Measuring the neutrino mass hierarchy with KM3NeT/ORCA

@article{Hofestadt2017MeasuringTN,
  title={Measuring the neutrino mass hierarchy with KM3NeT/ORCA},
  author={Jannik Hofestadt},
  journal={Journal of Physics: Conference Series},
  year={2017}
}
  • J. Hofestadt
  • Published 15 January 2017
  • Physics
  • Journal of Physics: Conference Series
ORCA (Oscillation Research with Cosmics in the Abyss) is the low-energy branch of KM3NeT, the next-generation research infrastructure hosting underwater Cherenkov detectors in the Mediterranean Sea. ORCA's primary goal is the determination of the neutrino mass hierarchy by measuring the matter-induced modifications on the oscillation probabilities of few-GeV atmospheric neutrinos. The ORCA detector design foresees a dense configuration of KM3NeT neutrino detection technology, optimised for… 
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References

SHOWING 1-10 OF 16 REFERENCES

KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss

KM3NeT, currently under construction in the abysses of the Mediterranean Sea, is a distributed research infrastructure that will host a km3-scale neutrino telescope (ARCA) for high-energy neutrino

Improving the neutrino mass hierarchy identification with inelasticity measurement in PINGU and ORCA

Multimegaton scale in under-ice and underwater detectors of atmospheric neutrinos with a few GeV energy threshold (PINGU, ORCA) open up new possibilities in the determination of neutrino properties,

Mass hierarchy, 2-3 mixing and CP-phase with huge atmospheric neutrino detectors

A bstractWe explore the physics potential of multi-megaton scale ice or water Cherenkov detectors with low (~ 1 GeV) threshold. Using some proposed characteristics of the PINGU detector setup we

Intrinsic limits on resolutions in muon- and electron-neutrino charged-current events in the KM3NeT/ORCA detector

A bstractStudying 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

Super-PINGU for measurement of the leptonic CP-phase with atmospheric neutrinos

A bstractWe explore a possibility to measure the CP-violating phase δ using multimegaton scale ice or water Cherenkov detectors with low, (0.2-1) GeV, energy threshold assuming that the neutrino mass

PINGU: A Vision for Neutrino and Particle Physics at the South Pole

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful

A Long Baseline Neutrino Oscillation Experiment Using J-PARC Neutrino Beam and Hyper-Kamiokande

Hyper-Kamiokande will be a next generation underground water Cherenkov detector with a total (fiducial) mass of 0.99 (0.56) million metric tons, approximately 20 (25) times larger than that of

Letter of intent for KM3NeT 2.0

The main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and (ii) the determination of the mass hierarchy of

Counting Electrons to Probe the Neutrino Mass Hierarchy

After the successful measurement of the mixing angle $\theta_{13}$, the determination of the neutrino mass hierarchy has become a priority for future neutrino experiments. We propose a conventional

The GENIE * Neutrino Monte Carlo Generator