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The cold dark matter model with cosmological constant and the flatness constraint

The Hubble parameter, a function of the cosmological redshift, is derived from the Friedmann-Robertson-Walker equation. The three physical parameters H0, Ω0m and ΩΛ are determined fitting the Hubble parameter to the data from measurements of redshift and luminosity distanc...

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Bibliografski detalji
Izdano u:Brazilian Journal of Physics
Glavni autori: A.C.B. Antunes, L.J. Antunes
Format: Artigo
Jezik:Inglês
Izdano: Sociedade Brasileira de Física 2010
Teme:
Online pristup:https://www.redalyc.org/articulo.oa?id=46415799001
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