2008
DOI: 10.1088/1742-6596/120/5/052055
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MOON for a next-generation neutrino-less double-beta decay experiment; present status and perspective

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Cited by 8 publications
(2 citation statements)
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“…Furthermore, the 100 Mo nucleus is a famous double-beta-decay emitter [31,32] and has been employed by various experiments, e.g. the NEMO Observatory [33], the MOON experiment [34], etc. Thus, nuclear-structure calculations in the Mo region are welcome for other processes and experiments too.…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, the 100 Mo nucleus is a famous double-beta-decay emitter [31,32] and has been employed by various experiments, e.g. the NEMO Observatory [33], the MOON experiment [34], etc. Thus, nuclear-structure calculations in the Mo region are welcome for other processes and experiments too.…”
Section: Introductionmentioning
confidence: 99%
“…Several experiments are focusing on different isotopes via utilizing various detector techniques such as GERDA (GERmanium Detector Array) [4], MAJORANA (Majorana Demonstrator) [5] and CDEX (China Dark matter EXperiment) with 76 Ge enrich high purity Ge detectors [6]; EXO (Enriched Xenon Observatory) [7] and KamLandZen (Kamioka Liquid Scintillator Antineutrino Detector) with liquid 136 Xe time projection chambers [8]; and CUORE (Cryogenic Underground Observatory for Rare Events) with 130 Te bolometric detectors [9]. The next-generation experiments with tonne scale detectors such as LEGEND ( 76 Ge) (MAJORANA + GERDA) [10,11], nEXO ( 136 Xe) [12], NEXT ( 136 Xe) [13], CUPID ( 130 Te) [14], SuperNEMO ( 82 Se, 150 Nd) [15], AMoRE ( 100 Mo) [16], COBRA ( 116 Cd) [17], CANDLES-III ( 48 Ca) [18], SNO + ( 130 Te) [19], TIN.TIN ( 124 Sn) [20], MOON ( 100 Mo) [21] and LUMINEU ( 100 Mo) [22] have been proposed. Some of them will start data taking over the next few years and others are under construction phase.…”
Section: Introductionmentioning
confidence: 99%