Tunneling Glashow-Weinberg-Salam Model Particles from Black Hole Solutions in Rastall Theory

被引：39

作者：

Ovgun, Ali ^{[1
,2
]}

Javed, Wajiha ^{[3
]}

Ali, Riasat ^{[3
]}

机构：

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

[2] Eastern Mediterranean Univ, Arts & Sci Fac, Phys Dept, Mersin 10, Famagusta, Northern Cyprus, Turkey

[3] Univ Educ, Div Sci & Technol, Township Campus, Lahore, Pakistan

来源：

ADVANCES IN HIGH ENERGY PHYSICS | 2018年 / 2018卷

关键词：

GENERALIZED UNCERTAINTY PRINCIPLE; HAWKING RADIATION; QUANTUM-GRAVITY; MINIMAL LENGTH; KERR; TEMPERATURE; RINDLER;

D O I：

10.1155/2018/3131620

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：

Using the semiclassical WKB approximation and Hamilton-Jacobi method, we solve an equation of motion for the Glashow-Weinberg-Salam model, which is important for understanding the unified gauge-theory of weak and electromagnetic interactions. We calculate the tunneling rate of the massive charged W-bosons in a background of electromagnetic field to investigate the Hawking temperature of black holes surrounded by perfect fluid in Rastall theory. Then, we study the quantum gravity effects on the generalized Proca equation with generalized uncertainty principle (GUP) on this background. We show that quantum gravity effects leave the remnants on the Hawking temperature and the Hawking radiation becomes nonthermal.

引用

页数：11

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