Thermodynamics of a collapsing shell in an expanding Universe
classification
🌀 gr-qc
keywords
collapseshellthermodynamicalareacollapsingconstantdescribeduring
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.