论文标题
对Xenon1t过量的响应响应：被忽视的暗物质签名？
Response-suggestion to The XENON1T excess: an overlooked dark matter signature?
论文作者
论文摘要
最近观察到最近的Xenon1t观察的主要选择是太阳轴，中微子磁矩和tri。在此简短说明中，我们建议通过搜索观察到的过量的行星依赖性来进行观察是否与暗物质（DM）流有关。如果得出了这样的相关性，则此提示（<3.5sigma）可能会成为被忽视的直接DM发现。为此，有必要分析所有Xenon1T数据的时间分布，尤其是使用其时间戳和能量的电子事件。值得注意的是，黑暗区域的速度可以通过单个天体或整个太阳系组合对地球产生行星的焦点效应。令人惊讶的是，即使DM速度适合行星重力透镜效应，这种可能性尚未在直接暗物质搜索领域中应用。需要重新定义广泛使用的直接暗物质搜索签名，而运气好的分析可能会确认或排除观察到的过量的太阳起源。因此，我们建议Xenon1t和Dama释放数据。
The main alternatives of the recent XENON1T observation are solar axions, neutrino magnetic moment and tritium. In this short note we suggest to crosscheck whether the observation is related or not to dark matter (DM) streams, by searching for planetary dependence of the observed excess. If such a correlation is derived, this hint (<3.5sigma) can become the overlooked direct DM discovery. To do this it is necessary to analyze the time distribution of all the XENON1T data, and in particular the electronic events with their time stamp and energy. Notably, the velocities of the dark sector allow for planetary focusing effects towards the earth either by a single celestial body or combined by the whole solar system. Surprisingly, as yet this possibility has not been applied in the field of direct dark matter search, even though DM velocities fit-in well planetary gravitational lensing effects. The widely used signature of a direct dark matter search needs to be redefined, while, with luck, such an analysis might confirm or exclude the solar origin of the observed excess. Therefore, we suggest that XENON1T and DAMA release the data.
