论文标题
回复Robinson and Michaud,Arxiv:2002.08893
Reply to Robinson and Michaud, arXiv:2002.08893
论文作者
论文摘要
我们回应了Robinson和Michaud(RM)评论(ARXIV:2002.08893)对我们最近的预印型ARXIV:2002.06937,在其中我们讨论了低阈值暗物质搜索的最新过度,并提供潜在的统一暗物质解释。我们感谢RM的反馈意见,这突出了对将来测量的至关重要的需求,以直接校准低$ \ sim $ 10 ev能量沉积的等离子体电荷收益率。 RM反对我们的断言,即在100〜EV以下的能量尺度下产生的等离子可能在声子中具有很大的分支分数。正如我们在下面提出的那样,RM提出的观点并没有使我们的主要结论无效,因为它们与我们在论文中讨论的能量量表大不相同。
We respond to Robinson and Michaud's (RM) comment (arXiv:2002.08893) on our recent preprint arXiv:2002.06937, in which we discuss recent excesses in low-threshold dark matter searches, and offer a potential unifying dark matter interpretation. We thank RM for their feedback, which highlights the critical need for future measurements to directly calibrate plasmon charge yields for low $\sim$ 10 eV energy depositions. RM objected to our assertion that plasmons generated at energy scales below 100~eV may have a large branching fraction into phonons. As we argue below, the points raised by RM do not invalidate our primary conclusions, as they pertain to a much different energy scale than we discuss in our paper.