Abstract

Different deformations and modifications have been proposed in the Kerr black hole solution. In the so-called non-Kerr metric a deformation function was proposed. This approach has been generalized to include two different deformation functions to obtain the CPR black hole (Cardoso et al. in Phys Rev D 89:064007, 2014). In this letter we develop the accelerating version of this spacetime and study its thermodynamics.

Details

Title
The CPR black hole with acceleration
Author
Gillani, Usman A 1 ; Saifullah Khalid 2   VIAFID ORCID Logo 

1  Quaid-i-Azam University, Department of Mathematics, Islamabad, Pakistan (GRID:grid.412621.2) (ISNI:0000 0001 2215 1297); National University of Technology, NUSASH Department, Islamabad, Pakistan (GRID:grid.512654.1) (ISNI:0000 0004 7535 8904) 
2  Quaid-i-Azam University, Department of Mathematics, Islamabad, Pakistan (GRID:grid.412621.2) (ISNI:0000 0001 2215 1297) 
Publication year
2021
Publication date
Sep 2021
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
DOI
https://doi.org/10.1140/epjc/s10052-021-09641-4
ProQuest document ID
2575157261
Copyright
© The Author(s) 2021. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.