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ΛCDM type Heckmann–Schuking model and Union 2.1 compilation

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Abstract

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 (Ω m )0, (ΩΛ)0 and (Ω σ )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.

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Authors and Affiliations

  1. Department of Mathematics, Kalyan P. G. College, Bhilai, 490006, India

    G. K. Goswami & R. N. Dewangan

  2. Department of Physics, United College of Engineering & Research, Greater Noida, 201306, India

    Anil Kumar Yadav

Authors
  1. G. K. Goswami
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  2. R. N. Dewangan
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  3. Anil Kumar Yadav
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Corresponding authors

Correspondence to G. K. Goswami or Anil Kumar Yadav.

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Goswami, G.K., Dewangan, R.N. & Yadav, A.K. ΛCDM type Heckmann–Schuking model and Union 2.1 compilation. Gravit. Cosmol. 22, 388–393 (2016). https://doi.org/10.1134/S0202289316040083

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  • DOI: https://doi.org/10.1134/S0202289316040083

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