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dc.contributor.authorLukes-Gerakopoulos, Gen_US
dc.contributor.authorAcquaviva, Gen_US
dc.contributor.authorMarkakis, Cen_US
dc.date.accessioned2019-09-19T09:40:34Z
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/59741
dc.description10 pages, 1 figure, to appear in the RAGtime20 conference proceedings (Opava, October 15-19 2018)en_US
dc.description10 pages, 1 figure, to appear in the RAGtime20 conference proceedings (Opava, October 15-19 2018)en_US
dc.description.abstractWe demonstrate that the thermodynamics of a perfect fluid describing baryonic matter can, in certain limits, lead to an equation of state similar to that of dark energy. We keep the cosmic fluid equation of state quite general by just demanding that the speed of sound is positive and less than the speed of light. In this framework, we discuss some propositions by looking at the asymptotic behavior of the cosmic fluid.en_US
dc.subjectgr-qcen_US
dc.subjectgr-qcen_US
dc.titleProbing Dark Energy through Perfect Fluid Thermodynamicsen_US
dc.typeConference Proceeding
dc.rights.holder© The Author(s) 2019
pubs.author-urlhttp://arxiv.org/abs/1902.11051v1en_US
pubs.notesNot knownen_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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