D.Fargion; Rome Univ.1 and INFN , Rome , Italy Introduction;

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Ultra High Energy Cosmic Ray radioactivity in flight painting TeV anisotropy sky D.Fargion; Rome Univ.1 and INFN , Rome , Italy Introduction; The presence of large scale TeVs anisotropy in Milagro, ARGO, ICECUBE and today Hawc sky remain a mistery: how may charged cosmic rays at tens TeV remain correlated while being bent by local solar and galactic magnetic fields in an expected smeared nearly homogeneous maps? Consider the Main CR anisotropy nearby Crab D.Fargion_CERN_13-9-2016

There are two main TeVs CR anisotropy in last Hawc Map: Region A and B, C D.Fargion_CERN_13-9-2016

The previous ARGO multi-energy gamma-CR sky is somehow the most telling in this source search connection. D.Fargion_CERN_13-9-2016

The same image seen from an anticentric galactic coordinate Map based on Crab. The role of the TeV anisotropy below (A) is well linked to the pulsar Crab in the ARGO center map D.Fargion_CERN_13-9-2016

Consider the zoomed region A at TeV anisotropy not far from Crab D.Fargion_CERN_13-9-2016

Does the origin of the Milagro-ARGO-Hawc anisotropy A be the small square or the black (Crab) circle? Crab is the probable source D.Fargion_CERN_13-9-2016

How may tens TeV reach such kpc distances ? We considered_2012_ UHECR as mostly light (or lightest ) radioactive nuclei whose decay in flight may feed by alfa and neutron as well as by gamma secondaries at the tens TeVs anisotropy. D.Fargion_CERN_13-9-2016

Addditional Taces We showed in the past the overlapping of UHECR and TeV sky, with remarkable correlation, whose presence might point for nearby galactic sources as Crab, Vela, Cygnus X3 and maybe nearest AGN as Cen A. D.Fargion_CERN_13-9-2016

More recent maps (2015) of UHECR and TeVs anisotropy D.Fargion_CERN_13-9-2016

Conclusions UHECR by Light nuclei in flight and their decay may pollute by their (smeared) direction the tens TeV sky by He (alfa) and neutrons and gamma leading to present tiny large scale TeV anisotropy in sky. D.Fargion_CERN_13-9-2016

references arXiv:1412.1573 The meaning of the UHECR Hot Spots: A Light Nuclei Nearby Astronomy Daniele Fargion, Graziano Ucci, Pietro Oliva, Pier Giorgio De Sanctis Lucentini Journal-ref: EPJ Web Conf. 99 (2015) 08002; Conference: C14-08-18.1 Proceedings . arXiv:1209.6090 Radioactivity and fragmentation of UHECR: Correlating gamma anisotropy and neutrino PeV events Daniele Fargion : Acta Polytechnica 53(Supplement):718--723, 2013 . arXiv:1207.0254 TeV gamma-UHECR anisotropy by decaying nuclei in flight: first neutrino traces? Journal-ref: EPJ Web of Conferences, 2013 Vol, 53; 06005 . arXiv:1201.0157 TeV sky versus AUGER one: are UHECR also radioactive, heavy galactic nuclei? Nuclear Inst. and Methods in Physics Research, A (2012), pp. 174-179 . arXiv:1112.6388 Apart Cen A are UHECR mostly heavy radioactive and galactic nuclei? Journal-ref: IOP Publishing Journal of Physics, Conference Series 375 (2012) 052014 D.Fargion_CERN_13-9-2016

D.Fargion_CERN_13-9-2016