Searching for soft relativistic jets in core-collapse supernovae with the IceCube optical follow-up program
Context. Transient neutrino sources such as gamma-ray bursts (GRBs) and supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of ≲ 100 s. While GRB neutrinos would be produced in high relativistic jets, core-collapse
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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