GUP parameter and black-hole temperature

¹ Theoretical Physics Group, Department of Physics, Kuwait University - P.O. Box 5969, Safat 13060, Kuwait
² Department of Physics and Astronomy, King Saud University - Riyadh 11451, Saudi Arabia
³ Netherlands Institute for Advanced Study - Korte Spinhuissteeg 3, 1012 CG Amsterdam, The Netherlands
⁴ Department of Physics, Faculty of Science, Benha University - Benha, 13518, Egypt

^(a) elias.vagenas@ku.edu.kw
^(b) salwams@ksu.edu.sa
^(c) ahmed.ali@fsc.bu.edu.eg

Received: 2 November 2017
Accepted: 11 January 2018

Abstract

Motivated by a recent work of Scardigli, Lambiase and Vagenas (SLV), we derive the GUP parameter, i.e., , when the GUP has a linear and quadratic term in momentum. The value of the GUP parameter is obtained by conjecturing that the GUP-deformed black-hole temperature of a Schwarzschild black hole and the modified Hawking temperature of a quantum-corrected Schwarzschild black hole are the same. The leading term in both cases is the standard Hawking temperature and since the corrections are considered as thermal, the modified and deformed expressions of temperature display a slight shift in the Hawking temperature. Finally, by equating the first correction terms, we obtain a value for the GUP parameter. In our analysis, the GUP parameter is not a pure number but depends on the ratio with the Planck mass and M the black-hole mass.