Classical and quantum evolution of non-isentropic hot singular layers in finite-temperature general relativity
arXiv:gr-qc/9911007 · doi:10.1023/A:1026602508168
Abstract
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.
final version, published in GRG as a letter