dc.creatorAmarilla, Leonardo
dc.creatorVucetich, Héctor
dc.date2010-07
dc.date2020-07-02T12:55:02Z
dc.date.accessioned2023-07-14T20:39:25Z
dc.date.available2023-07-14T20:39:25Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/99733
dc.identifierhttps://ri.conicet.gov.ar/11336/16544
dc.identifierissn:0217-751X
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7440090
dc.descriptionWe consider a brane-world cosmological model coupled to a bulk scalar field. Since the brane tension turns out to be proportional to Newton’s coupling G, in such a model a time variation of G naturally occurs. By resorting to available bounds on the variation of G, the parameters of the model are constrained. The constraints coming from nucleosynthesis and CMB result to be the severest ones.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectBrane-world
dc.subjectCosmology
dc.subjectVarying
dc.subjectConstants
dc.titleBrane-world cosmology and varying G
dc.typeArticulo
dc.typePreprint


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