Fermions Tunneling and Quantum Corrections for Quintessential Kerr-Newman-AdS Black Hole

Abstract

This paper is devoted to study charged fermion particles tunneling through the horizon of Kerr-Newman-AdS black hole surrounded by quintessence by using Hamilton-Jacobi ansatz. In our analysis, we investigate Hawking temperature as well as quantum corrected Hawking temperature on account of generalized uncertainty principle. Moreover, we discuss the effects of correction parameter $\beta$ on the corrected Hawking temperature $T_{e-H}$, graphically. We conclude that the temperature $T_{e-H}$ vanishes when $\beta =\mathrm{100}$, whereas for $\beta <\mathrm{100}$ and $\beta >\mathrm{100}$, the temperature turns out to be positive and negative, respectively. We observe that the graphs of $T_{e-H}$ w.r.t. quintessence parameter $\alpha$ exhibit behavior only for the particular ranges, i.e., $\mathrm{0}<\alpha <\mathrm{1}/\mathrm{6}$, charge $\mathrm{0}<Q\le \mathrm{1}$, and rotation parameter $\mathrm{0}<a\le \mathrm{1}$. For smaller and larger values of negative $\mathrm{\Lambda }$, as horizon increases, the temperature decreases and increases, respectively.