Assay-based background projection for the Majorana Demonstrator using Monte Carlo uncertainty propagation

I. J. Arnquist, F. T. Avignone, A. S. Barabash, C. J. Barton, K. H. Bhimani, E. Blalock, B. Bos, M. Busch, T. S. Caldwell, Y. D. Chan, C. D. Christofferson, P. H. Chu, M. L. Clark, C. Cuesta, J. A. Detwiler, Yu Efremenko, H. Ejiri, S. R. Elliott, N. Fuad, G. K. GiovanettiM. P. Green, J. Gruszko, I. S. Guinn, V. E. Guiseppe, C. R. Haufe, R. Henning, D. Hervas Aguilar, E. W. Hoppe, A. Hostiuc, M. F. Kidd, I. Kim, R. T. Kouzes, T. E. Lannen V, A. Li, J. M. López-Castaño, R. D. Martin, R. Massarczyk, S. J. Meijer, T. K. Oli, L. S. Paudel, W. Pettus, A. W.P. Poon, D. C. Radford, A. L. Reine, K. Rielage, N. W. Ruof, D. C. Schaper, S. J. Schleich, D. Tedeschi, R. L. Varner, S. Vasilyev, S. L. Watkins, J. F. Wilkerson, C. Wiseman, W. Xu, C. H. Yu

Research output: Contribution to journalArticlepeer-review

Abstract

The background index (BI) is an important quantity to project and calculate the half-life sensitivity of neutrinoless double-β decay (0νββ) experiments. An analysis framework is presented to calculate the BI using the specific activities, masses, and simulated efficiencies of an experiments components as distributions. This Bayesian framework includes a unified approach to combine specific activities from assay. Monte Carlo uncertainty propagation is used to build a BI distribution from the specific activity, mass, and efficiency distributions. This method is applied to the Majorana Demonstrator, which deployed arrays of high-purity Ge detectors enriched in Ge76 to search for 0νββ. The original assay-based projection is requantified in the new framework, using the as-built geometry of the Demonstrator and additional assay information. While 47% higher than the original projection, the resulting BI of [8.95±0.36]×10-4cts/(keVkgyr) from the Th232 and U238 decay chains does not account for the higher-Than-expected BI observed by the Demonstrator. This method enables us to demonstrate the statistical incompatibility between the Demonstrator's observed background and the assay results.

Original languageEnglish
Article number055804
JournalPhysical Review C
Volume110
Issue number5
DOIs
StatePublished - Nov 2024

Funding

This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Contracts/Awards No. DE-AC02-05CH11231, No. DE-AC05-00OR22725, No. DE-AC05-76RL0130, No. DE-FG02-97ER41020, No. DE-FG02-97ER41033, No. DE-FG02-97ER41041, No. DE-SC0012612, No. DE-SC0014445, No. DE-SC0017594, No. DE-SC0018060, No. DE-SC0022339, and No. LANLEM77/LANLEM78. We acknowledge support from the Particle Astrophysics Program and Nuclear Physics Program of the National Science Foundation through Grants No. MRI-0923142, No. PHY-1003399, No. PHY-1102292, No. PHY-1206314, No. PHY-1614611, No. PHY-1812409, No. PHY-1812356, No. PHY-2111140, and No. PHY-2209530. We gratefully acknowledge the support of the Laboratory Directed Research & Development (LDRD) program at Lawrence Berkeley National Laboratory for this work. We gratefully acknowledge the support of the U.S. Department of Energy through the Los Alamos National Laboratory LDRD Program, the Oak Ridge National Laboratory LDRD Program, and the Pacific Northwest National Laboratory LDRD Program for this work. We gratefully acknowledge the support of the South Dakota Board of Regents Competitive Research Grant. We acknowledge the support of the Natural Sciences and Engineering Research Council of Canada, funding Reference No. SAPIN-2017-00023, and from the Canada Foundation for Innovation John R. Evans Leaders Fund. We acknowledge support from the 2020/2021 L'Or\u00E9al-UNESCO for Women in Science Programme. This research used resources provided by the Oak Ridge Leadership Computing Facility at Oak Ridge National Laboratory and by the National Energy Research Scientific Computing Center, a U.S. Department of Energy Office of Science User Facility. We thank our hosts and colleagues at the Sanford Underground Research Facility for their support.

FundersFunder number
Oak Ridge National Laboratory LDRD Program
Pacific Northwest National Laboratory
Canada Foundation for Innovation John R. Evans Leaders Fund
Oak Ridge National Laboratory
National Energy Research Scientific Computing Center
Los Alamos National Laboratory
U.S. Department of Energy
South Dakota Board of Regents
Laboratory Directed Research and Development
Office of Science
National Science FoundationPHY-1003399, PHY-1812409, PHY-1614611, PHY-1206314, PHY-1102292, PHY-2209530, PHY-1812356, MRI-0923142, PHY-2111140
National Science Foundation
Natural Sciences and Engineering Research Council of CanadaSAPIN-2017-00023
Natural Sciences and Engineering Research Council of Canada
Nuclear PhysicsDE-AC05-00OR22725, DE-AC05-76RL0130, DE-AC02-05CH11231, DE-SC0012612, DE-FG02-97ER41020, DE-SC0017594, DE-FG02-97ER41033, LANLEM77/LANLEM78, DE-SC0022339, DE-SC0018060, DE-FG02-97ER41041, DE-SC0014445
Nuclear Physics

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