Weighing Neutrinos with Galaxy Surveys
W. Hu, D.J. Eisenstein, M. Tegmark
Abstract
We show that galaxy redshift
surveys provide an extraordinarily sensitive probe of the neutrino
mass, with eV mass neutrinos suppressing the power spectrum by a factor of two.
The upcoming Sloan Digital Sky Survey should detect N nearly degenerate massive
neutrino species with mass m_\nu > 0.65 (\Omega_m h^2/0.1 N)^{0.8} eV
at better than 2\sigma once cosmic microwave background experiments, which are
themselves insensitive to m_\nu, measure two other cosmological parameters.
There is significant overlap between this region and that implied by the
LSND experiment, and even m_\nu ~ 0.1 eV, as implied by the
atmospheric neutrino anomaly, can affect cosmological measurements.
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Publication Info
IASSNS-AST-97/XX
Phys. Rev. Lett. 80 5255 (1998)
whu@ias.edu