Quasilocal energy of a rotating object described by Kerr spacetime
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DOI: 10.1103/physrevd.98.104051
Abstract: The Brown-York quasi-local energy of a rotating black hole described by the Kerr metric and enclosed by a fixed-radius surface is calculated by direct computation. No special assumptions on the angular momentum or the radial… read more here.
Keywords: rotating object; object described; quasilocal energy; energy rotating ... See more keywords