5 Result(s)
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Article
V. Sciacca
Physics
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Article
Open AccessDependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units
KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collaboration aims at identifying and ...
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Article
Open AccessIntrinsic limits on resolutions in muon- and electron-neutrino charged-current events in the KM3NeT/ORCA detector
Studying atmospheric neutrino oscillations in the few-GeV range with a multi-megaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA ...
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Article
Open AccessLong term monitoring of the optical background in the Capo Passero deep-sea site with the NEMO tower prototype
The NEMO Phase-2 tower is the first detector which was operated underwater for more than 1 year at the “record” depth of 3500 m. It was designed and built within the framework of the NEMO (NEutrino Mediterrane...
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Article
Open AccessThe prototype detection unit of the KM3NeT detector
A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80 km offshore the Italian coast. KM3NeT in its final configuration will contain several hundreds of detec...
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The Bi-Hamiltonian Theory of the Harry Dym Equation
We describe how the Harry Dym equation fits into the the bi-Hamiltonian formalism for the Korteweg–de Vries equation and other soliton equations. This is achieved using a certain Poisson pencil constructed fro...
