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Alpha backgrounds in the AMoRE-Pilot experimentopen access

Authors
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.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.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.
Issue Date
Dec-2022
Publisher
SPRINGER
Citation
EUROPEAN PHYSICAL JOURNAL C, v.82, no.12, pp.1 - 13
Indexed
SCIE
SCOPUS
Journal Title
EUROPEAN PHYSICAL JOURNAL C
Volume
82
Number
12
Start Page
1
End Page
13
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/182357
DOI
10.1140/epjc/s10052-022-11104-3
ISSN
1434-6044
Abstract
The Advanced Mo-based Rare process Experiment (AMoRE)-Pilot experiment is an initial phase of the AMoRE search for neutrinoless double beta decay of Mo-100, with the purpose of investigating the level and sources of backgrounds. Searches for neutrinoless double beta decay generally require ultimately low backgrounds. Surface alpha 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 energy spectra fitted with the corresponding simulated spectra for six crystal detectors, where sources of background contributions could be identified through high energy alpha 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 contaminations by extrapolating from the alpha background fitting model.
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