Supernova limits on brane world cosmology

dc.creatorFairbairn, Malcolm
dc.creatorGoobar, Ariel
dc.date2005-11-01
dc.date2006-01-22
dc.date.accessioned2026-07-07T10:43:23Z
dc.date.available2026-07-07T10:43:23Z
dc.descriptionBy combining the first year data from the Supernova Legacy Survey (SN LS) and the recent detection of the baryon acoustic peak in the Sloan Digital Sky Survey data, we are able to place strong constraints on models where the cosmic acceleration is due to the leakage of gravity from the brane into the bulk on large scales. In particular, we are able to show that the DGP model is not compatible with a spatially flat universe. We generalize our analysis to phenomenological toy models where the curvature of the brane enters into the Friedmann equations in different ways.
dc.descriptioncomments added on baryon oscillations/typos fixed 8 pages, 3 figs
dc.identifierhttps://arxiv.org/abs/astro-ph/0511029
dc.identifierhttp://arxiv.org/abs/astro-ph/0511029
dc.identifierPhys.Lett.B642:432-435,2006
dc.identifierdoi:10.1016/j.physletb.2006.07.048
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182222
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleSupernova limits on brane world cosmology
dc.typetext

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