Abstract The recent puzzling results of the XENON1T collaboration at few keV electronic recoils could be due to the scattering of solar neutrinos endowed with finite Majorana transition magnetic moments (TMMs). Within such general formalism, we find that the observed excess in the XENON1T data agrees well with this interpretation. The required TMM strengths lie within the limits set by current experiments, such as Borexino, specially when one takes into account a possible tritium contamination.

中文翻译：

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来自跃迁中微子磁矩的 XENON1T 信号

摘要 XENON1T 合作在几个 keV 电子反冲下的最近令人费解的结果可能是由于具有有限马约拉纳跃迁磁矩 (TMM) 的太阳中微子的散射。在这种一般形式主义中，我们发现 XENON1T 数据中观察到的过量与这种解释非常吻合。所需的 TMM 强度在当前实验（例如 Borexino）设定的范围内，特别是当考虑到可能的氚污染时。