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UHECR (Ultra High Energy Cosmic Rays) were expected to be protons, to flystraight and to suffer from a GZK (opacity on CMB radiation) cut off. AUGERsuggested in 2007 that such early UHECR anisotropy was compatible with theforeseen Super-Galactic plane, while both HIRES and AUGER confirmed thisapparent GZK cut-off in the spectra. However, the same AUGER composition since2007 had favored nuclei (and not nucleons). The recent absence of narrow angleclustering in UHECR maps, as it should be expected for protons, the missing ofevents along the nearest Cluster Virgo, the wide spread (nearly 16 degreeangle) of UHECR along Cen A are in disagreement with the first proton-UHECRAUGER understanding. Since 2008 we had claimed a light nuclei role for the CenA crowded area. However the ICECUBE absence of TeV neutrino clustering oranisotropy, its spectra steepening favors mostly a ruling atmospheric neutrinonoise up to tens TeV. However two recent PeV neutrino event, cannot easilycoexist or been extrapolated with such an atmospheric ruling scenario, or withGZK (either nucleons or nuclei) secondary expected spectra. Finally tens of TeVgamma anisotropy in ARGO-MILAGRO-ICECUBE maps may hardly be associated withknown hadronic sources. We imagine such anisotropy ruled by diffused gammasecondaries, shining along UHECR bending and flight: radioactive (Ni,Co,Al,D,neutron) light and heavy UHECR nuclei in GRB-SGRs-jet, while scattering ordecaying in flight, may paint in the sky (by gamma, electrons and neutrinossecondaries) their trajectories and bending, connecting UHECR spread eventswith TeV anisotropy, and also offering a very realistic source of first,otherwise puzzling, observed PeV neutrinos. Evidences for such relativistic Nijet in 4U1630-47 system has been observed recently by D\'iaz Trigocollaboration.

Radioactivity and fragmentation of UHECR: Correlating gamma anisotropy and neutrino PeV events