Entropy of Microwave Background Radiation in Observable Universe

dc.creatorPiao, Yun-Song
dc.date2006-06-05
dc.date2006-07-17
dc.date.accessioned2026-07-07T10:40:55Z
dc.date.available2026-07-07T10:40:55Z
dc.descriptionWe show that the cosmological constant at late time places a bound on the entropy of microwave background radiation deposited in the future event horizon of a given observer, $S\leq S_{Λ_0}^{3/4}$. This bound is independent of the energy scale of reheating and the FRW evolution after reheating. We also discuss why the entropy of microwave background in our observable universe has its present value.
dc.description3 pages, no figures, revised version to publish in PRD brief report
dc.identifierhttps://arxiv.org/abs/gr-qc/0606024
dc.identifierhttp://arxiv.org/abs/gr-qc/0606024
dc.identifierPhys.Rev.D74:047301,2006
dc.identifierdoi:10.1103/PhysRevD.74.047301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181474
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleEntropy of Microwave Background Radiation in Observable Universe
dc.typetext

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