High energy neutrinos from a slow jet model of core collapse supernovae

Details High energy neutrinos from a slow jet model of core collapse supernovae High energy neutrinos from a slow jet model of core collapse supernovae

2005-09-23

arxiv.org/abs/astro-ph/0509729v1

Mod.Phys.Lett. A20 (2005) 2351-2368

Astronomy and Astrophysics

Astrophysics

17 pages, 5 figures, invited brief review

Scientific paper

10.1142/S0217732305018414

It has been hypothesized recently that core collapse supernovae are triggered by mildly relativistic jets following observations of radio properties of these explosions. Association of a jet, similar to a gamma-ray burst jet but only slower, allows shock acceleration of particles to high energy and non-thermal neutrino emission from a supernova. Detection of these high energy neutrinos in upcoming kilometer scale Cherenkov detectors may be the only direct way to probe inside these astrophysical phenomena as electromagnetic radiation is thermal and contains little information. Calculation of high energy neutrino signal from a simple and slow jet model buried inside the pre-supernova star is reviewed here. The detection prospect of these neutrinos in water or ice detector is also discussed in this brief review. Jetted core collapse supernovae in nearby galaxies may provide the strongest high energy neutrino signal from point sources.

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