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arXiv 1109.4154nucl-ex
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吨级~(76)Ge无中子双β衰变实验的深度要求

Depth Requirements for a Tonne-scale 76Ge Neutrinoless Double-beta Decay Experiment

The MAJORANA Collaboration, E. Aguayo, F. T. Avignone, H. O. Back, A. S. Barabash, M. Bergevin, F. E. Bertrand, M. Boswell, V. Brudanin, M. Busch, Y-D. Chan, C.… 展开作者

The MAJORANA Collaboration, E. Aguayo, F. T. Avignone, H. O. Back, A. S. Barabash, M. Bergevin, F. E. Bertrand, M. Boswell, V. Brudanin, M. Busch, Y-D. Chan, C. D. Christofferson, J. I. Collar, D. C. Combs, R. J. Cooper, J. A. Detwiler, P. J. Doe, Yu. Efremenko, V. Egorov, H. Ejiri, S. R. Elliott, J. Esterline, J. E. Fast, N. Fields, P. Finnerty, F. M. Fraenkle, V. M. Gehman, G. K. Giovanetti, M. P. Green, V. E. Guiseppe, K. Gusey, A. L. Hallin, R. Hazama, R. Henning, A. Hime, E. W. Hoppe, M. Horton, S. Howard, M. A. Howe, R. A. Johnson, K. J. Keeter, M. E. Keillor, C. Keller, J. D. Kephart, M. F. Kidd, A. Knecht, O. Kochetov, S. I. Konovalov, R. T. Kouzes, B. D. LaFerriere, B. H. LaRoque, J. Leon, L. E. Leviner, J. C. Loach, S. MacMullin, M. G. Marino, R. D. Martin, D. -M. Mei, J. H. Merriman, M. L. Miller, L. Mizouni, M. Nomachi, J. L. Orrell, N. R. Overman, D. G. Phillips, A. W. P. Poon, G. Perumpilly, G. Prior, D. C. Radford, K. Rielage, R. G. H. Robertson, M. C. Ronquest, A. G. Schubert, T. Shima, M. Shirchenko, K. J. Snavely, V. Sobolev, D. Steele, J. Strain, K. Thomas, V. Timkin, W. Tornow, I. Vanyushin, R. L. Varner, K. Vetter, K. Vorren, J. F. Wilkerson, B. A. Wolfe, E. Yakushev, A. R. Young, C. -H. Yu, V. Yumatov, C. Zhang

摘要:

无中微子双β衰变实验可以潜在地确定中微子的马约拉纳或狄拉克性质,并有助于理解中微子的绝对质量标度和等级。未来基于76 Ge的研究目标是半衰期灵敏度>10^27 y,以探索中微子的质量等级。要达到这种灵敏度,需要在衰变Q值周围的4 keV宽的感兴趣光谱区域内,背景速率<1计数吨^-1 y^-1。我们调查所需的超载,以达到这个背景的目标,在吨级的实验与紧凑的(铜和铅)屏蔽的基础上的宇宙射线背景率的蒙特卡罗计算。我们发现,鉴于目前在这些类型的计算中存在很大的不确定性,需要一个地下深度>~5200 mwe的场地进行吨级试验,该试验采用类似于计划中的40 kg MAJORANA演示器的紧凑屏蔽。所需的覆盖层高度依赖于所选择的屏蔽配置,并且如果例如采用液体冷冻剂和水屏蔽或主动中子屏蔽,则可以显著地放松。MAJORANA DEMONSTRATOR和GERDA探测器的运行将有助于减少宇宙射线背景速率的不确定性,并将影响未来吨级实验的屏蔽类型和位置的选择。2013年4月:同行审议进程显示,需要更好地确定否决权拒绝因素之一(第12页所述的4的因素)。我们对这一参数的重新评估迄今为止没有得到对手稿中所述值的有力支持,我们需要进一步研究以得出可靠的估计。这项进一步的研究将取代本文中所描述的工作,并且可能会或可能不会导致关于未来吨级76 Ge无中微子双β衰变实验的~>5200 mwe要求的相同结论。

英文摘要:

Neutrinoless double-beta decay experiments can potentially determine the Majorana or Dirac nature of the neutrino, and aid in understanding the neutrino absolute mass scale and hierarchy. Future 76Ge-based searches target a half-life sensitivity of >10^27 y to explore the inverted neutrino mass hierarchy. Reaching this sensitivity will require a background rate of <1 count tonne^-1 y^-1 in a 4-keV-wide spectral region of interest surrounding the Q value of the decay. We investigate the overburden required to reach this background goal in a tonne-scale experiment with a compact (copper and lead) shield based on Monte Carlo calculations of cosmic-ray background rates. We find that, in light of the presently large uncertainties in these types of calculations, a site with an underground depth >~5200 mwe is required for a tonne-scale experiment with a compact shield similar to the planned 40-kg MAJORANA DEMONSTRATOR. The required overburden is highly dependent on the chosen shielding configuration and could be relaxed significantly if, for example, a liquid cryogen and water shield, or an active neutron shield were employed. Operation of the MAJORANA DEMONSTRATOR and GERDA detectors will serve to reduce the uncertainties on cosmic-ray background rates and will impact the choice of shielding style and location for a future tonne-scale experiment. 4/2013: The peer review process revealed that one of the veto rejection factors (the factor-of-4 described on p12) needs to be better established. Our reevaluation of this parameter to date has not yielded strong support for the value stated in the manuscript, and we require further study to develop a solid estimate. This further study will supersede the work described in this manuscript, and may or may not lead to the same conclusion regarding the ~>5200 mwe requirement for future tonne-scale 76Ge neutrinoless double beta decay experiments.

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