Thin charged shells and the violation of the third law of black hole mechanics

Details Thin charged shells and the violation of the third law of black hole mechanics Thin charged shells and the violation of the third law of black hole mechanics

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983gregr..15..403p&link_type=abstract

General Relativity and Gravitation (ISSN 0001-7701), vol. 15, May 1983, p. 403-415.

Astronomy and Astrophysics

Astronomy

5

Black Holes (Astronomy), Charged Particles, Cosmic Dust, Gravitational Collapse, Spherical Shells, Thin Walled Shells, Astrodynamics, Astronomical Models, Reissner-Nordstrom Solution, Relativity, Singularity (Mathematics), Space-Time Functions

Scientific paper

The collapse of an infinitely thin spherical shell of charged matter, which surrounds a spherically symmetric black hole or has a flat interior, is analyzed in connection with the laws of black hole mechanics and the cosmic censorship hypothesis. An effective potential is introduced to describe the motion of the shell. The process, proposed by Farrugia and Hajicek as a counterexample to the third law, is discussed and generalized to the case of nondust shells.

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