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Cosmological parameters from large scale structure observations

Novosyadlyj, B.
Gottloeber, S.
Lukash, V. N.
Apunevych, S.
Published in Astronomy & astrophysics. 2000, vol. 356, no. 2, p. 418-434
Abstract The possibility of determining cosmological parameters on the basis of a wide set of observational data including the Abell-ACO cluster power spectrum and mass function, peculiar velocities of galaxies, the distribution of Ly-[FORMULA] clouds and CMB temperature fluctuations is analyzed. Using a [FORMULA] minimization method, assuming [FORMULA] and no contribution from gravity waves, we show that this data set determines quite precisely the values of the spectral index n of the primordial power spectrum, baryon, cold dark matter and massive neutrino density [FORMULA], [FORMULA] and [FORMULA] respectively, the Hubble constant [FORMULA]km/s/Mpc) and the value of the cosmological constant, [FORMULA].
Keywords Galaxies: clusters: generalCosmology: theoryCosmology: dark matterCosmology: large-scale structure of Universe
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NOVOSYADLYJ, B. et al. Cosmological parameters from large scale structure observations. In: Astronomy & astrophysics, 2000, vol. 356, n° 2, p. 418-434. https://archive-ouverte.unige.ch/unige:1021

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Deposited on : 2009-02-26

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