Dark Energy and Neutrino Mass Limits from Baryogenesis

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dc.creatorGu, Peihong
dc.creatorWang, Xiulian
dc.creatorZhang, Xinmin
dc.date2003-07-10
dc.date2003-08-03
dc.date.accessioned2026-07-07T10:28:53Z
dc.date.available2026-07-07T10:28:53Z
dc.descriptionIn this brief report we consider couplings of the dark energy scalar, such as Quintessence to the neutrinos and discuss its implications in studies on the neutrino mass limits from Baryogenesis. During the evolution of the dark energy scalar, the neutrino masses vary, consequently the bounds on the neutrino masses we have here differ from those obtained before.
dc.description5 pages,3 figures. Version accepted for publication in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/hep-ph/0307148
dc.identifierhttp://arxiv.org/abs/hep-ph/0307148
dc.identifierPhys.Rev.D68:087301,2003
dc.identifierdoi:10.1103/PhysRevD.68.087301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177608
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleDark Energy and Neutrino Mass Limits from Baryogenesis
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