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

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

2008-01-12

arxiv.org/abs/0801.1921v2

Int.J.Mod.Phys.D18:501-512,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

13 pages, 2 figures; Modified to improve the visibility of figures

Scientific paper

10.1142/S0218271809014534

The 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 $\Lambda $CDM. The results from both theories are in good agreement and the fits are satisfactory. The correspondence between both approaches is discussed and interpreted.

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