4.7 Article

Search for invisible modes of nucleon decay in water with the SNO plus detector

期刊

PHYSICAL REVIEW D
卷 99, 期 3, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.99.032008

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资金

  1. Canada Foundation for Innovation (CFI)
  2. Canada: Natural Sciences and Engineering Research Council
  3. Canada: Canadian Institute for Advanced Research (CIFAR)
  4. Canada: Queen's University at Kingston
  5. Canada: Ontario Ministry of Research, Innovation and Science
  6. Canada: Alberta Science and Research Investments Program
  7. Canada: National Research Council
  8. Canada: Federal Economic Development Initiative for Northern Ontario
  9. Canada: Northern Ontario Heritage Fund Corporation
  10. Canada: Ontario Early Researcher Awards
  11. U.S.: Department of Energy Office of Nuclear Physics
  12. U.S.: National Science Foundation
  13. U.S.: University of California, Berkeley
  14. U.S.: Department of Energy National Nuclear Security Administration through the Nuclear Science and Security Consortium
  15. UK: Science and Technology Facilities Council (STFC)
  16. UK: European Union's Seventh Framework Programme under the European Research Council (ERC) grant agreement
  17. UK: Marie Curie grant agreement
  18. Portugal: Fundacao para a Ciencia e a Tecnologia (FCT-Portugal)
  19. Germany: the Deutsche Forschungsgemeinschaft
  20. Mexico: DGAPA-UNAM
  21. Mexico: Consejo Nacional de Ciencia y Tecnologia
  22. SNOLAB
  23. WestGRID
  24. ComputeCanada
  25. University of Alberta
  26. Simon Fraser University
  27. GridPP Collaboration
  28. Rutherford Appleton Laboratory
  29. CFI
  30. Alberta Economic Development and Trade (EDT)
  31. UC Berkeley
  32. U.S. Department of Energy, Office of Science, Office of High Energy Physics
  33. STFC [ST/N000404/1, 1653414, SNO+, ST/N000307/1, 1945253, ST/K001329/1, 1935451, ST/N000420/1, ST/S000933/1] Funding Source: UKRI

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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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