Le Chatelier-Braun principle in cosmological physics

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dc.creatorPavon, Diego
dc.creatorWang, Bin
dc.date2007-12-04
dc.date2008-04-25
dc.date.accessioned2026-07-07T12:29:54Z
dc.date.available2026-07-07T12:29:54Z
dc.descriptionAssuming that dark energy may be treated as a fluid with a well defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around.
dc.description6 pages, revtex file, no figures; version accepted for publication in General Relativity and Gravitation
dc.identifierhttps://arxiv.org/abs/0712.0565
dc.identifierhttp://arxiv.org/abs/0712.0565
dc.identifierGen.Rel.Grav.41:1-5,2009
dc.identifierdoi:10.1007/s10714-008-0656-y
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215987
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleLe Chatelier-Braun principle in cosmological physics
dc.typetext

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