School of Chemistry and Physics, University of Adelaide, Adelaide, South Australia 5005, Australia.
Phys Rev Lett. 2013 Mar 29;110(13):131302. doi: 10.1103/PhysRevLett.110.131302. Epub 2013 Mar 28.
We have performed a search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first time, the DeepCore subarray is included in the analysis, lowering the energy threshold and extending the search to the austral summer. The 317 days of data collected between June 2010 and May 2011 are consistent with the expected background from atmospheric muons and neutrinos. Upper limits are set on the dark matter annihilation rate, with conversions to limits on spin-dependent and spin-independent scattering cross sections of weakly interacting massive particles (WIMPs) on protons, for WIMP masses in the range 20-5000 GeV/c2. These are the most stringent spin-dependent WIMP-proton cross section limits to date above 35 GeV/c2 for most WIMP models.
我们使用 IceCube 中微子望远镜的 79 根-string 配置,在太阳中心进行了暗物质湮灭中微子的搜索。这是 DeepCore 子探测器首次被纳入分析,降低了能量阈值并将搜索范围扩展到了南半球的夏季。2010 年 6 月至 2011 年 5 月期间收集的 317 天数据与预期的大气中微子和中微子背景一致。我们对暗物质湮灭率设置了上限,并将其转换为对弱相互作用大质量粒子(WIMP)与质子的自旋相关和自旋无关散射截面的限制,WIMP 质量在 20-5000 GeV/c2 范围内。对于大多数 WIMP 模型,这些是迄今为止在 35 GeV/c2 以上最严格的自旋相关 WIMP-质子散射截面限制。