Alessandro Pesci 2007 Class. Quantum Grav. 24 6219 doi:10.1088/0264-9381/24/24/005
Alessandro Pesci
Show affiliationsIn a classical spacetime satisfying Einstein's equation and the null convergence condition, the same quantum mechanical effects that cause black holes to have a temperature are found to imply, if joined to the macroscopic nature of entropy, the covariant entropy bound in its generalized form. This is obtained from thermodynamics, as applied across the local Rindler causal horizon through every point p of the null hypersurfaces L the covariant entropy bound refers to, in the direction of the null geodesics generating L.
04.20.Gz Spacetime topology, causal structure, spinor structure
04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics
83C75 Space-time singularities, cosmic censorship, etc.
83C05 Einstein's equations (general structure, canonical formalism, Cauchy problems)
Issue 24 (21 December 2007)
Received 29 August 2007, in final form 29 October 2007
Published 27 November 2007
Alessandro Pesci 2007 Class. Quantum Grav. 24 6219
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