在SuperCDMS中通过轫致辐射和Migdal效应搜寻低质量暗物质
A Search for Low-mass Dark Matter via Bremsstrahlung Radiation and the Migdal Effect in SuperCDMS
AI总结:
本文利用SuperCDMS数据,通过轫致辐射和Migdal效应两个非弹性散射通道搜寻亚GeV暗物质,将暗物质质量排除限分别推至220 MeV/c²和30 MeV/c²。
摘要:
我们利用轮廓似然框架对先前发表的SuperCDMS数据进行了新的分析,通过两个非弹性散射通道搜寻亚GeV暗物质粒子:轫致辐射和Migdal效应。考虑到这些可能的非弹性散射通道,在现有实验能量阈值的限制下,实验灵敏度可以扩展到通过暗物质-核子弹性散射通道无法探测到的暗物质质量范围。我们通过轫致辐射通道排除了质量低至$220~\ extrm{MeV}/c^2$、截面为$2.7 \ imes 10^{-30}~\ extrm{cm}^2$的暗物质。Migdal通道的搜寻总体上提供了显著更严格的限制,排除了质量低至$30~\ extrm{MeV}/c^2$、截面为$5.0 \ imes 10^{-30}~\ extrm{cm}^2$的暗物质。
英文摘要:
We present a new analysis of previously published of SuperCDMS data using a profile likelihood framework to search for sub-GeV dark matter (DM) particles through two inelastic scattering channels: bremsstrahlung radiation and the Migdal effect. By considering these possible inelastic scattering channels, experimental sensitivity can be extended to DM masses that are undetectable through the DM-nucleon elastic scattering channel, given the energy threshold of current experiments. We exclude DM masses down to $220~\textrm{MeV}/c^2$ at $2.7 \times 10^{-30}~\textrm{cm}^2$ via the bremsstrahlung channel. The Migdal channel search provides overall considerably more stringent limits and excludes DM masses down to $30~\textrm{MeV}/c^2$ at $5.0 \times 10^{-30}~\textrm{cm}^2$.
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。