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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...
Tallennettuna:
| Julkaisussa: | Brazilian Journal of Physics |
|---|---|
| Päätekijät: | , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Sociedade Brasileira de Física
2010
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| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=46415799001 |
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