Equation of State for a van der Waals Universe during Reissner-Nordstrom Expansion

Simple item page
dc.creatorProdanov, Emil M.
dc.creatorIvanov, Rossen I.
dc.creatorGueorguiev, V. G.
dc.date2008-05-31
dc.date.accessioned2026-07-07T11:33:52Z
dc.date.available2026-07-07T11:33:52Z
dc.descriptionIn a previous work [E.M. Prodanov, R.I. Ivanov, and V.G. Gueorguiev, Reissner-Nordstrom Expansion, Astroparticle Physics 27 (150-154) 2007], we proposed a classical model for the expansion of the Universe during the radiation-dominated epoch based on the gravitational repulsion of the Reissner-Nordstrom geometry - naked singularity description of particles that "grow" with the drop of the temperature. In this work we model the Universe during the Reissner-Nordstrom expansion as a van der Waals gas and determine the equation of state.
dc.description13 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/0806.0076
dc.identifierhttp://arxiv.org/abs/0806.0076
dc.identifierJHEP0806:060,2008
dc.identifierdoi:10.1088/1126-6708/2008/06/060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198047
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEquation of State for a van der Waals Universe during Reissner-Nordstrom Expansion
dc.typetext

Files

Collections

arXiv