QSSC re-examined for the newly discovered SNe Ia

Details QSSC re-examined for the newly discovered SNe Ia QSSC re-examined for the newly discovered SNe Ia

2004-12-02

arxiv.org/abs/astro-ph/0412048v1

Int.J.Mod.Phys.D14:345-354,2005

Astronomy and Astrophysics

Astrophysics

13 pages including 2 figures; accepted in Int. J. Mod. Phys. D

Scientific paper

10.1142/S0218271805006547

We examine the possible consistency of the quasi-steady state model with the newly discovered SNe Ia. The model assumes the existence of metallic dust ejected from the SNe explosions, which extinguishes light travelling over long distances. We find that the model shows a reasonable fit to the data, which improves if one takes account of the weak gravitational lensing effect of the SNe which have been observed on the brighter side.

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