利用展望实验改进了短基线中微子振荡搜索和能谱测量

M. Andriamirado, A. Balantekin, H. Band, C. Bass, D. Bergeron, D. Berish, N. Bowden, J. Brodsky, C. Bryan, T. Classen, A. Conant, G. Deichert, M. Diwan, M. Dolinski, A. Erickson, B. Foust, J. Gaison, A. Galindo-Uribarri, C. Gilbert, B. Goddard, B. Hackett, S. Hans, A. Hansell, K. Heeger, D. Jaffe, X. Ji, D. C. Jones, O. Kyzylova, C. Lane, T. Langford, J. Larosa, B. Littlejohn, X. Lu, J. Maricic, M. Mendenhall, A. Meyer, R. Milincic, I. Mitchell, P. Mueller, H. Mumm, J. Napolitano, C. Nave, R. Neilson, J. Nikkel, D. Norcini, S. Nour, J. Palomino, D. Pushin, X. Qian, E. Romero-Romero, R. Rosero, P. T. Surukuchi, M. A. Tyra, R. Varner, D. Venegas-Vargas, P. Weatherly, C. White, J. Wilhelmi, A. Woolverton, M. Yeh, A. Zhang, C. Zhang, X. Zhang
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引用次数: 59

摘要

本文详细报道了橡树岭国家实验室高富集高通量同位素堆(HFIR) PROSPECT实验的无菌中微子振荡和U-235反中微子能谱测量结果。在距离85兆瓦HFIR核心中心平均基线距离7.9米的96个日历日的数据中,PROSPECT探测器观察到U-235裂变产物衰变中产生的5万多个反中微子相互作用。通过比较10个在6.7和9.2米之间的反应堆-探测器基线检测到的能谱,已经确定了反中微子到轻惰性中微子振荡的新极限。基线之间测得的能谱差异显示,反中微子对无菌中微子振荡没有统计学意义,不利于反应堆反中微子异常在2.5 $\sigma$置信水平上的最佳拟合点。所报道的U-235反中微子能谱测量结果与U-235 β能谱转换生成的能谱模型非常吻合,$\chi^2$ /DOF为31/31。PROSPECT能够在2.4 $\sigma$置信水平上否定U-235反中微子是造成模型和商业反应堆堆芯数据之间光谱差异的唯一原因的假设。相对于没有观测到的偏差,在2.2 $\sigma$置信水平上,PROSPECT数据模型偏差与商业岩心实验观测到的偏差相似。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Improved short-baseline neutrino oscillation search and energy spectrum measurement with the PROSPECT experiment at HFIR
We present a detailed report on sterile neutrino oscillation and U-235 antineutrino energy spectrum measurement results from the PROSPECT experiment at the highly enriched High Flux Isotope Reactor (HFIR) at Oak Ridge National Laboratory. In 96 calendar days of data taken at an average baseline distance of 7.9 m from the center of the 85 MW HFIR core, the PROSPECT detector has observed more than 50,000 interactions of antineutrinos produced in beta decays of U-235 fission products. New limits on the oscillation of antineutrinos to light sterile neutrinos have been set by comparing the detected energy spectra of ten reactor-detector baselines between 6.7 and 9.2 meters. Measured differences in energy spectra between baselines show no statistically significant indication of antineutrinos to sterile neutrino oscillation and disfavor the Reactor Antineutrino Anomaly best-fit point at the 2.5$\sigma$ confidence level. The reported U-235 antineutrino energy spectrum measurement shows excellent agreement with energy spectrum models generated via conversion of the measured U-235 beta spectrum, with a $\chi^2$/DOF of 31/31. PROSPECT is able to disfavor at 2.4$\sigma$ confidence level the hypothesis that U-235 antineutrinos are solely responsible for spectrum discrepancies between model and data obtained at commercial reactor cores. A data-model deviation in PROSPECT similar to that observed by commercial core experiments is preferred with respect to no observed deviation, at a 2.2$\sigma$ confidence level.
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