Interacting dark matter and cosmic acceleration

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dc.contributor.authorCardenas, Victor H.
dc.contributor.authorLepe, Samuel
dc.date.accessioned2021-08-26T17:49:11Z
dc.date.available2021-08-26T17:49:11Z
dc.date.issued2020
dc.description.abstractWe study the effect of an explicit interaction between two scalar fields components describing dark matter in the context of a recent proposal framework for interaction. We find that, even assuming a very small coupling, it is sufficient to explain the observational effects of a cosmological constant, and also overcome the problems of the Λ CDM model without assuming an exotic dark energy.en_ES
dc.identifier.doihttps://doi.org/10.1140/epjc/s10052-020-08443-4
dc.identifier.urihttp://repositoriobibliotecas.uv.cl/handle/uvscl/2276
dc.language.isoenen_ES
dc.publisherEDP Sciencesen_ES
dc.publisherSocietà Italiana di Fisicaen_ES
dc.publisherSpringer Berlin Heidelbergen_ES
dc.sourceThe European Physical Journal Cen_ES
dc.subjectDARK ENERGYen_ES
dc.subjectDARK MATTERen_ES
dc.subjectCOSMOLOGYen_ES
dc.titleInteracting dark matter and cosmic accelerationen_ES
dc.typeArticuloen_ES
uv.catalogadorRCR DIBRAen_ES

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