Physics – High Energy Physics
Scientific paper
Aug 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1040...32s&link_type=abstract
KEK COSMOPHYSICS GROUP INAUGURAL CONFERENCE ``ACCELERATORS IN THE UNIVERSE'': Interplay between High Energy Physics and Cosmophy
Physics
High Energy Physics
Background Radiations, Dark Matter, Dark Energy, Neutrino Mass And Mixing, Quantum Cosmology, Spectroscopy And Spectrophotometry, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Star Formation
Scientific paper
We present the first attempt to analytically study the nonlinear matter power spectrum for a mixed dark matter model containing neutrinos of total mass ~0.1 eV, based on cosmological perturbation theory. The suppression in the power spectrum amplitudes due to massive neutrinos is enhanced in the weakly nonlinear regime. We demonstrate that, thanks to this enhanced effect, the use of such a nonlinear model may enable a precision of σ(mν,tot)~0.07 eV in constraining the total neutrino mass for the planned galaxy redshift survey, a factor of two improvement compared to the linear regime.
Saito Shun
Takada Masahiro
Taruya Atsushi
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