期刊
PHYSICAL REVIEW D
卷 99, 期 3, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.99.032008
关键词
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资金
- Canada Foundation for Innovation (CFI)
- Canada: Natural Sciences and Engineering Research Council
- Canada: Canadian Institute for Advanced Research (CIFAR)
- Canada: Queen's University at Kingston
- Canada: Ontario Ministry of Research, Innovation and Science
- Canada: Alberta Science and Research Investments Program
- Canada: National Research Council
- Canada: Federal Economic Development Initiative for Northern Ontario
- Canada: Northern Ontario Heritage Fund Corporation
- Canada: Ontario Early Researcher Awards
- U.S.: Department of Energy Office of Nuclear Physics
- U.S.: National Science Foundation
- U.S.: University of California, Berkeley
- U.S.: Department of Energy National Nuclear Security Administration through the Nuclear Science and Security Consortium
- UK: Science and Technology Facilities Council (STFC)
- UK: European Union's Seventh Framework Programme under the European Research Council (ERC) grant agreement
- UK: Marie Curie grant agreement
- Portugal: Fundacao para a Ciencia e a Tecnologia (FCT-Portugal)
- Germany: the Deutsche Forschungsgemeinschaft
- Mexico: DGAPA-UNAM
- Mexico: Consejo Nacional de Ciencia y Tecnologia
- SNOLAB
- WestGRID
- ComputeCanada
- University of Alberta
- Simon Fraser University
- GridPP Collaboration
- Rutherford Appleton Laboratory
- CFI
- Alberta Economic Development and Trade (EDT)
- UC Berkeley
- U.S. Department of Energy, Office of Science, Office of High Energy Physics
- STFC [ST/N000404/1, 1653414, SNO+, ST/N000307/1, 1945253, ST/K001329/1, 1935451, ST/N000420/1, ST/S000933/1] Funding Source: UKRI
This paper reports results from a search for nucleon decay through invisible modes, where no visible energy is directly deposited during the decay itself, during the initial water phase of SNO+. However, such decays within the oxygen nucleus would produce an excited daughter that would subsequently deexcite, often emitting detectable gamma rays. A search for such gamma rays yields limits of 2.5 x 10(29) y at 90% Bayesian credibility level (with a prior uniform in rate) for the partial lifetime of the neutron, and 3.6 x 10(29) y for the partial lifetime of the proton, the latter a 70% improvement on the previous limit from SNO. We also present partial lifetime limits for invisible dinucleon modes of 1.3 x 10(28) y for nn, 2.6 x 10(28) y for pn and 4.7 x 10(28) y for pp, an improvement over existing limits by close to 3 orders of magnitude for the latter two.
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