Embedding a Schwarzschild black hole in a Hernquist dark matter halo suppresses particle creation rates, changes scattering cross sections, and alters null and timelike geodesics relative to the vacuum case.
An effective black hole remnant via infinite evaporation time due to generalized uncertainty principle.Journal of High Energy Physics, 2018(10):1–11
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Particle production, absorption, scattering, and geodesics in a Schwarzschild-Hernquist black hole
Embedding a Schwarzschild black hole in a Hernquist dark matter halo suppresses particle creation rates, changes scattering cross sections, and alters null and timelike geodesics relative to the vacuum case.