Quantum tunneling from three-dimensional black holes

被引：38

作者：

Ejaz, Asiya ^{[1
]}

Gohar, H. ^{[1
]}

Lin, Hai ^{[2
,3
,4
]}

Saifullah, K. ^{[1
,2
,3
,5
]}

Yau, Shing-Tung ^{[2
,3
,4
]}

机构：

[1] Quaid I Azam Univ, Dept Math, Islamabad, Pakistan

[2] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA

[3] Harvard Univ, Ctr Fundamental Laws Nat, Cambridge, MA 02138 USA

[4] Harvard Univ, Dept Math, Cambridge, MA 02138 USA

[5] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA

来源：

PHYSICS LETTERS B | 2013年 / 726卷 / 4-5期

关键词：

RADIATION;

D O I：

10.1016/j.physletb.2013.09.015

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study Hawking radiation from three-dimensional black holes. For this purpose the emission of charged scalar and charged fermionic particles is investigated from charged BTZ black holes, with and without rotation. We use the quantum tunneling approach incorporating WKB approximation and spacetime symmetries. Another class of black holes which is asymptotic to a Sol three-manifold has also been investigated. This procedure gives us the tunneling probability of outgoing particles, and we compute the temperature of the radiation for these black holes. We also consider the quantum tunneling of particles from black hole asymptotic to Sol geometry. (C) 2013 Elsevier B.V. All rights reserved.

引用

页码：827 / 833

页数：7

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