| Autor: |
Elgarøy Ø; Institute of Astronomy, University of Cambridge, Madingley Road, United Kingdom., Lahav O, Percival WJ, Peacock JA, Madgwick DS, Bridle SL, Baugh CM, Baldry IK, Bland-Hawthorn J, Bridges T, Cannon R, Cole S, Colless M, Collins C, Couch W, Dalton G, De Propris R, Driver SP, Efstathiou GP, Ellis RS, Frenk CS, Glazebrook K, Jackson C, Lewis I, Lumsden S, Maddox S, Norberg P, Peterson BA, Sutherland W, Taylor K |
| Jazyk: |
angličtina |
| Zdroj: |
Physical review letters [Phys Rev Lett] 2002 Aug 05; Vol. 89 (6), pp. 061301. Date of Electronic Publication: 2002 Jul 19. |
| DOI: |
10.1103/PhysRevLett.89.061301 |
| Abstrakt: |
We constrain f(nu) identical with Omega(nu)/Omega(m), the fractional contribution of neutrinos to the total mass density in the Universe, by comparing the power spectrum of fluctuations derived from the 2 Degree Field Galaxy Redshift Survey with power spectra for models with four components: baryons, cold dark matter, massive neutrinos, and a cosmological constant. Adding constraints from independent cosmological probes we find f(nu)<0.13 (at 95% confidence) for a prior of 0.1
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| Databáze: |
MEDLINE |
| Externí odkaz: |
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