Black-hole thermodynamics for the nonstationary case.

Details Black-hole thermodynamics for the nonstationary case. Black-hole thermodynamics for the nonstationary case.

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimb.105..857k&link_type=abstract

Nuovo Cimento B, Vol. 105, No. 8/9, p. 857 - 865

Computer Science

2

Black Holes: Thermodynamics

Scientific paper

An attempt of nonstationary black-hole thermodynamics is made for the case of the radiation mode of the Vaidya metric. Calculating the modified temperature from the wave equation, entropy is defined by the apparent horizon, as the local quantity whose state is a proper fiducial equilibrium state. In these thermodynamic quantities the authors try to see what role the mass-varying effects play of. So it is a kind of quasi-equilibrium thermodynamic theory on the two points of view for mass-varying processes, rather than a complete nonequilibrium thermodynamics.

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