来自AMoRE-I的无中子双β衰变的改进极限

A. Agrawal, V. V. Alenkov, P. Aryal, J. Beyer, B. Bhandari, R. S. Boiko, K. Boonin, O. Buzanov, C. R. Byeon, N. Chanthima, M. K. Cheoun, J. S. Choe, Seonho Choi, S. Choudhury, J. S. Chung, F. A. Danevich, M. Djamal, D. Drung, C. Enss, A. Fleischmann, A. M. Gangapshev, L. Gastaldo, Y. M. Gavrilyuk, A. M. Gezhaev, O. Gileva, V. D. Grigorieva, V. I. Gurentsov, C. Ha, D. H. Ha, E. J. Ha, D. H. Hwang, E. J. Jeon, J. A. Jeon, H. S. Jo, J. Kaewkhao, C. S. Kang, W. G. Kang, V. V. Kazalov, S. Kempf, A. Khan, S. Khan, D. Y. Kim, G. W. Kim, H. B. Kim, Ho-Jong Kim, H. J. Kim, H. L. Kim, H. S. Kim, M. B. Kim, S. C. Kim, S. K. Kim, S. R. Kim, W. T. Kim, Y. D. Kim, Y. H. Kim, K. Kirdsiri, Y. J. Ko, V. V. Kobychev, V. Kornoukhov, V. V. Kuzminov, D. H. Kwon, C. H. Lee, DongYeup Lee, E. K. Lee, H. J. Lee, H. S. Lee, J. Lee, J. Y. Lee, K. B. Lee, M. H. Lee, M. K. Lee, S. W. Lee, Y. C. Lee, D. S. Leonard, H. S. Lim, B. Mailyan, E. P. Makarov, P. Nyanda, Y. Oh, S. L. Olsen, S. I. Panasenko, H. K. Park, H. S. Park, K. S. Park, S. Y. Park, O. G. Polischuk, H. Prihtiadi, S. Ra, S. S. Ratkevich, G. Rooh, M. B. Sari, J. Seo, K. M. Seo, B. Sharma, K. A. Shin, V. N. Shlegel, K. Siyeon, J. So, N. V. Sokur, J. K. Son, J. W. Song, N. Srisittipokakun, V. I. Tretyak, R. Wirawan, K. R. Woo, H. J. Yeon, Y. S. Yoon, Q. Yue
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Oh, S. L. Olsen, S. I. Panasenko, H. K. Park, H. S. Park, K. S. Park, S. Y. Park, O. G. Polischuk, H. Prihtiadi, S. Ra, S. S. Ratkevich, G. Rooh, M. B. Sari, J. Seo, K. M. Seo, B. Sharma, K. A. Shin, V. N. Shlegel, K. Siyeon, J. So, N. V. Sokur, J. K. Son, J. W. Song, N. Srisittipokakun, V. I. Tretyak, R. Wirawan, K. R. Woo, H. J. Yeon, Y. S. Yoon, Q. Yue","doi":"arxiv-2407.05618","DOIUrl":null,"url":null,"abstract":"AMoRE searches for the signature of neutrinoless double beta decay of\n$^{100}$Mo with a 100 kg sample of enriched $^{100}$Mo. Scintillating molybdate\ncrystals coupled with a metallic magnetic calorimeter operate at milli-Kelvin\ntemperatures to measure the energy of electrons emitted in the decay. As a\ndemonstration of the full-scale AMoRE, we conducted AMoRE-I, a pre-experiment\nwith 18 molybdate crystals, at the Yangyang Underground Laboratory for over two\nyears. The exposure was 8.02 kg$\\cdot$year (or 3.89\nkg$_{\\mathrm{^{100}Mo}}\\cdot$year) and the total background rate near the\nQ-value was 0.025 $\\pm$ 0.002 counts/keV/kg/year. We observed no indication of\n$0\\nu\\beta\\beta$ decay and report a new lower limit of the half-life of\n$^{100}$Mo $0\\nu\\beta\\beta$ decay as $\nT^{0\\nu}_{1/2}>3.0\\times10^{24}~\\mathrm{years}$ at 90\\% confidence level. 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引用次数: 0

摘要

AMoRE 利用 100 千克的富集 $^{100}$Mo 样品寻找 $^{100}$Mo 的无中子双贝塔衰变特征。闪烁钼酸盐晶体与金属磁性量热计在毫开尔文温度下运行,测量衰变中发射的电子能量。作为全面 AMoRE 的演示,我们在艳阳地下实验室进行了为期两年多的 AMoRE-I 预实验,实验中使用了 18 颗钼酸盐晶体。暴露量为每年 8.02 千克(或每年 3.89 千克),Q 值附近的总本底率为每年 0.025 个计数/千伏安/千克。我们没有观测到0\nu\beta\beta$衰变的迹象,并报告了一个新的$^{100}$Mo $0\nu\beta\beta$ 衰变半衰期下限,即在90%置信度下,$T^{0\nu}_{1/2}>3.0\times10^{24}~\mathrm{years}$。使用在不同模型框架下估计的核矩阵元素,包括最近的壳模型计算,有效马约拉纳质量极限范围为$m_{/beta/beta}<$(210--610) meV。
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Improved limit on neutrinoless double beta decay of \mohundred~from AMoRE-I
AMoRE searches for the signature of neutrinoless double beta decay of $^{100}$Mo with a 100 kg sample of enriched $^{100}$Mo. Scintillating molybdate crystals coupled with a metallic magnetic calorimeter operate at milli-Kelvin temperatures to measure the energy of electrons emitted in the decay. As a demonstration of the full-scale AMoRE, we conducted AMoRE-I, a pre-experiment with 18 molybdate crystals, at the Yangyang Underground Laboratory for over two years. The exposure was 8.02 kg$\cdot$year (or 3.89 kg$_{\mathrm{^{100}Mo}}\cdot$year) and the total background rate near the Q-value was 0.025 $\pm$ 0.002 counts/keV/kg/year. We observed no indication of $0\nu\beta\beta$ decay and report a new lower limit of the half-life of $^{100}$Mo $0\nu\beta\beta$ decay as $ T^{0\nu}_{1/2}>3.0\times10^{24}~\mathrm{years}$ at 90\% confidence level. The effective Majorana mass limit range is $m_{\beta\beta}<$(210--610) meV using nuclear matrix elements estimated in the framework of different models, including the recent shell model calculations.
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