A Crab-like synthetic population of young pulsar wind nebulae can contribute roughly 5% of the IceCube Galactic neutrino flux near 100 TeV in an optimistic hadronic-proton model.
A., Ansoldi, S., Antonelli, L
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Potential Contribution of Young Pulsar Wind Nebulae to Galactic High-Energy Neutrino Emission
A Crab-like synthetic population of young pulsar wind nebulae can contribute roughly 5% of the IceCube Galactic neutrino flux near 100 TeV in an optimistic hadronic-proton model.