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The observed excess of high-energy cosmic rays from the Galactic plane in theenergy range \sim 10^18 eV may be naturally explained by neutron primariesgenerated in the photo-dissociation of heavy nuclei. In this scenario, neutronswith lower energy decay before reaching the Earth and produce a detectable fluxin a 1 km^3 neutrino telescope. The initial flavor composition of theseneutrinos, \phi(\bar\nu_e):\phi(\bar\nu_\mu):\phi(\bar\nu_\tau)=1:0:0, offersthe opportunity to perform a combined \bar\nu_\mu/\bar\nu_\tau appearance and\bar\nu_e disappearance experiment. The observable ratio\phi(\bar\nu_\mu)/\phi(\bar\nu_e+\bar\nu_\tau) of fluxes arriving on Earthdepends appreciably on the 13-mixing angle \theta_13 and the leptonic CP phase\delta_CP, opening thus a new experimental avenue to measure these twoquantities.Comment: 4 pages, 2 eps figures. Enlarged discussion, references added.  Matches version to appear in PR

physical review letters

Measuring the 13 Neutrino Mixing Angle and the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>C</mml:mi><mml:mi>P</mml:mi></mml:math>Phase with Neutrino Telescopes

Measuring the 13 Neutrino Mixing Angle and theCPPhase with Neutrino Telescopes