MOON for neutrino-less double beta decays. Majorana neutrinos by spectroscopic studies of double beta decays

Details MOON for neutrino-less double beta decays. Majorana neutrinos by spectroscopic studies of double beta decays MOON for neutrino-less double beta decays. Majorana neutrinos by spectroscopic studies of double beta decays

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008epjst.162..239e&link_type=abstract

The European Physical Journal Special Topics, Volume 162, Issue 1, pp.239-250

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6

Scientific paper

The MOON (Majorana/Mo Observatory Of Neutrinos) project aims at studies of the Majorana nature of the neutrino ( ν) and the ν-mass spectrum by spectroscopic experiments of neutrino-less double beta decays (0 νββ) with the ν-mass sensitivity of < m {/ν m }> = 100-30 meV. The solid scintillator option of the MOON detector is a super ensemble of multi-layer modules, each being composed by PL scintillator plates and position-sensitive detector planes with good overall energy resolution of σ ≈ 2% at the Q ββ ≈ 3 MeV. Thin ββ source films are interleaved between the detector planes. High localization of the two β tracks enables one to select true signals and reject BG ones. The multi-layer structure of the detector makes it realistic to build a compact ton-scale detector. MOON with detector ≠ ββ source is used for studying 0 νββ decays from 100Mo, 82Se and other ββ isotopes with large Q ββ . Real-time exclusive measurements of low energy solar neutrinos can be made by observing inverse β rays from solar- ν captures of 100Mo in delayed coincidence with the subsequent β decay of 100Tc.

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