Proceedings of 40th International Conference on High Energy Physics — PoS(ICHEP2020) 2021
DOI: 10.22323/1.390.0149
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KM3NeT/ORCA: status and perspectives for neutrino oscillation and mass hierarchy measurements

Abstract: A next-generation neutrino telescope infrastructure, the Kilometer Cube Neutrino Telescope KM3NeT, is currently under construction in the Mediterranean Sea. Its low energy configuration ORCA is optimised for the detection of atmospheric neutrinos with energies above 1 GeV. The main goal of the ORCA detector is the precise measurement of atmospheric neutrino oscillation parameters and the determination of the neutrino mass ordering. The detector is also sensitive to a variety of other physics topics, such as da… Show more

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Cited by 5 publications
(4 citation statements)
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“…ANTARES has recorded additional data from 2017 to 2022, which represents a ∼50% increase with respect to that used in the present analysis and are currently being analysed. Furthermore, the next generation of neutrino telescopes in the Mediterranean Sea, KM3NeT-ORCA and -ARCA, now under deployment [71][72][73][74], are expected to further improve these limits. Open Access.…”
Section: Discussionmentioning
confidence: 99%
“…ANTARES has recorded additional data from 2017 to 2022, which represents a ∼50% increase with respect to that used in the present analysis and are currently being analysed. Furthermore, the next generation of neutrino telescopes in the Mediterranean Sea, KM3NeT-ORCA and -ARCA, now under deployment [71][72][73][74], are expected to further improve these limits. Open Access.…”
Section: Discussionmentioning
confidence: 99%
“…The bounds obtained with ANTARES are more restrictive than what is allowed by current experimental constraints. The next generation of neutrino telescopes in the Mediterranean Sea, KM3NeT-ORCA and -ARCA, now under deployment [65,66,67,68], are expected to further improve these limits.…”
Section: Discussionmentioning
confidence: 99%
“…Such a detector, like the planned ORCA, will efficiently detect the Cherenkov radiation emitted along the path of μ ± produced by the interactions of ν μ and νμ with the nucleons in the instrumented volume or near it. In addition, it will be posible to detect showers due to the e or τ produced by the associated neutrinos [54,67,68].…”
Section: Neutrino Events and Test Of Earth's Compositionmentioning
confidence: 99%