2017
DOI: 10.1063/1.5007637
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Search for neutrinoless double beta decay with GERDA phase II

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Cited by 19 publications
(32 citation statements)
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“…We study scenarios involving multiple couplings in section 8. We apply the following experimental limits [7,12,13,86] In table 6 we show bounds on m ββ and the low-energy dimension-six, -seven, and -nine operators of eq. (3.4), which were derived using the NMEs of refs.…”
Section: Single-coupling Constraintsmentioning
confidence: 99%
See 1 more Smart Citation
“…We study scenarios involving multiple couplings in section 8. We apply the following experimental limits [7,12,13,86] In table 6 we show bounds on m ββ and the low-energy dimension-six, -seven, and -nine operators of eq. (3.4), which were derived using the NMEs of refs.…”
Section: Single-coupling Constraintsmentioning
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: 98%
“…High-purity Germanium (HPGe) is a good target and detector that can be used in both experiments. Since a lot of efforts have been devoted to suppress the background of the HPGe detector system, including operating in deep underground laboratories, carefully selecting low radioactive materials, producing necessary parts underground, and building active and passive shields, the background level can be typically decreased to about 1 count/(keV·kg·day) (cpkkd) for direct light dark matter detection at 2 ∼ 4 keV energy range [1,2] and about 10 −6 cpkkd for 0νββ decay detection at Q ββ of 2039 keV in recent years [3][4][5][6]. In addition to primordial radionuclides, cosmogenic radionuclides in crystals can contribute crucial backgrounds.…”
mentioning
confidence: 99%
“…The ability to detect scintillation light allows to reject backgrounds with coincident energy release in HPGe detectors and LAr [8]. Results from Phase II were published in [9,11]. A detailed description of the GERDA Phase II setup can be found in [12].…”
Section: Gerdamentioning
confidence: 99%