Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

Jonathan Granot; Dafne Guetta

doi:10.1103/PhysRevLett.90.191102

Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

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

Abstract

The supranova model for [Formula presented]-ray bursts (GRBs) has recently gained popularity. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). High energy protons from the PWB can interact with photons from the rich radiation field inside the PWB or collide with cold protons from the supernova remnant, producing pions which decay into [Formula presented] neutrinos. The predicted neutrino flux from the PWBs that host the GRBs should be easily detectable by planned [Formula presented] detectors.

Original language	English
Pages (from-to)	191102/1-191102/4
Number of pages	1
Journal	Physical Review Letters
Volume	90
Issue number	19
DOIs	https://doi.org/10.1103/PhysRevLett.90.191102
State	Published - 16 May 2003
Externally published	Yes

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10.1103/PhysRevLett.90.191102

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abstract = "The supranova model for [Formula presented]-ray bursts (GRBs) has recently gained popularity. In this scenario the GRB occurs weeks to years after a supernova explosion, and is located inside a pulsar wind bubble (PWB). High energy protons from the PWB can interact with photons from the rich radiation field inside the PWB or collide with cold protons from the supernova remnant, producing pions which decay into [Formula presented] neutrinos. The predicted neutrino flux from the PWBs that host the GRBs should be easily detectable by planned [Formula presented] detectors.",

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Neutrinos from pulsar wind bubbles as precursors to gamma-ray bursts

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