High energy neutrino emission from young
โ
G.F. Burgio; B. Link
๐
Article
๐
2006
๐
Elsevier Science
๐
English
โ 119 KB
We propose that young (t age t10 5 yr), rapidly rotating pulsars can accelerate ions to energies of $1 PeV near the surface of a neutron star. Protons undergo resonant excitation with surface X-rays and produce a beam of m neutrinos with energies of several tens of TeV which could be detectable by c