Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2008-03-17
AIP Conf.Proc.1016:343-349,2008
Physics
High Energy Physics
High Energy Physics - Phenomenology
Latex 12 pages, 3 figures, correct typos and add new references
Scientific paper
10.1063/1.2943596
We investigate the way how the total mass sum of neutrinos can be constrained from the neutrinoless double beta decay and cosmological probes with cosmic microwave background (WMAP 3-year results), large scale structures including 2dFGRS and SDSS data sets. First we discuss, in brief, on the current status of neutrino mass bounds from neutrino beta decays and cosmic constrain within the flat $\Lambda CMD$ model. In addition, we explore the interacting neutrino dark-energy model, where the evolution of neutrino masses is determined by quintessence scalar filed, which is responsable for cosmic acceleration today. Assuming the flatness of the universe, the constraint we can derive from the current observation is $\sum m_{\nu} < 0.87$eV at the 95 % confidence level, which is consistent with $\sum m_{\nu} < 0.68$eV in the flat $\Lambda CDM$ model. Finally we discuss the future prospect of the neutrino mass bound with weak-lensing effects.
Ichiki Kiyotomo
Kajino Taka
Keum Yong-Yeon
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