当你无法关闭太阳时，分辨太阳中微子和太阳轴子
Telling Solar Neutrinos from Solar Axions When You Can't Shut Off the Sun
摘要：
XENON1 T实验最近报告了低电子反冲能量下的过量事件，这可能是由于探测器内太阳中微子通过大中微子磁矩的相互作用。我们指出，$^{51}$ Cr中微子源放置在靠近探测器可以直接测试这一假设。
英文摘要：
The XENON1T experiment recently reported an excess of events at low electron recoil energies, which may be due to interactions of solar neutrinos inside the detector via a large neutrino magnetic moment. We point out that a $^{51}$Cr neutrino source placed close to the detector can directly test this hypothesis.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
