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Authordc.contributor.authorAsenjo, Felipe A. 
Authordc.contributor.authorHojman Guiñerman, Sergio 
Admission datedc.date.accessioned2018-06-21T16:24:01Z
Available datedc.date.available2018-06-21T16:24:01Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationPhysical Review D 96, 044021 (2017)es_ES
Identifierdc.identifier.other10.1103/PhysRevD.96.044021
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/149122
Abstractdc.description.abstractExact electromagnetic wave solutions to Maxwell equations on anisotropic Bianchi I cosmological spacetime backgrounds are studied. The waves evolving on Bianchi I spacetimes exhibit birefringence (associated with linear polarization) and dispersion. The particular case of a vacuum-dominated anisotropic Universe, which reproduces a Friedmann-Robertson-Walker Universe (for late times)-while, for earlier times, it matches a Kasner Universe-is studied. The electromagnetic waves do not, in general, follow null geodesics. This produces a modification of the cosmological redshift, which is then dependent on light polarization, its dispersion, and its non-null geodesic behavior. New results presented here may help to tackle some issues related to the "horizon" problem.es_ES
Patrocinadordc.description.sponsorshipCONICyT-Chile 79130002es_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.titleBirefringent light propagation on anisotropic cosmological backgroundses_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