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arXiv 1306.5084physics.ins-dethep-ex
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无中微子双β衰变实验中的本底GERDA

The background in the neutrinoless double beta decay experiment GERDA

The GERDA collaboration, M. Agostini, M. Allardt, E. Andreotti, A. M. Bakalyarov, M. Balata, I. Barabanov, M. Barnabe Heider, N. Barros, L. Baudis, C. Bauer, N.… 展开作者

The GERDA collaboration, M. Agostini, M. Allardt, E. Andreotti, A. M. Bakalyarov, M. Balata, I. Barabanov, M. Barnabe Heider, N. Barros, L. Baudis, C. Bauer, N. Becerici-Schmidt, E. Bellotti, S. Belogurov, S. T. Belyaev, G. Benato, A. Bettini, L. Bezrukov, T. Bode, V. Brudanin, R. Brugnera, D. Budjas, A. Caldwell, C. Cattadori, A. Chernogorov, F. Cossavella, E. V. Demidova, A. Domula, V. Egorov, R. Falkenstein, A. Ferella, K. Freund, N. Frodyma, A. Gangapshev, A. Garfagnini, C. Gotti, P. Grabmayr, V. Gurentsov, K. Gusev, K. K. Guthikonda, W. Hampel, A. Hegai, M. Heisel, S. Hemmer, G. Heusser, W. Hofmann, M. Hult, L. V. Inzhechik, L. Ioannucci, J. Janicsko Csathy, J. Jochum, M. Junker, T. Kihm, I. V. Kirpichnikov, A. Kirsch, A. Klimenko, K. T. Knoepfle, O. Kochetov, V. N. Kornoukhov, V. V. Kuzminov, M. Laubenstein, A. Lazzaro, V. I. Lebedev, B. Lehnert, H. Y. Liao, M. Lindner, I. Lippi, X. Liu, A. Lubashevskiy, B. Lubsandorzhiev, G. Lutter, C. Macolino, A. A. Machado, B. Majorovits, W. Maneschg, I. Nemchenok, S. Nisi, C. O'Shaughnessy, D. Palioselitis, L. Pandola, K. Pelczar, G. Pessina, A. Pullia, S. Riboldi, C. Sada, M. Salathe, C. Schmitt, J. Schreiner, O. Schulz, B. Schwingenheuer, S. Schoenert, E. Shevchik, M. Shirchenko, H. Simgen, A. Smolnikov, L. Stanco, H. Strecker, M. Tarka, C. A. Ur, A. A. Vasenko, O. Volynets, K. von Sturm, V. Wagner, M. Walter, A. Wegmann, T. Wester, M. Wojcik, E. Yanovich, P. Zavarise, I. Zhitnikov, S. V. Zhukov, D. Zinatulina, K. Zuber, G. Zuzel

摘要:

INFN的Gran Sasso地下实验室(LNGS)的锗探测器阵列(GERDA)实验正在寻找76 Ge的无中微子双β衰变。信号的特征是在2039 keV处的单能峰,即衰变的Q值Q_bb。为了避免信号搜索中的偏差,本分析不考虑落在以Q_bb为中心的40 keV宽区域中的所有那些事件。本文叙述了无中微子双β衰变分析所需的主要参数。一个背景模型被开发来描述所观察到的能谱。该模型包含几个贡献,预计材料筛选的基础上,或通过观察能谱中的特征结构建立。该模型预测了在Q_bb附近的盲窗的平坦能谱,背景指数范围为17.6 ~ 23.8*10^{-3}计数/(keV kg yr)。一部分以前没有考虑过的数据被用来检验背景模型的预测是否一致。在这个能量区域中观察到的事件数量与背景模型一致。Q-bb的背景主要是近源,主要是由于42 K,214 Bi,228 Th,60 Co和来自226 Ra衰变链的α放射性同位素。各个分数取决于污染物的假定位置。它示出,除去已知的伽马峰后,能谱可以拟合在200 keV的能量范围内的Q_bb与恒定的背景。这给出了与完整模型一致的背景指数和相同大小的不确定性。

英文摘要:

The GERmanium Detector Array (GERDA) experiment at the Gran Sasso underground laboratory (LNGS) of INFN is searching for neutrinoless double beta decay of 76Ge. The signature of the signal is a monoenergetic peak at 2039 keV, the Q-value of the decay, Q_bb. To avoid bias in the signal search, the present analysis does not consider all those events, that fall in a 40 keV wide region centered around Q_bb. The main parameters needed for the neutrinoless double beta decay analysis are described. A background model was developed to describe the observed energy spectrum. The model contains several contributions, that are expected on the basis of material screening or that are established by the observation of characteristic structures in the energy spectrum. The model predicts a flat energy spectrum for the blinding window around Q_bb with a background index ranging from 17.6 to 23.8*10^{-3} counts/(keV kg yr). A part of the data not considered before has been used to test if the predictions of the background model are consistent. The observed number of events in this energy region is consistent with the background model. The background at Q-bb is dominated by close sources, mainly due to 42K, 214Bi, 228Th, 60Co and alpha emitting isotopes from the 226Ra decay chain. The individual fractions depend on the assumed locations of the contaminants. It is shown, that after removal of the known gamma peaks, the energy spectrum can be fitted in an energy range of 200 kev around Q_bb with a constant background. This gives a background index consistent with the full model and uncertainties of the same size.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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