Neutrinos of Energy [Formula presented] from Gamma-Ray Bursts in Pulsar Wind Bubbles

The supranova model for [Formula presented]-ray bursts (GRBs) is becoming increasingly more popular. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). Protons accelerated in the internal shocks that emit the GRB may interact with the external PWB photons producing pions which decay into [Formula presented] neutrinos. A [Formula presented] neutrino detector would observe several events per year correlated with the GRBs.