Thin shells and the surface gravity of black holes

Details Thin shells and the surface gravity of black holes Thin shells and the surface gravity of black holes

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nciml..30..186l&link_type=abstract

Nuovo Cimento, Lettere, Serie 2, vol. 30, Feb. 7, 1981, p. 186-188. Research supported by Queen's University, and Natural Scien

Astronomy and Astrophysics

Astronomy

1

Black Holes (Astronomy), Spherical Shells, Stellar Gravitation, Surface Properties, Thin Walled Shells, Ideal Fluids, Ideal Gas, Manifolds, Red Shift, Reissner Theory, Schwarzschild Metric, Tachyons, Vectors (Mathematics)

Scientific paper

A Killing congruence which, when reduced to the horizon of a black hole, generates the surface gravity of the horizon is used to generate a thin shell, and it is shown that the surface gravity can also be interpreted as the redshifted trace of the surface pressure of the shell. It is pointed out that as the time-like hypersurface dividing spacetime into two-distinct four-dimensional manifolds which represents the history of a thin shell is forced onto the absolute event horizon of one of the four-dimensional manifolds, the particle distribution on the hypersurface must become tachyonic.

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