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 the first place and would also clash with a certain number of other astrophysical observables. Quantitatively, the significance of the discrepancy ranges from $3.3\sigma$ for the rate of period change of pulsating white dwarfs and exceeds $19\sigma$ for the $R$ parameter and for $M_{I,\mathrm{TRGB}}$.

中文翻译：

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太阳轴无法解释XENON1T过量

我们认为，当面对恒星演化的天体物理观测结果时，关于近期XENON1T过量的太阳轴的解释是站不住脚的。我们讨论了为什么发出足够强烈的太阳轴通量来解释异常数据的原因将首先从根本上改变色度图中某些类型的恒星的分布，并且还会与其他数量的恒星发生冲突的原因。天体物理观测物。从数量上看，差异的重要性范围为$3.3\sigma$ 脉动白矮星周期变化率超过 $19\sigma$ 为了 $\mathrm{[R}$ 参数和 ${\mathrm{中号}}_{\mathrm{一世}，\mathrm{RGB}}$。