Improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-break galaxies
- Physics Department and Sezione INFN, University of Rome 'La Sapienza', Ple Aldo Moro 2, 00185 Rome (Italy)
- Center for Cosmology, Department of Physics and Astronomy, University of California Irvine, Irvine, California 92697 (United States)
We use measurements of luminosity-dependent galaxy bias at several different redshifts, SDSS at z=0.05, DEEP2 at z=1, and LBGs at z=3.8, combined with WMAP 5-year cosmic microwave background anisotropy data and SDSS Red Luminous Galaxy survey three-dimensional clustering power spectrum to put constraints on cosmological parameters. Fitting this combined dataset, we show that the luminosity-dependent bias data that probe the relation between halo bias and halo mass and its redshift evolution are very sensitive to sum of the neutrino masses: in particular, we obtain the upper limit of at the 95% confidence level for a {lambda}CDM+m{sub {nu}} model, with a {sigma}{sub 8} equal to {sigma}{sub 8}=0.759{+-}0.025 (1{sigma}). When we allow the dark energy equation-of-state parameter w to vary, we find w=-1.30{+-}0.19 for a general wCDM+m{sub {nu}} model with the 95% confidence level upper limit on the neutrino masses at . The constraint on the dark energy equation of state further improves to w=-1.125{+-}0.092 when using also ACBAR and supernovae Union data, in addition to above, with a prior on the Hubble constant from the Hubble Space Telescope.
- OSTI ID:
- 21254419
- Journal Information:
- Physical Review. D, Particles Fields, Vol. 78, Issue 8; Other Information: DOI: 10.1103/PhysRevD.78.083535; (c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
Similar Records
NEW NEUTRINO MASS BOUNDS FROM SDSS-III DATA RELEASE 8 PHOTOMETRIC LUMINOUS GALAXIES
Evolution in the HALO Masses of Isolated Galaxies between Z~;1 andZ~;0: From Deep2 to SDSS