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- W1558647588 abstract "We present a decisive test to probe the young pulsar origin of ultrahigh energy cosmic rays (UHECRs) within the next decade, with the IceCube neutrino detector. Pulsars, especially for those spinning close to millisecond periods at birth, are good candidate sources for the production of UHECRs. We demonstrated that it is possible with the extragalactic pulsar population to explain the measurements of the Auger Observatory consistently. Here we calculate the diffusive neutrino flux, produced inevitably while particles cross the supernova ejecta, associated with this pulsar scenario. We predict that the pulsar population should produce a diffusive neutrino flux that lies considerably above the IceCube-5 years sensitivity in the 10^18 eV energy range, and is below the current IceCube sensitivity. Even in the most pessimistic case, one expects a minimum flux of neutrinos, detectable with IceCube within a decade. This conclusion stands for any pulsar scenario that explains the UHECR data, regardless of the uncertainties on UHECR production." @default.
- W1558647588 created "2016-06-24" @default.
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- W1558647588 date "2013-11-08" @default.
- W1558647588 modified "2023-09-27" @default.
- W1558647588 title "A decisive test for the young pulsar origin of ultrahigh energy cosmic rays with IceCube" @default.
- W1558647588 hasPublicationYear "2013" @default.
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