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arXiv · astro-ph/0609561

Production of high-energy μneutrinos from young neutron stars

G. F. Burgio·B. Link
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Abstract

Young, rapidly rotating neutron stars could accelerate protons to energies of $\sim 1$ PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the $Δ$ resonance and produce pions. The pions subsequently decay to produce muon neutrinos. We find that the energy spectrum of muon neutrinos consists of a sharp rise at $\sim 50$ TeV, corresponding to the onset of the resonance, above which the flux drops as $ε_ν^{-2}$ up to an upper-energy cut-off that is determined by either kinematics or by the maximum energy to which protons are accelerated. We predict event rates as high as 10-50 km$^{-2}$ yr$^{-1}$ from relatively young, close neutron stars. Such fluxes would be detectable by IceCube.

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G. F. Burgio, B. Link. 2006-09-20. Production of high-energy μneutrinos from young neutron stars. https://doi.org/10.1016/j.nuclphysbps.2006.11.030

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