The stochastic charge correction to Hawking e± emission, previously derived semi-classically, is shown here to arise from QED, with a net correction below 2%.
(C11) from Vasquezet al.[1] for δϵ(h − h′) which resembles that of a Dirac delta function in the limit whereϵ is small
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Corrections to Hawking radiation from asteroid-mass primordial black holes: analytic and numerical evaluation of the stochastic charge effect
The stochastic charge correction to Hawking e± emission, previously derived semi-classically, is shown here to arise from QED, with a net correction below 2%.