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   <subfield code="a">Oscillations of atmospheric neutrinos with a large neutrino telescope</subfield>
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   <subfield code="c">[M. Laveder]</subfield>
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   <subfield code="a">Summary: The sensitivity of a large water Čerenkov neutrino telescope in detecting possible oscillations (v μ→v τ) and (v μ→v e) of atmospheric neutrinos is studied, taking also into account the Wolfenstein, Mikheyev and Smirnov matter effects. The large water Čerenkov device is able to detect with high accuracy upward-going muons with energies greater than 10 GeV. After one year running time the search for ν oscillations will reach the following sensitivity for the oscillation parameters: Δm 2&gt;3·10−3 (eV2), for sin22θ=1, sin22θ&gt;4·10−2, for Δm 2&gt;0.1 (eV2) for the oscillation (v μ→v τ) and δm 2&gt;4·10−3 (eV2), for sin22θ=1, sin22θ&gt;8·10−3, for δm 2=6·10−2 (eV2) for the oscillation (v μ→v e). These limits are well below the current accelerator and reactor limits. It is also stressed the importance of such a measurement in the context of solar ν puzzle.</subfield>
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