Curvaton reheating in tachyonic braneworld inflation

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dc.contributor.authorCampuzano, C.
dc.contributor.authorDel Campo, S.
dc.contributor.authorHerrera, R.
dc.date.accessioned2023-03-21T19:33:08Z
dc.date.available2023-03-21T19:33:08Z
dc.date.issued2005-10
dc.descriptionIndexación: Scopus.
dc.description.abstractThe curvaton reheating in a tachyonic braneworld inflationary universe model with an exponential potential is studied. We have found that the energy density in the kinetic epoch, has a complicated dependencies of the scale factor. For different scenarios the temperature of reheating is computed, finding an upper limit that lies in the range 1014-1016 GeV.es
dc.description.urihttps://journals-aps-org.recursosbiblioteca.unab.cl/prd/abstract/10.1103/PhysRevD.72.083515
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, Volume 72, Issue 815, October 2005, Article number 083515es
dc.identifier.doi10.1103/PhysRevD.72.083515
dc.identifier.issn1550-2368
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/47732
dc.language.isoenes
dc.publisherAmerican Physical Societyes
dc.rights.licenseAttribution 4.0 International (CC BY 4.0)
dc.rights.urihttps://journals-aps-org.recursosbiblioteca.unab.cl/prd/about
dc.subjectcurvaton reheatinges
dc.subjecttachyonices
dc.subjectbraneworld inflationary universe modeles
dc.titleCurvaton reheating in tachyonic braneworld inflationes
dc.typeArtículoes
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