Investigating the Generalized Uncertainty Principle Effects on Hawking Radiation in Rotating Linear Dilaton Black Holes

TL;DR

This paper explores how the Generalized Uncertainty Principle influences Hawking radiation from rotating linear dilaton black holes, revealing that GUP modifies temperature and entropy, with implications for quantum gravity and astrophysics.

Contribution

It introduces a thermal emission model incorporating GUP effects in rotating linear dilaton black holes, highlighting their impact on Hawking temperature and entropy.

Findings

GUP decreases Hawking temperature as parameters increase

Hawking temperature rises with black hole mass

GUP effects have implications for the information loss paradox

Abstract

The impact of the Generalized Uncertainty Principle (GUP) on Hawking particle emission in a rotating linear dilaton black hole (RLDBH) spacetime is examined in this thesis. The concerned study presents a thermal emission model for black holes (BHs) that incorporates the influence of gravitational lens particles through GUP during the quantum tunneling process. The findings suggest that with GUP support, the temperature of Hawking radiation decreases as GUP parameters increase and rises with an increasing BH mass. The thesis also delves into the repercussions of these discoveries on the information loss paradox and adjusted entropy, while also exploring the potential utilization of astrophysical data to confirm GUP effects. In conclusion, our work underscores the significant role of GUP in the thermal emission of non-asymptotically flat (NAF), stationary BHs and its capacity to shed light on the intricate relationship between astrophysics and quantum gravity.