Large-scale galaxy correlations as a test for dark energy

Large-scale galaxy correlations as a test for dark energy

We have shown earlier that, contrary to popular belief, Einstein--de Sitter (E--deS) models can still fit the {\sl WMAP} data on the cosmic microwave background provided one adopts a low Hubble constant and relaxes the usual assumption that the primordial density perturbation is scale-free. The rece...

Bibliográfalaš dieđut
Váldodahkkit:	Blanchard, A, Douspis, M, Rowan-Robinson, M, Sarkar, S
Materiálatiipa:	Journal article
Giella:	English
Almmustuhtton:	2005

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