Non-commutative black hole solutions derived via Seiberg-Witten map on potentials exhibit eliminated temperature divergence, phase transitions, and stable Planck-mass remnants proposed as gravitational dark matter.
Energy Conservation and Hawking Radiation
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abstract
The conservation of energy implies that an isolated radiating black hole cannot have an emission spectrum that is precisely thermal. Moreover, the no-hair theorem is only approximately applicable. We consider the implications for the black hole information puzzle.
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UNVERDICTED 4representative citing papers
Spin-dependent particle creation densities, greybody factors, absorption cross sections, and evaporation lifetimes are computed for scalar, vector, tensor, and spinorial modes around black holes in f(R,T) gravity.
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.
Using a deformed dispersion relation, the Hawking temperature and tunneling rate for fermions from non-stationary Kerr black holes receive corrections dependent on the horizon's angular parameters.
citing papers explorer
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New Construction of Black Hole Solution in Non-Commutative Geometry and Their Thermodynamic Properties
Non-commutative black hole solutions derived via Seiberg-Witten map on potentials exhibit eliminated temperature divergence, phase transitions, and stable Planck-mass remnants proposed as gravitational dark matter.
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Spin effects on particle creation and evaporation in $f(R,T)$ gravity
Spin-dependent particle creation densities, greybody factors, absorption cross sections, and evaporation lifetimes are computed for scalar, vector, tensor, and spinorial modes around black holes in f(R,T) gravity.
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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.
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Modified Fermions Tunneling Radiation from Non-stationary, Axially Symmetric Kerr Black Hole
Using a deformed dispersion relation, the Hawking temperature and tunneling rate for fermions from non-stationary Kerr black holes receive corrections dependent on the horizon's angular parameters.