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Searches for Dark Matter Annihilations in the Sun with IceCube and DeepCore in the 79-string configuration

机译:在79字符串配置中搜索在Sun中的暗物质湮灭,在79字符串配置中使用iceCube和Deepcore

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Dark matter could be indirectly detected through the observation of neutrinos produced as part of itsself-annihilation process. Possible signatures are an excess neutrino flux from the Sun, where dark matter could begravitationally trapped. The recent commissioning of the full DeepCore sub-array, a low-energy extension of theIceCube neutrino observatory, offers exciting opportunities for neutrino physics in the energy region of 10 GeV to 1 TeV.DeepCore's improved energy reach will, in particular, provide sensitivity to neutrinos from attractive WIMP candidates,like the neutralino or the lightest Kaluza-Klein particle (LKP), down to WIMP masses in the region of about 50 GeV.This will lead to stringent upper limits on the flux of muons from dark matter annihilations in the Sun and constraints onWIMP-proton cross-sections. We report on the search for dark matter annihilations in the Sun with the IceCube neutrinodetector in the 79-string configuration, which includes the full DeepCore sub-array. Furthermore, we review the impactsof IceCube observations of the Sun upon supersymmetric (SUSY) dark matter models.
机译:暗物质可以通过如itsself湮灭过程的一部分产生的中微子的观察来间接地检测。可能的签名是由太阳,在那里暗物质可能begravitationally被困过量中微子流量。最近调试全DeepCore子阵列的,theIceCube中微子天文台的低能量扩展名,在10 GeV的1 TeV.DeepCore的提高能达到的能量区域中微子物理提供了令人兴奋的机会将,特别是提供灵敏度中微子从有吸引力的候选WIMP,如中性微或最轻克鲁札 - 克莱因粒子(LKP),下降到WIMP群众在约50 GeV.This该区域将导致严谨上μ子从暗物质湮灭通量上限Sun和约束onWIMP质子横截面。我们在寻找在Sun暗物质湮灭与冰块neutrinodetector在79串的配置,包括全DeepCore子阵列报告。此外,我们在超对称(超对称)暗物质模型审查impactsof太阳的冰块观察。

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