Charged fermions tunneling from stationary axially symmetric black holes with generalized uncertainty principle

被引：9

作者：

Rizwan, Muhammad ^{[1
,2
]}

Ali, Muhammad Zubair ^{[3
]}

Ovgun, Ali ^{[4
,5
]}

机构：

[1] Natl Univ Modern Languages, Fac Engn & Comp Sci, Dept Comp Sci, H-9, Islamabad, Pakistan

[2] Natl Univ Sci & Technol, Sch Nat Sci, H-12, Islamabad, Pakistan

[3] Univ Waikato, Fac Computat & Math Sci, Dept Math & Stat, Hamilton 3216, New Zealand

[4] Pontificia Univ Catolica Valparaiso, Inst Fis, Casilla 4950, Valparaiso, Chile

[5] Eastern Mediterranean Univ, Phys Dept, Arts & Sci Fac, Via Mersin 10, Famagusta, North Cyprus, Turkey

来源：

MODERN PHYSICS LETTERS A | 2019年 / 34卷 / 23期

关键词：

Black holes; Hawking radiation; black hole thermodynamics; black hole temperature; modified Dirac equation; Hamilton-Jacobi method; WKB approximation; HAWKING RADIATION; QUANTUM-GRAVITY; MINIMAL LENGTH; PARTICLES; ENTROPY;

D O I：

10.1142/S0217732319501840

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, we study the tunneling of charged fermions from the stationary axially symmetric black holes using the generalized uncertainty principle (GUP) via Wentzel, Kramers, and Brillouin (WKB) method. The emission rate of the charged fermions and corresponding modified Hawking temperature of Kerr-Newman black hole, Einstein-axwell-dilaton-axion (EMDA) black hole, Kaluza-Klein dilaton black hole, and then, charged rotating black string are obtained and we show that the corrected thermal spectrum is not purely thermal because of the minimal scale length which cause the black hole's remnant.

引用

页数：15

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