Alpha backgrounds in the AMoRE-Pilot experiment
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Published:2022-12-16
Issue:12
Volume:82
Page:
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ISSN:1434-6052
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Container-title:The European Physical Journal C
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language:en
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Short-container-title:Eur. Phys. J. C
Author:
Alenkov V., Bae H. W., Beyer J., Boiko R. S., Boonin K., Buzanov O., Chanthima N., Cheoun M. K., Choi S. H., Danevich F. A., Djamal M., Drung D., Enss C., Fleischmann A., Gangapshev A., Gastaldo L., Gavriljuk Yu. M., Gezhaev A., Grigoryeva V. D., Gurentsov V., Ha D. H., Ha C., Ha E. J., Hahn I., Jeon E. J.ORCID, Jeon J., Jo H. S., Kaewkhao J., Kang C. S., Kang S. J., Kang W. G., Karki S., Kazalov V., Khan A., Khan S., Kim D.-Y., Kim G. W., Kim H. B., Kim H. J., Kim H. L., Kim H. S., Kim I., Kim W. T., Kim S. R., Kim S. C., Kim S. K., Kim Y. D., Kim Y. H., Kirdsiri K., Ko Y. J., Kobychev V. V., Kornoukhov V., Kuz’minov V., Kwon D. H., Lee C., Lee E. K., Lee H. J., Lee H. S., Lee J., Lee J. S., Lee J. Y., Lee K. B., Lee M. H., Lee M. K., Lee S. H., Lee S. W., Lee S. W., Leonard D. S., Li J., Li Y., Limkitjaroenporn P., Mailyan B., Makarov E. P., Oh S. Y., Oh Y. M., Gileva O., Olsen S., Pabitra A., Panasenko S., Pandey I., Park C. W., Park H. K., Park H. S., Park K. S., Park S. Y., Polischuk O. G., Prihtiadi H., Ra S. J., Ratkevich S., Rooh G., Sari M. B., Seo J., Seo K. M., Shin J. W., Shin K. A., Shlegel V. N., Siyeon K., Sokur N. V., Son J.-K., Srisittipokakun N., Toibaev N., Tretyak V. I., Wirawan R., Woo K. R., Yoon Y. S., Yue Q.
Abstract
AbstractThe Advanced Mo-based Rare process Experiment (AMoRE)-Pilot experiment is an initial phase of the AMoRE search for neutrinoless double beta decay of $$^{100}$$
100
Mo, with the purpose of investigating the level and sources of backgrounds. Searches for neutrinoless double beta decay generally require ultimately low backgrounds. Surface $$\alpha $$
α
decays on the crystals themselves or nearby materials can deposit a continuum of energies that can be as high as the Q-value of the decay itself and may fall in the region of interest (ROI). To understand these background events, we studied backgrounds from radioactive contaminations internal to and on the surface of the crystals or nearby materials with Geant4-based Monte Carlo simulations. In this study, we report on the measured $$\alpha $$
α
energy spectra fitted with the corresponding simulated spectra for six crystal detectors, where sources of background contributions could be identified through high energy $$\alpha $$
α
peaks and continuum parts in the energy spectrum for both internal and surface contaminations. We determine the low-energy contributions from internal and surface $$\alpha $$
α
contaminations by extrapolating from the $$\alpha $$
α
background fitting model.
Funder
National Research Foundation Institute for Basic Science Ministry of Science and Higher Education of the Russian Federation
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Reference39 articles.
1. Stefano Dell’Oro, Simone Marcocci, Matteo Viel, Francesco Vissani, Adv. High Energy Phys. 2016, 2162659 (2016). https://doi.org/10.1155/2016/2162659 2. R.N. Mohapatra et al., Rep. Prog. Phys. 70, 1757–1867 (2007). https://doi.org/10.1088/0034-4885/70/11/R02 3. P.A. Zyla et al., (Particle Data Group), Prog. Theor. Exp. Phys. 8, 083C01 (2020). https://doi.org/10.1093/ptep/ptaa104 4. C. Giunti, C.W. Kim, Fundamentals of Neutrino Physics and Astrophysics, Oxford, UK: Univ. Pr. 10, (2007). https://doi.org/10.1093/acprof:oso/9780198508717.001.0001 5. A. Gando, Y. Gando, T. Hachiya et al., Phys. Rev. Lett. 117, 082503 (2016). https://doi.org/10.1103/PhysRevLett.117.082503
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