Abstract
We adopt the approach to the problem of neutrino oscillations in a magnetic field introduced in [1] and extended to the case of three neutrino generations in [2] to investigate the impact of ultrahighenergy neutrino oscillations in the interstellar magnetic field. Based on the assumption that UHE neutrinos flavour distribution follows the pattern 1:2:0, we have estimated the fluxes detected by a terrestrial neutrino telescope. We find out that the interaction with a magnetic field does not significantly modify the flavour distribution of UHE neutrinos unless they possess transition magnetic moments.
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