2014
DOI: 10.1038/nature13432
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Search for Majorana neutrinos with the first two years of EXO-200 data

Abstract: Many extensions of the Standard Model of particle physics suggest that neutrinos should be Majorana-type fermions, but this assumption is difficult to confirm. Observation of neutrinoless double-beta decay (0νββ), a spontaneous transition that may occur in several candidate nuclei, would verify the Majorana nature of the neutrino and constrain the absolute scale of the neutrino mass spectrum. Recent searches carried out with 76 Ge (GERDA experiment) and 136 Xe (KamLAND-Zen and EXO-200 experiments) have establi… Show more

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Cited by 386 publications
(324 citation statements)
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“…The dimension-six and -seven operators enter through the external sources, l µ , r µ , s, and p. Contributions from the dimension-six tensor operator require two additional derivatives which increase the chiral index by two. As such, the dominant contribution from C (6) T comes from the pion-nucleon sector which is discussed below.…”
Section: Mesonic Sectormentioning
confidence: 99%
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“…The dimension-six and -seven operators enter through the external sources, l µ , r µ , s, and p. Contributions from the dimension-six tensor operator require two additional derivatives which increase the chiral index by two. As such, the dominant contribution from C (6) T comes from the pion-nucleon sector which is discussed below.…”
Section: Mesonic Sectormentioning
confidence: 99%
“…The observation of 0νββ would have far reaching implications: it would demonstrate that neutrinos are Majorana fermions [2], shed light on the mechanism of neutrino mass generation, and give insight on leptogenesis scenarios for the generation of the matterantimatter asymmetry in the universe [3]. The current experimental limits on the halflives are already impressive [4][5][6][7][8][9][10][11][12][13], at the level of T 0ν 1/2 > 5.3 × 10 25 y for 76 Ge [12] and T 0ν 1/2 > 1.07 × 10 26 y for 136 Xe [13], with next generation ton-scale experiments aiming at a sensitivity of T 0ν 1/2 ∼ 10 27−28 y. By itself, the observation of 0νββ would not immediately point to the underlying physical origin of LNV.…”
Section: Introductionmentioning
confidence: 99%
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“…The authors thank J. Feintzeig, L. Gladstone, P. Mosteiro, and V. Singh for carefully reviewing the manuscript, M. Nastasi for preparing the 60 Co calibration sources, and F. Iachello for helpful discussions concerning the NME literature. [39], KamLAND-Zen [40] independently), and (c) 76 Ge (combined limit from Gerda, IGEX, HDM [41]). The vertical arrows aim to emphasize the range currently probed with each isotope.…”
Section: Fig 4 (Color Online)mentioning
confidence: 99%