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Cosmic Rays Above The Second Knee From Clusters Of Galaxies And Associated High-energy Neutrino Emission

机译:星系团和相关的高能中微子发射引起的第二个膝盖上方的宇宙射线

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Accretion and merger shocks in clusters of galaxies are potential accelerators of high-energy protons, which can give rise to high-energy neutrinos through pp interactions with the intracluster gas. We discuss the possibility that protons from cluster shocks make a significant contribution to the observed cosmic rays in the energy range between the second knee at ~10~(17.5) eV and the ankle at ~10~(18.5) eV. The accompanying cumulative neutrino background above ~PeV may be detectable by upcoming neutrino telescopes such as IceCube or KM3NeT, providing a test of this scenario as well as a probe of cosmic-ray confinement properties in clusters.
机译:星系团中的增生和合并冲击是高能质子的潜在加速器,通过与团簇内气体的pp相互作用可以产生高能中微子。我们讨论了簇冲击的质子在第二个膝盖在〜10〜(17.5)eV和踝关节在〜10〜(18.5)eV之间的能量范围内对观察到的宇宙射线做出重大贡献的可能性。即将出现的中微子望远镜(如IceCube或KM3NeT)可能会探测到〜PeV以上伴随的累积中微子本底,从而提供了对这种情况的测试以及对星团中宇宙射线约束性质的探测。

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