High-energy neutrino emission from the core of low luminosity AGNs triggered by magnetic reconnection acceleration

摘要: The detection of astrophysical very high energy (VHE) neutrinos in the range TeV-PeV energies by IceCube observatory has opened a new season astrophysics. Energies ~PeV imply that are originated from sources where cosmic rays (CRs) can be accelerated up to ~ 10^{17}eV. Recently, we have shown observed TeV gamma-rays radio-galaxies may hadronic origin their nuclear region and such case this could lead neutrino production. In paper show relativistic protons magnetic reconnection core these produce VHE via decay charged pions produced photo-meson process. We also calculated diffuse flux found it associated data.