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• W3196367776 abstract "Assuming that the vacuum energy-momentum tensor is not exceptionally large, we consider 4D evaporating black holes with spherical symmetry and evaluate the proper distance $Delta L$ between the time-like apparent horizon and the surface of the collapsing matter after it has entered the apparent horizon. We show that $Delta L$ can never be larger than $mathcal{O}(n^{3/2}ell_p)$ when the black hole is evaporated to $1/n$ of its initial mass, as long as $n ll a^{2/3}/ell_p^{2/3}$ (where $a$ is the Schwarzschild radius and $ell_p$ is the Planck length). For example, the distance between the matter and the apparent horizon must be Planckian at the Page time." @default.
• W3196367776 created "2021-09-13" @default.
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• W3196367776 date "2021-09-02" @default.
• W3196367776 modified "2023-10-17" @default.
• W3196367776 title "Distance between collapsing matter and apparent horizon in evaporating black holes" @default.
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• W3196367776 doi "https://doi.org/10.1103/physrevd.104.064005" @default.
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