Neutrinos of energy similar to 10(16) eV from gamma-ray bursts in pulsar wind bubbles

D Guetta; J Granot

doi:10.1103/PhysRevLett.90.201103

Neutrinos of energy similar to 10(16) eV from gamma-ray bursts in pulsar wind bubbles

D Guetta, J Granot

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

The supranova model for [Formula presented]-ray bursts (GRBs) is becoming increasingly more popular. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). Protons accelerated in the internal shocks that emit the GRB may interact with the external PWB photons producing pions which decay into [Formula presented] neutrinos. A [Formula presented] neutrino detector would observe several events per year correlated with the GRBs.

Original language	English
Pages (from-to)	4
Number of pages	1
Journal	Physical Review Letters
Volume	90
Issue number	20
DOIs	https://doi.org/10.1103/PhysRevLett.90.201103
State	Published - 23 May 2003
Externally published	Yes

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10.1103/PhysRevLett.90.201103

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abstract = "The supranova model for [Formula presented]-ray bursts (GRBs) is becoming increasingly more popular. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). Protons accelerated in the internal shocks that emit the GRB may interact with the external PWB photons producing pions which decay into [Formula presented] neutrinos. A [Formula presented] neutrino detector would observe several events per year correlated with the GRBs.",

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Neutrinos of energy similar to 10(16) eV from gamma-ray bursts in pulsar wind bubbles

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