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TeV Neutrinos from Successful and Choked Gamma-Ray Bursts

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Mészáros, Peter, Waxman, Eli·2001·Physical Review Letters

Abstract

Core collapse of massive stars resulting in a relativistic fireball jet which breaks through the stellar envelope is a widely discussed scenario for gamma-ray burst production. For very extended or slow rotating stars, the jet may be unable to break through the envelope. Both penetrating and choked jets will produce, by photomeson interactions of accelerated protons, a burst of greater, greater than or similar to 5 TeV neutrinos while propagating in the envelope. The predicted flux, from both penetrating and choked jets, should be easily detectable by planned 1 km(3) neutrino telescopes.

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Metadata

Authors
Mészáros, P., & Waxman, E.
Venue
Physical Review Letters
Published
2001-10-04
Volume
87
Issue
17
Pages
171102-171102
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2051627582
Cited by
293
References
0
FWCI
7.53
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: TeV Neutrinos from Successful and Choked Gamma-Ray Bursts. https://app.cochat.ai/papers/10.1103/physrevlett.87.171102
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Mészáros, P., & Waxman, E. (2001). TeV Neutrinos from Successful and Choked Gamma-Ray Bursts. Physical Review Letters. https://doi.org/10.1103/physrevlett.87.171102

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