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On Radiative Fluxes and Coulombic Charges in the Balance Law for Black Hole Evaporation
In asymptotically-flat spacetimes, there is a clear distinction between radiative fluxes and Coulombic charges. Using the Wald-Zoupas prescription, we identify the classical radiative flux of a massless scalar field in 3+1 dimensions. In a spherically-symmetric model of black hole evaporation, the b
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