利用萨德伯里中微子天文台寻找hep中微子
Searching for hep Neutrinos using the Sudbury Neutrino Observatory
摘要：
萨德伯里中微子天文台最近完成了第三阶段也是最后阶段的工作，积累了超过1082天的中微子数据，能量范围约为5-20 MeV。几乎所有观测到的中微子都是由太阳中的8B反应引起的。所谓的hep过程（3 He + p -> 4 He + e + nu_e）也发生在太阳中，但尚未被观察到。hep中微子的能量端点延伸到8B谱以上。本文介绍了三相分析，最终将是最敏感的反应。
英文摘要：
The Sudbury Neutrino Observatory has recently finished its third and final phase, and has accumulated over 1082 days of neutrino data, spanning the energy range from approximately 5-20 MeV. Almost all the observed neutrinos are due to the 8B reaction in the Sun. The so-called hep process (3He + p -> 4He + e + nu_e) also occurs in the Sun, but has not yet been observed. hep neutrino energy endpoint extends above the 8B spectrum. This paper describes the three phase analysis that will ultimately be the most sensitive to this reaction.
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。
