Timelike limit surfaces, apparent horizons and event horizons of radiating Kerr-Newman-de Sitter black holes, inflation and cosmic censorship

Details Timelike limit surfaces, apparent horizons and event horizons of radiating Kerr-Newman-de Sitter black holes, inflation and cosmic censorship Timelike limit surfaces, apparent horizons and event horizons of radiating Kerr-Newman-de Sitter black holes, inflation and cosmic censorship

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cqgra..16..343x&link_type=abstract

Classical and Quantum Gravity, Volume 16, Issue 2, pp. 343-350 (1999).

Mathematics

Logic

6

Scientific paper

Coupling between angular momentum and the cosmological constant does not
produce distortion or deformation of apparent horizons. Only to a
first-order perturbation or approximation can it affect the shape of
event horizons.

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