Event horizon area in a slowly changing Weyl geometry

Details Event horizon area in a slowly changing Weyl geometry Event horizon area in a slowly changing Weyl geometry

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982cajph..60.1155b&link_type=abstract

Canadian Journal of Physics, vol. 60, Aug. 1982, p. 1155-1162. Research supported by the University of Utah

Astronomy and Astrophysics

Astronomy

Astronomical Models, Black Holes (Astronomy), Dynamic Response, Relativity, Stellar Evolution, Approximation, Constraints, Singularity (Mathematics), Steady State

Scientific paper

The paper considers a class of models of dynamically distorted black hole event horizons based on a slow evolution of black hole Weyl geometries. With the time scale for the evolution taken arbitrarily large, a fairly simple mathematical description of the 'quasistatic' geometry results. With this description, it is shown how the constraint on event horizon area is related to the absence of singularities at the horizon. The evolution of intrinsic event horizon geometry is plotted for a specific example.

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