Fermions Analysis of IR modified Horava-Lifshitz gravity: Tunneling and Perturbation Perspectives

TL;DR

This paper explores fermionic Hawking radiation and quasinormal modes in IR modified Hořava-Lifshitz gravity, revealing consistency with thermodynamics and longer-lived fermionic perturbations compared to Schwarzschild black holes.

Contribution

It provides the first detailed analysis of fermions tunneling and quasinormal modes in IR modified Hořava-Lifshitz gravity, including numerical calculations of mode frequencies.

Findings

Fermions tunneling results agree with thermodynamic calculations.

Fermions quasinormal modes have longer lifetimes than in Schwarzschild black holes.

Fermions perturbations exhibit higher frequencies and smaller damping rates.

Abstract

In this paper, we investigate the fermions Hawking radiation and quasinormal modes in infra-red modified Ho$\check{r}$ava-Lifshitz gravity under tunneling and perturbation perspectives.Firstly, through the fermions tunneling in IR modified Ho$\check{r}$ava-Lifshitz gravity,we obtain the Hawking radiation emission rate, tunneling temperature and entropy for the Kehagias-Sfetsos black hole. It is found that the results of fermions tunneling are in consistence with the thermodynamics results obtained by calculating surface gravity.Secondly, we numerically calculate the lowing quasinormal modes frequencies of fermions perturbations by using WKB formulas including the third orders and the sixth orders approximations simultaneously. It turns out that the actual frequency of fermions perturbation is larger than in the Schwarzschild case, and the damping rate is smaller than for the pure Schwarzschild. The resluts of fermions perturbation suggest the quasinormal modes could be lived more longer in Ho$\check{r}$ava-Lifshitz gravity.