论文标题
太阳轴无法解释Xenon1t多余
Solar axions cannot explain the XENON1T excess
论文作者
论文摘要
我们认为，当面对恒星进化的天体物理观察结果时，近期Xenon1t过量的太阳轴上的解释是不可替代的。我们讨论了为什么太阳轴的通量足够强烈以解释异常数据的原因将一开始就会改变某些类型的恒星在颜色数字图中的分布，并且还将与其他一定数量的天体物理观测值发生冲突。数量上，差异的重要性范围从脉动白矮人的周期变化率的$3.3σ$不等，对于$ r $ - 参数的$19σ$，$19σ$，$ m_ {i，{\ rm trgb}}} $。
We argue that the interpretation in terms of solar axions of the recent XENON1T excess is not tenable when confronted with astrophysical observations of stellar evolution. We discuss the reasons why the emission of a flux of solar axions sufficiently intense to explain the anomalous data would radically alter the distribution of certain type of stars in the color-magnitude diagram in first place, and would also clash with a certain number of other astrophysical observables. Quantitatively, the significance of the discrepancy ranges from $3.3σ$ for the rate of period change of pulsating White Dwarfs, and exceedes $19σ$ for the $R$-parameter and for $M_{I,{\rm TRGB}}$.
