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

Soebur Razzaque; Peter Meszaros; Eli Waxman

doi:10.1142/s0217732305018414

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

Soebur Razzaque·Peter Meszaros·Eli Waxman

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Abstract

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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Soebur Razzaque, Peter Meszaros, Eli Waxman. 2005-09-23. High energy neutrinos from a slow jet model of core collapse supernovae. https://doi.org/10.1142/s0217732305018414

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