Neutrino flux predictions for galactic plerions

D Guetta; E Amato

doi:10.1016/S0927-6505(02)00221-9

Neutrino flux predictions for galactic plerions

D Guetta, E Amato

Department of Physics

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

25 Scopus citations

Abstract

We consider a class of plerions that have been detected in the TeV range, and investigate the possibility that the emission is due to π⁰ decay. From the TeV flux we derive what is the expected ν flux at Earth and find that this is likely to exceed the detection threshold of the upcoming km² neutrino detectors.

Original language	English
Pages (from-to)	403-407
Number of pages	5
Journal	Astroparticle Physics
Volume	19
Issue number	3
DOIs	https://doi.org/10.1016/S0927-6505(02)00221-9
State	Published - Jun 2003

Keywords

high energy photons
neutrinos
supernova remnants

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10.1016/S0927-6505(02)00221-9

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abstract = "We consider a class of plerions that have been detected in the TeV range, and investigate the possibility that the emission is due to π0 decay. From the TeV flux we derive what is the expected ν flux at Earth and find that this is likely to exceed the detection threshold of the upcoming km2 neutrino detectors.",

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Neutrino flux predictions for galactic plerions

Abstract

Keywords

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