High energy neutrino emission from young pulsars

Details High energy neutrino emission from young pulsars High energy neutrino emission from young pulsars

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nimpa.567..486b&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, Volume 567, Issue 2, p. 486-488.

Physics

Scientific paper

We propose that young (t≲10yr), rapidly rotating pulsars can accelerate ions to energies of ˜1PeV near the surface of a neutron star. Protons undergo resonant excitation with surface X-rays and produce a beam of μ neutrinos with energies of several tens of TeV which could be detectable by current technology. Detection of these neutrinos would further our understanding of high-energy processes that take place in the stellar magnetosphere.

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