Using the cluster mass function from weak lensing to constrain neutrino masses - INSPIRE

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Using the cluster mass function from weak lensing to constrain neutrino masses

Nov, 2006

7 pages

Published in:

Phys.Rev.D 75 (2007) 083510

e-Print:

astro-ph/0611761 [astro-ph]

DOI:

10.1103/PhysRevD.75.083510

PDG: SUM OF THE NEUTRINO MASSES,

{\mathit m}_{\mathrm {tot}}

View in:

ADS Abstract Service

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Abstract: (arXiv)

We discuss the variation of cosmological upper bounds on

M_\nu

, the sum of the neutrino masses, with the choice of data sets included in the analysis, pointing out a few oddities not easily seen when all data sets are combined. For example, the effect of applying different priors varies significantly depending on whether we use the power spectrum from the 2dFGRS or SDSS galaxy survey. A conservative neutrino mass limit of

M_\nu < 1.43

eV (95%C.L.) is obtained by combining the WMAP 3 year data with the cluster mass function measured by weak gravitational lensing. This limit has the virtue of not making any assumptions about the bias of luminous matter with respect to the dark matter, and is in this sense (and this sense only) bias-free.

14.60.Pq
95.35.+d
neutrino: mass
upper limit
gravitation: lens
dark matter
cosmic background radiation
galaxy: cluster
supernova
baryon: oscillation

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