Measuring neutrino masses with weak lensing

Details Measuring neutrino masses with weak lensing Measuring neutrino masses with weak lensing

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..870..518w&link_type=abstract

INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 9th Conference CIPAN2006. AIP Conference Proceedings, Volume 870, pp. 518-520 (2

Physics

Nuclear Physics

1

Neutrino Mass And Mixing, Gravitational Lenses And Luminous Arcs, Cosmology

Scientific paper

Weak gravitational lensing of distant galaxies by large scale structure (LSS) provides an unbiased way to map the matter distribution in the low redshift universe. This technique, based on the measurement of small distortions in the images of the source galaxies induced by the intervening LSS, is expected to become a key cosmological probe in the future. We discuss how future lensing surveys can probe the sum of the neutrino masses at the 0 05 eV level.

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