We study tilted cold dark matter (CDM) models, that is OMEGA0 = 1 models with a primordial spectral index n less than or similar to 1. We test these models against three experiments on the cosmic microwave background anisotropy at 7', 3-degrees, and 6-degrees, and against measurements of galaxy peculiar velocities on large scales. These observations together suggest that the whole class of tilted CDM models with n less-than-or-equal-to 1 can be ruled out, for any value of the biasing parameter b.

Muciaccia, P., Mei, S., DE GASPERIS, G., Vittorio, N. (1993). Tilted cold dark matter models confront the cosmic microwave background and the galaxy peculiar velocity field. THE ASTROPHYSICAL JOURNAL, 410(2), L61-L64 [10.1086/186880].

Tilted cold dark matter models confront the cosmic microwave background and the galaxy peculiar velocity field

DE GASPERIS, GIANCARLO;VITTORIO, NICOLA
1993-01-01

Abstract

We study tilted cold dark matter (CDM) models, that is OMEGA0 = 1 models with a primordial spectral index n less than or similar to 1. We test these models against three experiments on the cosmic microwave background anisotropy at 7', 3-degrees, and 6-degrees, and against measurements of galaxy peculiar velocities on large scales. These observations together suggest that the whole class of tilted CDM models with n less-than-or-equal-to 1 can be ruled out, for any value of the biasing parameter b.
1993
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Con Impact Factor ISI
COSMIC MICROWAVE BACKGROUND; DARK MATTER; GALAXIES, FORMATION
Muciaccia, P., Mei, S., DE GASPERIS, G., Vittorio, N. (1993). Tilted cold dark matter models confront the cosmic microwave background and the galaxy peculiar velocity field. THE ASTROPHYSICAL JOURNAL, 410(2), L61-L64 [10.1086/186880].
Muciaccia, P; Mei, S; DE GASPERIS, G; Vittorio, N
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/45006
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