Bogoliubov coefficients from scattering a scalar in a collapsing EM background (single copy of Vaidya) match ray-tracing results and connect to Hawking radiation through the double copy.
Hawking Radiation from Charged Black Holes via Gauge and Gravitational Anomalies
3 Pith papers cite this work. Polarity classification is still indexing.
abstract
Extending gr-qc/0502074, we show that in order to avoid a breakdown of general covariance and gauge invariance at the quantum level the total flux of charge and energy in each outgoing partial wave of a charged quantum field in a Reissner-Nordstrom black hole background must be equal to that of a (1+1) dimensional blackbody at the Hawking temperature with the appropriate chemical potential.
verdicts
UNVERDICTED 3representative citing papers
Thermal bath corrections derived via thermofield dynamics enhance the evaporation rate of primordial black holes, shortening their lifetimes relative to zero-temperature calculations.
Hawking temperatures for emergent gravity metrics of KN and KNAdS are calculated along θ=0, modified by dark energy from DBI k-essence fields, with metrics satisfying Einstein equations at large r.
citing papers explorer
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Hawking Radiation meets the Double Copy
Bogoliubov coefficients from scattering a scalar in a collapsing EM background (single copy of Vaidya) match ray-tracing results and connect to Hawking radiation through the double copy.
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Evaporation of Primordial Black Holes in a Thermal Universe: A Thermofield Dynamics Approach
Thermal bath corrections derived via thermofield dynamics enhance the evaporation rate of primordial black holes, shortening their lifetimes relative to zero-temperature calculations.
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The Hawking temperature in the context of dark energy for Kerr-Newman and Kerr-Newman-AdS backgrounds
Hawking temperatures for emergent gravity metrics of KN and KNAdS are calculated along θ=0, modified by dark energy from DBI k-essence fields, with metrics satisfying Einstein equations at large r.