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Some spacetimes containing non-rotating extremal isolated horizons

Oct, 2012

15 pages

Published in:

Class.Quant.Grav. 30 (2013) 145008

e-Print:

1210.6889 [gr-qc]

DOI:

10.1088/0264-9381/30/14/145008

View in:

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Abstract: (IOP)

Well-known results demonstrate the uniqueness of extremal isolated horizons (equivalently near-horizon spacetimes) in (3 + 1) dimensions. This paper briefly reviews some of these results and then explicitly constructs families of non-asymptotically flat, non-spherically symmetric spacetimes that nevertheless contain spherically symmetric extremal horizons that are isomorphic to those found in Reissner–Nordström spacetimes.

Note:

15 pages, 1 figure. V2: significant revision with compression and (hopefully) clarification of presentation, one appendix removed. Ultimate results are unchanged

04.20.-q
04.70.Bw
04.20.Jb
04.20.Ex
black hole: horizon
electromagnetic field

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Figures(1)

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