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• W1898656887 abstract "The current scenario of black hole evaporation holds that the Hawking energy flux $F$ is powered by pair creation at the horizon. However, pair creation produces entanglements, some of which must necessarily be broken before the black hole evaporates completely. That leads to loss of information and violation of unitarity. In this paper, an alternative scenario is suggested that reproduces the essential features of Hawking evaporation, but does not invoke pair creation with its attendant problems. In this accreting Boulware scenario, a positive flux $F$ is still an outflux at infinity, but near the horizon it becomes an influx of negative energy. This negative energy flux (marginally) satisfies the Flanagan energy inequality." @default.
• W1898656887 created "2016-06-24" @default.
• W1898656887 creator A5089991267 @default.
• W1898656887 date "2015-04-09" @default.
• W1898656887 modified "2023-09-27" @default.
• W1898656887 title "Shenanigans at the black hole horizon: pair creation or Boulware accretion?" @default.
• W1898656887 hasPublicationYear "2015" @default.
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