TY - JOUR
T1 - Neutrinos of Energy [Formula presented] from Gamma-Ray Bursts in Pulsar Wind Bubbles
AU - Guetta, Dafne
AU - Granot, Jonathan
N1 - Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 2003
Y1 - 2003
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85038328906&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.90.201103
DO - 10.1103/PhysRevLett.90.201103
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C2 - 12785881
AN - SCOPUS:85038328906
SN - 0031-9007
VL - 90
SP - 4
JO - Physical Review Letters
JF - Physical Review Letters
IS - 20
ER -