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  4. Search for neutrinoless double-β decay in ^{76}Ge with 26 kg yr of exposure from the Majorana Demonstrator

Search for neutrinoless double-β decay in ^{76}Ge with 26 kg yr of exposure from the Majorana Demonstrator

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Author(s)
Alvis, S. I.
•
Arnquist, I. J.
•
Avignone, F. T.
•
Barabash, A. S.
•
Barton, C. J.
•
Basu, V.
•
Bertrand, F. E.
•
Bos, B.
•
Busch, M.
•
Buuck, M.
more
Date Issued
August 23, 2019
Publisher
American Physical Society
Citation
Phys. Rev. C 100, 025501 (2019)
Version
Final published version
Abstract
The Majorana Collaboration is operating an array of high-purity Ge detectors to search for the neutrinoless double-β decay of ^{76}Ge. The Majorana Demonstrator consists of 44.1 kg of Ge detectors (29.7 kg enriched to 88% in ^{76}Ge) split between two modules constructed from ultraclean materials. Both modules are contained in a low-background shield at the Sanford Underground Research Facility in Lead, South Dakota. We present updated results on the search for neutrinoless double-β decay in ^{76}Ge with 26.0±0.5 kg yr of enriched exposure. With the Demonstrator's energy resolution of 2.53 keV FWHM at Q_{ββ}, which is the best among all neutrinoless double-β decay experiments, we observe one event in the region of interest with 0.65 events expected from the estimated background, resulting in a lower limit on the ^{76}Ge neutrinoless double-β decay half-life of 2.7×10^{25} yr [90% confidence level (CL)] with a median sensitivity of 4.8×10^{25} yr (90% CL). Depending on the matrix elements used, a 90% CL upper limit on the effective Majorana neutrino mass in the range of 200–433 meV is obtained. The measured background in the configurations with full shielding and optimized grounding is 11.9±2.0 counts/(FWHM t yr).
MIT Department
Massachusetts Institute of Technology. Department of Physics
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
https://hdl.handle.net/1721.1/136941
DOI of Published Version
https://doi.org/10.1103/PhysRevC.100.025501
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