TY - JOUR

T1 - Hawking radiation from cubic and quartic black holes via tunneling of GUP corrected scalar and fermion particles

AU - Javed, Wajiha

AU - Babar, Rimsha

AU - Övgün, Ali

N1 - Funding Information:
A.Ö. acknowledges financial support provided under the Chilean FONDECYT Grant No. 3170035. The authors thank an anonymous referees for their useful suggestions that helped improve the paper.
Publisher Copyright:
© 2019 World Scientific Publishing Company.

PY - 2019/3/21

Y1 - 2019/3/21

N2 - We analyze the effect of the generalized uncertainty principle (GUP) on the Hawking radiation from the hairy black hole in U(1) gauge-invariant scalar-vector-tensor theory by utilizing the semiclassical Hamilton-Jacobi method. To do so, we evaluate the tunneling probabilities and Hawking temperature for scalar and fermion particles for the given spacetime of the black holes with cubic and quartic interactions. For this purpose, we utilize the modified Klein-Gordon equation for the Boson particles and then Dirac equations for the fermion particles, respectively. Next, we examine that the Hawking temperature of the black holes do not depend on the properties of tunneling particles. Moreover, we present the corrected Hawking temperature of scalar and fermion particles which look similar in both interactions, but there are different mass and momentum relationships for scalar and fermion particles in cubic and quartic interactions.

AB - We analyze the effect of the generalized uncertainty principle (GUP) on the Hawking radiation from the hairy black hole in U(1) gauge-invariant scalar-vector-tensor theory by utilizing the semiclassical Hamilton-Jacobi method. To do so, we evaluate the tunneling probabilities and Hawking temperature for scalar and fermion particles for the given spacetime of the black holes with cubic and quartic interactions. For this purpose, we utilize the modified Klein-Gordon equation for the Boson particles and then Dirac equations for the fermion particles, respectively. Next, we examine that the Hawking temperature of the black holes do not depend on the properties of tunneling particles. Moreover, we present the corrected Hawking temperature of scalar and fermion particles which look similar in both interactions, but there are different mass and momentum relationships for scalar and fermion particles in cubic and quartic interactions.

KW - Effective Hawking temperature

KW - modified Dirac equation

KW - modified Klein-Gordon

UR - http://www.scopus.com/inward/record.url?scp=85062354226&partnerID=8YFLogxK

U2 - 10.1142/S0217732319500573

DO - 10.1142/S0217732319500573

M3 - Article

AN - SCOPUS:85062354226

VL - 34

JO - Modern Physics Letters A

JF - Modern Physics Letters A

SN - 0217-7323

IS - 9

M1 - 1950057

ER -