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Authordc.contributor.authorMarra, Valerio 
Authordc.contributor.authorSapone, Domenico 
Admission datedc.date.accessioned2018-07-24T13:44:41Z
Available datedc.date.available2018-07-24T13:44:41Z
Publication datedc.date.issued2018
Cita de ítemdc.identifier.citationPhysical Review D 97, 083510 (2018)es_ES
Identifierdc.identifier.other10.1103/PhysRevD.97.083510
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/150188
Abstractdc.description.abstractWe test both the Friedmann-Lemaitre-Robertson-Walker geometry and ACDM cosmology in a model-independent way by reconstructing the Hubble function H(z), the comoving distance D(z), and the growth of structure f sigma(8)(z) using the most recent data available. We use the linear model formalism in order to optimally reconstruct the above cosmological functions, together with their derivatives and integrals. We then evaluate four of the null tests available in the literature that probe both background and perturbation assumptions. For all the four tests, we find agreement, within the errors, with the standard cosmological model.es_ES
Patrocinadordc.description.sponsorshipCNPq FAPES Fondecyt 11140496es_ES
Lenguagedc.language.isoenes_ES
Publisherdc.publisherAmerican Physical Societyes_ES
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Sourcedc.sourcePhysical Review Des_ES
Títulodc.titleNull tests of the standard model using the linear model formalismes_ES
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadortjnes_ES
Indexationuchile.indexArtículo de publicación ISIes_ES


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Attribution-NonCommercial-NoDerivs 3.0 Chile
Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile