Abstract
In this paper, the modified Hawking temperature of a static Riemann space-time is studied using the generalized Klein–Gordon equation and the generalized Dirac equation. Applying the Kerner–Mann quantum tunneling method, the modified Hawking temperatures for scalar particles and fermions that cross the event horizon of the black hole have been derived. We observe that the quantum gravity effects reduce the rise of thermal radiation temperature of the black hole.
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