Research ArticleNo Access

Evaporation of black hole under the effect of quantum gravity

Riasat Ali

https://orcid.org/0000-0002-9371-1113

Department of Mathematics, GC University Faisalabad Layyah Campus, Layyah 31200, Pakistan

E-mail Address: riasatyasin@gmail.com

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Rimsha Babar

Division of Science and Technology, University of Education, Vehari, Lahore 54590, Pakistan

E-mail Address: rimsha.babar10@gmail.com

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Muhammad Asgher

Department of Mathematics, The Islamia University of Bahawalpur, Bahawalpur 63100, Pakistan

E-mail Address: m.asgher145@gmail.com

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, and

Syed Asif Ali Shah

Department of Mathematics and Statistics, The University of Lahore, 1-Km Raiwind Road, Sultan Town, Lahore 54000, Pakistan

E-mail Address: asifalishah695@gmail.com

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https://doi.org/10.1142/S0219887822500177Cited by:12 (Source: Crossref)

Abstract

This paper provides an extension for Hawking temperature of Reissner–Nordström-de Sitter (RN-DS) black hole (BH) with global monopole as well as $5$ $5$ D charged black hole. We consider the black holes metric and investigate the effects of quantum gravity ( $α$ $α$ ) on Hawking radiation. We investigate the charged boson particles tunneling through the horizon of black holes by using the Hamilton–Jacobi ansatz phenomenon. In our investigation, we study the quantum radiation to analyze the Lagrangian wave equation with generalized uncertainty principle and calculate the modified Hawking temperatures for black holes. Furthermore, we analyze the charge and correction parameter effects on the modified Hawking temperature and examine the stable and unstable condition of RN-DS BH with global monopole as well as $5$ $5$ D charged black hole.

Keywords:

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