2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/184807In this paper we discuss possible ultra high energy ($\ge$ TeV) neutrino emission from Supernova Remnants (SNRs), specifically the hadronic gamma ray production models. Recent very high energy (VHE) $γ$ ray observation from SNRs is the main motivation behind this study.6 pages, 3 figures, uses revtexAstrophysicstext