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 distances of type-I...
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| Udgivet i: | Brazilian Journal of Physics |
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| Principais autores: | , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Sociedade Brasileira de Física
2010
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=46415799001 |
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