Classical and quantum evolution of non-isentropic hot singular layers in finite-temperature general relativity

Details Classical and quantum evolution of non-isentropic hot singular layers in finite-temperature general relativity Classical and quantum evolution of non-isentropic hot singular layers in finite-temperature general relativity

1999-11-03

arxiv.org/abs/gr-qc/9911007v1

Gen.Rel.Grav. 31 (1999) 571-577

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

final version, published in GRG as a letter

Scientific paper

The spherically symmetric layer of matter is considered within the frameworks
of general relativity. We perform generalization of the already known theory
for the case of nonconstant surface entropy and finite temperature. We also
propose the minisuperspace model to determine the behaviour of temperature
field and perform the Wheeler-DeWitt quantization.

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