What is the fate of a black hole embedded in an expanding universe ?
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چکیده
Within a large class of exact solutions of the Einstein equations describing a black hole embedded in a Friedmann universe it is shown that, under certain assumptions, only those with comoving Hawking-Hayward quasi-local mass are generic, in the sense that they are late-time attractors. PACS: 04.70.Bw, 04.20.Jb, 04.50.+h
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تاریخ انتشار 2008