Revealing the supernova-gamma-ray burst connection with TeV neutrinos - INSPIRE

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Revealing the supernova-gamma-ray burst connection with TeV neutrinos

Shin'ichiro Ando
(
- Tokyo U. and
- Ohio State U.
)
,
John F. Beacom
(
- Ohio State U. and
- Ohio State U., Dept. Astron.
)

Feb, 2005

4 pages

Published in:

Phys.Rev.Lett. 95 (2005) 061103

e-Print:

astro-ph/0502521 [astro-ph]

DOI:

10.1103/PhysRevLett.95.061103

Report number:

UTAP-514

View in:

ADS Abstract Service

reference search210 citations

Citations per year

Abstract: (arXiv)

Gamma-ray bursts (GRBs) are rare but powerful explosions displaying highly relativistic jets. It has been suggested that a significant fraction of the much more frequent core-collapse supernovae are accompanied by comparably energetic but mildly relativistic jets, which would indicate an underlying supernova--GRB connection. We calculate the neutrino spectra from the decays of pions and kaons produced in jets in supernovae, and show that the kaon contribution is dominant and provides a sharp break near 20 TeV, which is a sensitive probe of the conditions inside the jet. For a supernova at 10 Mpc, 30 events above 100 GeV are expected in a 10 s burst in the IceCube detector.

98.70.Rz
96.40.Tv
98.70.Sa
97.60.Bw
supernovae
stellar radiation
galactic cosmic rays
cosmic ray neutrinos
astrophysical jets
gamma-ray bursts

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Figures(0)

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