Fitting the luminosity data from type Ia supernovae in the frame of the Cosmic Defect theory

Simple item page
dc.creatorTartaglia, A.
dc.creatorCapone, M.
dc.creatorCardone, V.
dc.creatorRadicella, N.
dc.date2008-01-12
dc.date2008-01-16
dc.date.accessioned2026-07-07T13:13:16Z
dc.date.available2026-07-07T13:13:16Z
dc.descriptionThe Cosmic Defect (CD) theory is reviewed and used to fit the data for the accelerated expansion of the universe, obtained from the apparent luminosity of 192 SnIa's. The fit from CD is compared with the one obtained by means of $Λ$CDM. The results from both theories are in good agreement and the fits are satisfactory. The correspondence between both approaches is discussed and interpreted.
dc.description13 pages, 2 figures; Modified to improve the visibility of figures
dc.identifierhttps://arxiv.org/abs/0801.1921
dc.identifierhttp://arxiv.org/abs/0801.1921
dc.identifierInt.J.Mod.Phys.D18:501-512,2009
dc.identifierdoi:10.1142/S0218271809014534
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229832
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleFitting the luminosity data from type Ia supernovae in the frame of the Cosmic Defect theory
dc.typetext

Files

Collections

arXiv