Why not any tau double bang in Icecube, yet?
Abstract
High Energy Neutrino Astronomy has been revealed by a sudden change in the flavor composition around maximal energies since three years of recording in ice km detector. However these discover didn' t led to any clear promised Neutrino Astronomy land yet. No correlation with hard gamma sources was found. Moreover the astrophysical spectra expected at Fermi value, seem to converge to a softer value, also required to avoid any Glashow resonant neutrino signal. We suggest a main solution within a composite flux ruled by prompt atmospheric neutrinos. Nevertheless the recent discover of twentyone crossing muons at hundreds TeVs had shown a first narrow overlapped doublet and a correlated track with a peculiar hard UHECR event clustering pointing to a well known microjet in bynary precession; these first connections hint for a non negligible astrophysical component making neutrino astronomy anyway already more than a hope.
Keywords
Cite
@article{arxiv.1512.08794,
title = {Why not any tau double bang in Icecube, yet?},
author = {D. Fargion and P. Oliva and G. Ucci},
journal= {arXiv preprint arXiv:1512.08794},
year = {2016}
}
Comments
11 pages, 3 figures