-58429900 Campina Grande, Paraiba, Brazil

来源：

EUROPEAN PHYSICAL JOURNAL C | 2019年 / 79卷 / 02期

关键词：

HAWKING RADIATION; STABILITY; QUANTIZATION; GEOMETRY;

D O I：

10.1140/epjc/s10052-019-6565-2

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

Loop quantum gravity (LQG) is a theory that proposes a way to model the behavior of the spacetime in situations where its atomic characteristic arises. Among these situations, the spacetime behavior near the Big Bang or black hole's singularity. The detection of gravitational waves, on the other hand, has opened the way to new perspectives in the investigation of the spacetime structure. In this work, by the use of a WKB method introduced by Schutz and Will (Astrophys J 291:L33, 1985), and after improved by Iyer and Will (Phys Rev D 35:3621, 1987), we study the gravitational wave spectrum emitted by loop quantum black holes, which correspond to a quantized version of the Schwarzschild spacetime by LQG techniques. From the results obtained, loop quantum black holes have been shown stable under axial gravitational perturbations.

引用

页数：10

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