Redshift spherical shell energy in isotropic Universes

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dc.creatorRomano, Antonio Enea
dc.date2007-02-08
dc.date2007-10-09
dc.date.accessioned2026-07-07T11:56:22Z
dc.date.available2026-07-07T11:56:22Z
dc.descriptionWe introduce the redshift spherical shell energy (RSSE), which can be used to test in the redshift space the radial inhomogeneity of an isotropic universe, providing additional constraints for LTB models, and a more general test of cosmic homogeneity.
dc.description11 pages, 2 figures, Accepted by Physical Review D15
dc.identifierhttps://arxiv.org/abs/astro-ph/0702229
dc.identifierhttp://arxiv.org/abs/astro-ph/0702229
dc.identifierPhys.Rev.D76:103525,2007
dc.identifierdoi:10.1103/PhysRevD.76.103525
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205558
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleRedshift spherical shell energy in isotropic Universes
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