On modified Hawking radiation under quantum gravity effects in the fermion sector
In this letter, after briefly discussing Hawking radiation (HR) as quantum tunneling, we emphasize that special care must be taken when computing temperature corrections in the presence of Lorentz invariance violation (LIV), particularly by ensuring consistency between the modified dispersion relation and the gamma matrix structure used to describe fermions that are tunneling. We present a consistent implementation of such corrections in static, spherically symmetric black hole (BH) spacetimes. As the conserved Killing energy $ω= p_μξ^μ$ in a stationary, asymptotically flat spacetime corresponds to the particle's energy measured by an observer at infinity, one might expect LIV terms that increase (decrease) the energy of a free particle, as defined in the local spacetime frame, to lead to a corresponding increase (decrease) in the Hawking temperature. We discuss the conditions under which this expectation holds. We also determined the changes in Bekenstein-Hawking entropy for Schwarzschild-like BHs, including corrections from LIV scenarios.