Asymptotically Einstein de Sitter cosmological black holes and the problem of energy conditions

Details Asymptotically Einstein de Sitter cosmological black holes and the problem of energy conditions Asymptotically Einstein de Sitter cosmological black holes and the problem of energy conditions

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cqgra..23.1971m&link_type=abstract

Classical and Quantum Gravity, Volume 23, Issue 6, pp. 1971-1987 (2006).

Mathematics

Logic

17

Scientific paper

It is shown that previous asymptotically Einstein de Sitter cosmological black hole spacetimes violate the energy conditions in some region of spacetime. Thus, cosmological black hole spacetimes (for the Schwarzschild and Reissner Nordström cases) are obtained that satisfy the energy conditions throughout spacetime. The solutions are obtained by performing conformal transformations on the isotropic forms of the isolated black hole metrics.

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