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- W1970032971 abstract "We argue that a process where a fuzzy space splits in two others can be used to explain the origin of the black hole entropy, and why a generalized second law of thermodynamics appears to hold in the presence of black holes. We reach the Bekenstein-Hawking formula from the count of the microstates of a black hole modeled by a fuzzy space. In this approach, a discrete area spectrum for the black hole, which becomes increasingly spaced as the black hole approaches the Planck scale, is obtained. We show that, as a consequence of this, the black hole radiation becomes less and less entropic as the black hole evaporates, in a way that some information about its initial state could be recovered." @default.
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- W1970032971 date "2011-09-21" @default.
- W1970032971 modified "2023-10-05" @default.
- W1970032971 title "A note on black-hole entropy, area spectrum, and evaporation" @default.
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- W1970032971 doi "https://doi.org/10.1209/0295-5075/96/10007" @default.
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