Third law of black-hole dynamics - A formulation and proof

Details Third law of black-hole dynamics - A formulation and proof Third law of black-hole dynamics - A formulation and proof

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvl..57..397i&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 57, July 28, 1986, p. 397-399. NSERC-supported research.

Astronomy and Astrophysics

Astronomy

63

Black Holes (Astronomy), Gravitational Collapse, Thermodynamics, Asymptotic Methods, Deposition, Implosions

Scientific paper

It is shown that no continuous process in which the energy tensor of
accreted matter remains bounded and satisfies the weak energy condition
in a neighborhood of the apparent horizon can reduce the surface gravity
of a black hole to zero within a finite advanced time. This gives a
precise expression to the third law of black-hole mechanics.

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