论文标题
Xenon1t数据中的系统学:15击反轴
Systematics in the XENON1T data: the 15-keV anti-axion
论文作者
论文摘要
Xenon1t的合作发现其科学中的电子后坐力事件过多的1个数据低于〜7 keV,其光谱形状与太阳能轴诱导的信号的预期一致。在零假设上,太阳能轴模型的统计显着性为3.5 $σ$。在这项工作中,我们为电子后坐力数据中的不构层次化提供了证据,这些数据可能会将轴突模型的局部意义降低到低至$ p \ 0.1 $。为了得出这一结论,我们搜索具有太阳轴模型的光谱模板的信号,但转移到了〜7 keV以上的较高(非物理)能量。我们发现,从该侧波段分析中发现的显着性分布并不遵循预期的卡方分布,这使我们能够量化不s灭模块可能影响到〜7 KEV以下能量的数据的解释程度。例如,我们发现当太阳轴模型的能量向上移动〜15 keV并允许具有负归一化时,与数据具有更高的拟合度。
The XENON1T collaboration has found an excess of electron recoil events in their Science Run 1 data below ~7 keV with a spectral shape consistent with that expected from a solar-axion-induced signal. The claimed statistical significance of the solar-axion model over the null hypothesis is 3.5$σ$. In this work we provide evidence for mismodeling in the electron recoil data that may decrease the local significance of the axion model to as low as $p \approx 0.1$. To reach this conclusion, we search for a signal with the spectral template of the solar axion model, but shifted to higher (unphysical) energies above ~7 keV. We find that the distribution of significances found from this side-band analysis does not follow the expected chi-square distribution, which allows us to quantify the extent to which mismodeling may be affecting the interpretation of the data at energies below ~7 keV. For example, we find that there is an even higher-significance fit to the data when the solar axion model is shifted upwards in energy by ~15 keV and allowed to have a negative normalization.