摘要
This study set out to investigate charged vector particles tunneling via horizons of a pair of accelerating rotating charged NUT black holes under the influence of quantum gravity.To this end,we use the modified Proca equation incorporating generalized uncertainty principle.Applying the WKB approximation to the field equation,we obtain a modified tunneling rate and the corresponding corrected Hawking temperature for this black hole.Moreover,we analyze the graphical behavior of the corrected Hawking temperature T'_H with respect to the event horizon for the given black hole.By considering quantum gravitational effects on Hawking temperatures,we discuss the stability analysis of this black hole.For a pair of black holes,the temperature T'_H increases with the increase in rotation parameters a andω,correction parameterβ,black hole acceleration a,and arbitrary parameter k,and decreases with the increase in electric e and magnetic charges g.
This study set out to investigate charged vector particles tunneling via horizons of a pair of accelerating rotating charged NUT black holes under the influence of quantum gravity.To this end,we use the modified Proca equation incorporating generalized uncertainty principle.Applying the WKB approximation to the field equation,we obtain a modified tunneling rate and the corresponding corrected Hawking temperature for this black hole.Moreover,we analyze the graphical behavior of the corrected Hawking temperature T’_H with respect to the event horizon for the given black hole.By considering quantum gravitational effects on Hawking temperatures,we discuss the stability analysis of this black hole.For a pair of black holes,the temperature T’_H increases with the increase in rotation parameters a and ω,correction parameter β,black hole acceleration a,and arbitrary parameter k,and decreases with the increase in electric e and magnetic charges g.
基金
financial support provided under the Chilean FONDECYT(3170035)
