Some studies on dark energy related problems

dc.creatorWang, Fei
dc.creatorYang, Jin Min
dc.date2005-04-06
dc.date.accessioned2026-07-07T12:25:01Z
dc.date.available2026-07-07T12:25:01Z
dc.descriptionIn this work we perform some studies related to dark energy. Firstly, we propose a dynamical approach to explain the dark energy content of the universe. We assume that a massless scalar field couples to the Hubble parameter with some Planck-mass suppressed interactions. This scalar field developes a Hubble parameter-dependent (thus time-dependent) vacum expectation value, which renders a time-independent relative density for dark energy and thus can explain the coincidence of the dark energy density of the universe. Secondly, we assume the dark matter particle is meta-stable and decays very lately into the dark energy scalar field. Such a conversion of matter to dark energy can give an explanation for the starting time of the accelerating expansion of the universe. Thirdly, we introduce multiple Affleck-Dine fields to the landscape scenario of dark energy in order to have the required baryon-asymmetry universe.
dc.description9 pages, 1 fig
dc.identifierhttps://arxiv.org/abs/hep-ph/0504046
dc.identifierhttp://arxiv.org/abs/hep-ph/0504046
dc.identifierEur.Phys.J.C45:815-818,2006
dc.identifierdoi:10.1140/epjc/s2005-02457-8
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/214500
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleSome studies on dark energy related problems
dc.typetext

Files

Collections