TY - JOUR
T1 - Neutrino signatures of the supernova
T2 - Gamma ray burst relationship
AU - Razzaque, Soebur
AU - Mészáros, Peter
AU - Waxman, Eli
PY - 2004
Y1 - 2004
N2 - We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and gamma-ray burst events down to much shorter time scales than what can be resolved with photons. As an illustrative example, we calculate the probability of neutrino induced muon and electron cascade events in a km scale under-ice detector at the South Pole, from the GRB 030329. Our calculations demonstrate that km scale neutrino telescopes are expected to detect signals that will allow us to constrain supernova-GRB models.
AB - We calculate the TeV-PeV neutrino fluxes of gamma-ray bursts associated with supernovae, based on the observed association between GRB 030329 and supernova SN 2003dh. The neutrino spectral flux distributions can test for possible delays between the supernova and gamma-ray burst events down to much shorter time scales than what can be resolved with photons. As an illustrative example, we calculate the probability of neutrino induced muon and electron cascade events in a km scale under-ice detector at the South Pole, from the GRB 030329. Our calculations demonstrate that km scale neutrino telescopes are expected to detect signals that will allow us to constrain supernova-GRB models.
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U2 - 10.1103/PhysRevD.69.023001
DO - 10.1103/PhysRevD.69.023001
M3 - Article
AN - SCOPUS:1342325325
SN - 1550-7998
VL - 69
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 2
ER -