ΛCDM type Heckmann–Schuking model and Union 2.1 compilation


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We study a ΛCDM type cosmological model in Heckmann-Schucking space-time, by using 287 high redshift (.3 ≤ z ≤ 1.4) SN Ia data on observed absolute magnitude along with their possible error from Union 2.1 compilation. We use the χ2 test to compare Union 2.1 compilation observed data and the corresponding theoretical values of the apparent magnitude (m). It is found that the best fit value of (Ωm)0, (ΩΛ)0 and (Ωσ)0 are 0.2940, 0.7058 and 0.0002, respectively, and the derived model represents the features of an accelerating universe which is consistent with the recent astrophysical observations.

Sobre autores

G. Goswami

Department of Mathematics

Autor responsável pela correspondência
Email: gk_goswami@yahoo.co.in
Índia, Bhilai, 490006

R. Dewangan

Department of Mathematics

Email: abanilyadav@yahoo.co.in
Índia, Bhilai, 490006

Anil Yadav

Department of Physics

Autor responsável pela correspondência
Email: abanilyadav@yahoo.co.in
Índia, Greater Noida, 201306

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