论文标题
Xenon1t信号来自过渡中微子磁矩
XENON1T signal from transition neutrino magnetic moments
论文作者
论文摘要
Xenon1T在几个KEV电子后坐力上的最新令人困惑的结果可能是由于太阳中微子的散射赋予了有限的Majorite Majorana转变磁矩（TMMS）。在这样的一般形式主义中，我们发现Xenon1t数据中观察到的过量与此解释非常吻合。所需的TMM强度位于当前实验设定的限制内，例如Borexino，特别是当人们考虑到可能的tri污染时。
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.
