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TeV neutrinos from core collapse supernovae and hypernovae
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A fraction of core collapse supernovae of type Ib/c are associated with Gamma-ray bursts, which are thought to produce highly relativistic jets. Recently, it has been hypothesized that a larger fraction of core collapse supernovae produce slower jets, which may contribute to the disruption and ejection of the supernova envelope, and explain the unusually energetic hypernovae. We explore the TeV neutrino signatures expected from such slower jets, and calculate the expected detection rates with upcoming Gigaton Cherenkov experiments. We conclude that individual jetted SNe may be detectable from nearby galaxies.
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Cited by 2 Pith papers
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Gamma-ray emission from decays of boosted nuclei in protomagnetar jets
Doppler-boosted, time-dilated radioactive decay lines from nuclei in protomagnetar jets could be detected by INTEGRAL/SPI and e-ASTROGAM from a supernova at 10 kpc.
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Particle Astrophysics with High and Ultrahigh Energy Neutrinos
Recent high and ultrahigh energy neutrino detections open a new observational window to the universe by revealing sources and processes inaccessible via photons.
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