arXiv · gr-qc/0409118
Thermodynamics of a collapsing shell in an expanding Universe
Abstract
We describe the quasi-static collapse of a radiating, spherical shell of matter in de Sitter space-time using a thermodynamical formalism. It is found that the specific heat at constant area and other thermodynamical quantities exhibit singularities related to phase transitions during the collapse.
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G. L. Alberghi, R. Casadio, G. Venturi. 2004-09-30. Thermodynamics of a collapsing shell in an expanding Universe. https://doi.org/10.1016/j.physletb.2004.09.063
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