Correlation Of Arrival Directions Of Neutrinos And Uhecrs: Pierre Auger Observatory And Antares Neutrino Telescope

Details Correlation Of Arrival Directions Of Neutrinos And Uhecrs: Pierre Auger Observatory And Antares Neutrino Telescope Correlation Of Arrival Directions Of Neutrinos And Uhecrs: Pierre Auger Observatory And Antares Neutrino Telescope

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.3209p&link_type=abstract

American Astronomical Society, HEAD meeting #11, #32.09; Bulletin of the American Astronomical Society, Vol. 41, p.704

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The origin of ultra-high energy cosmic rays (UHECRs) and neutrinos is still a mystery. Hadronic acceleration theory suggests that they should originate in the same sources (astrophysical or cosmological), together with gamma-rays. While gamma-rays have been linked to astrophysical sources, no point source of UHECRs or neutrinos has been found so far. We present a new multi-messenger approach in the search for point sources using high-energy particles: correlation between arrival directions of neutrinos and UHECRs, and its application to the neutrino telescope ANTARES and the Pierre Auger Observatory.

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