Abstract
We investigate the way the total mass sum of neutrinos can be constrained from the neutrinoless double beta-decay and cosmological probes with cosmic microwave background (CMBR), large-scale structures including 2dFGRS and SDSS datasets. First we discuss, in brief, the current status of neutrino mass bounds from neutrino beta decays and cosmic constraint within the flat ΛCMD model. In addition, we explore the interacting neutrino dark-energy model, where the evolution of neutrino masses is determined by quintessence scalar field, which is responsible for cosmic acceleration. Assuming the flatness of the Universe, the constraint we can derive from the current observation is \(\sum m_{\nu } < 0.87\) eV at 95% confidence level, which is consistent with \(\sum m_{\nu } < 0.68\) eV in the flat ΛCDM model without Lyman alpha forest data. In the presence of Lyman- α forest data, interacting dark-energy models prefer a weaker bound \(\sum m_{\nu } < 0.43\) eV to \(\sum m_{\nu } < 0.17\) eV (Seljark et al). Finally, we discuss the future prospect of the neutrino mass bound with weak-lensing effects.
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Acknowledgements
YYK is grateful to the organizers of UNICOS 2014 for the opportunity to present this work and for the warm hospitality. YYK would like to thank LAPTh at Annecy in France for the warm hospitality he has received during his visit there. His work is partially supported by the Research Professorship (A) of Ewha Womans University during 2010–2011, and by the Basic Science Research Programme through the National Research Foundation of Korea (NRF) funded by the Korean Ministry of Education, Science and Technology (Grant Nos 0409-20130121; 0409-20140077) and International Cooperation Research Programme funded by the Korean Ministry of Science, ICT and Future Planning (Grant No. 0409-20130159).
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KEUM, YY. Neutrino mass bounds from neutrinoless double beta-decays and cosmological probes. Pramana - J Phys 86, 437–451 (2016). https://doi.org/10.1007/s12043-015-1164-8
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DOI: https://doi.org/10.1007/s12043-015-1164-8
Keywords
- Neutrino masses
- neutrinoless double beta decay
- large-scale structures
- interacting neutrino dark-energy model