Friedmann Thermodynamics and the Geometry of the Universe

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dc.creatorBayin, Selcuk S.
dc.date2008-04-01
dc.date.accessioned2026-07-07T09:29:40Z
dc.date.available2026-07-07T09:29:40Z
dc.descriptionIn a recent article we have introduced Friedmann thermodynamics, where certain geometric parameters in Friedmann models are treated like their thermodynamic counterparts (temperature, entropy, Gibbs potential etc.). This model has the advantage of allowing us to determine the geometry of the universe by thermodynamic stability arguments. In this article we review connections between thermodynamics, geometry and cosmology.
dc.descriptionKey note speech delivered in the International Conference on Efficiency, Costs, Optimization, Simulation and Environmental Impact of Energy Systems, ECOS'95 and ASME
dc.identifierhttps://arxiv.org/abs/0804.0153
dc.identifierhttp://arxiv.org/abs/0804.0153
dc.identifierProceedings of ECOS' 95 and ASME, Y.A. Gogus, Y.A. Ozturk, G. Tsatsaronis (eds.) Vol.1, pg. 3, 1995
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/157872
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFriedmann Thermodynamics and the Geometry of the Universe
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