High energy neutrino emission from young pulsars
โ Scribed by G.F. Burgio; B. Link
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 119 KB
- Volume
- 567
- Category
- Article
- ISSN
- 0168-9002
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โฆ Synopsis
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 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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