标题： 超高能宇宙射线窄聚类与冰立方穿过μ子的相关性 显示英文标题

标题： UHECR narrow clustering correlating IceCube through-going muons

摘要： 最近的超高能宇宙射线事件由AUGER和望远镜阵列（TA）提出，表明北和南的宽集群，称为热点，与附近的AGN有关，例如M82和Cen A中的AGN。 在同一框架下，自2008年以来，我们假设超高能宇宙射线是由轻核和最轻的核组成的，以解释否则令人尴尬的附近室女座星系团的巨大缺失，这种缺失是由于最轻的核从室女座距离的光解离而变得脆弱和不透明。 此外，超高能宇宙射线图显示了一些狭窄的集群，一些靠近银河平面，如SS 433方向，以及在平面的另一侧的天际线：我们在2014年对它们进行了标记，建议可能的近源活动，同时也作为超高能中微子。 事实上，自去年以来，2015年，最高能量的IceCube穿过式μ子，数百TeV能量的超高能上行中微子事件，确实显示（在北天空标记的三个案例中有两个）了预期的超高能中微子信号与狭窄聚集的超高能宇宙射线的重叠。 新的数据具有更高的能量阈值，某种程度上重新确认了我们的初步提议；通过额外的相关超高能中微子与超高能中微子以及或与狭窄的超高能宇宙射线聚集事件，出现了新的可能来源。 遗迹中微子质量通过ZeV中微子散射可能起到一定作用。 显示英文摘要

摘要： The recent UHECR events by AUGER and the Telescope Array (TA) suggested that wide clusterings as the North and South, named Hot Spot, are related to near AGNs such as the one in M82 and Cen A. In the same frame since 2008 we assumed that the UHECR are made by light and lightest nuclei to explain the otherwise embarrassing absence of the huge nearby Virgo cluster, absence due to the fragility and the opacity of lightest nuclei by photo-dissociation from Virgo distances. Moreover UHECR map exhibits a few narrow clustering, some near the galactic plane, as toward SS 433 and on the opposite side of the plane at celestial horizons: we tagged them in 2014 suggesting possible near source active also as a UHE neutrino. Indeed since last year, 2015, highest IceCube trough-going muons, UHE up-going neutrino events at hundreds TeV energy, did show (by two cases over three tagged in North sky) the expected overlapping of UHE neutrinos signals with narrow crowding UHECR. New data with higher energy threshold somehow re-confirmed our preliminary proposal; new possible sources appear by a additional correlated UHE-neutrino versus UHE-neutrino and-or with narrow UHECR clustering events. A possible role of relic neutrino mass scattering by ZeV neutrino arised.