Department of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom.
Instituto de Física, Universidade de São Paulo, São Paulo 05508-090, Brazil.
Phys Rev Lett. 2023 Mar 10;130(10):101001. doi: 10.1103/PhysRevLett.130.101001.
Dark matter elastic scattering off nuclei can result in the excitation and ionization of the recoiling atom through the so-called Migdal effect. The energy deposition from the ionization electron adds to the energy deposited by the recoiling nuclear system and allows for the detection of interactions of sub-GeV/c^{2} mass dark matter. We present new constraints for sub-GeV/c^{2} dark matter using the dual-phase liquid argon time projection chamber of the DarkSide-50 experiment with an exposure of (12 306±184) kg d. The analysis is based on the ionization signal alone and significantly enhances the sensitivity of DarkSide-50, enabling sensitivity to dark matter with masses down to 40 MeV/c^{2}. Furthermore, it sets the most stringent upper limit on the spin independent dark matter nucleon cross section for masses below 3.6 GeV/c^{2}.
暗物质与原子核的弹性散射可能会通过所谓的 Migdal 效应导致反冲原子的激发和电离。电离电子的能量沉积与反冲核系统的能量沉积相加,从而允许探测亚 GeV/c^{2}质量暗物质的相互作用。我们使用 DarkSide-50 实验的双相液态氩时间投影室展示了新的亚 GeV/c^{2}暗物质限制,该实验的曝光量为 (12 306±184) kg d。该分析仅基于电离信号,极大地提高了 DarkSide-50 的灵敏度,使其能够探测质量低至 40 MeV/c^{2}的暗物质。此外,它为质量低于 3.6 GeV/c^{2}的暗物质与核子的自旋无关相互作用设定了最严格的上限。