Results 21 to 30 of about 77,742 (251)

Double neutrino production and detection in neutrino detectors [PDF]

open access: yesPhysical Review D, 2013
Large, high-energy ($E>100$ GeV) cosmic neutrino telescopes are now quite mature. IceCube, for example, observes about 50,000 well-reconstructed single atmospheric neutrino events/year, with energies above 100 GeV. Although the neutrino detection probability is small, current detectors are large enough so that it is possible to detect two neutrinos ...
van der Drift, Don, Klein, Spencer R.
openaire   +2 more sources

Probing invisible neutrino decay with KM3NeT/ORCA

open access: yesJournal of High Energy Physics, 2023
In the era of precision measurements of the neutrino oscillation parameters, upcoming neutrino experiments will also be sensitive to physics beyond the Standard Model.
The KM3NeT collaboration   +254 more
doaj   +1 more source

The IceCube Neutrino Observatory: Instrumentation and Online Systems [PDF]

open access: yes, 2016
The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detector built to date, was completed in 2011 and enabled the discovery of high ...
Aartsen, M. G.   +352 more
core   +3 more sources

Cascade sensitivity studies for KM3NeT

open access: yesEPJ Web of Conferences, 2016
KM3NeT is a future research infrastructure in the deep seas of the Mediterranean housing a large scale neutrino telescope. The first phase of construction of the telescope has started.
Fusco Luigi Antonio
doaj   +1 more source

Design and first tests of the S3 detector of reactor antineutrinos [PDF]

open access: yesEPJ Web of Conferences, 2021
The new experiment S3 devoted to the study of reactor antineutrinos was designed and constructed as a common activity of IEAP CTU in Prague and JINR (Dubna). The S3 detector is a compact, highly segmented polystyrene-based scintillating detector composed
Slavíčková Mária   +20 more
doaj   +1 more source

The ICARUS experiment

open access: yesEPJ Web of Conferences, 2018
The 760 ton liquid argon ICARUS T600 detector performed a successful threeyear physics run at the underground LNGS laboratories, studying neutrino oscillations with the CNGS neutrino beam and searching for atmospheric neutrino interactions in cosmic rays.
Farnese Christian
doaj   +1 more source

Neutrino Interferometry In Curved Spacetime [PDF]

open access: yes, 2004
Gravitational lensing introduces the possibility of multiple (macroscopic) paths from an astrophysical neutrino source to a detector. Such a multiplicity of paths can allow for quantum mechanical interference to take place that is qualitatively different
A. Gould   +61 more
core   +2 more sources

A relic neutrino detector [PDF]

open access: yesSecond international workshop on particle physics and the early universe (COSMO-98), 1999
Probably the most promising way of detecting cosmic neutrinos is measuring the mechanical force exerted by elastic scattering of cosmic neutrinos from macroscopic targets. The expected acceleration is $\sim 10^{-23} cm/s^2$ for Dirac neutrinos of mass $\sim 10 eV$ and local density $\sim 10^7/ cm^3$. A novel torsion balance design is presented.
openaire   +2 more sources

Neutrino trident scattering at near detectors [PDF]

open access: yesJournal of High Energy Physics, 2019
Abstract Neutrino trident scattering is a rare Standard Model process where a charged-lepton pair is produced in neutrino-nucleus scattering. To date, only the dimuon final-state has been observed, with around 100 total events, while the other channels are as yet unexplored.
Peter Ballett   +5 more
openaire   +6 more sources

Future neutrino physics with Hyper-Kamiokande [PDF]

open access: yesEPJ Web of Conferences
Hyper-Kamiokande, the next-generation neutrino observatory in Japan, evolves from its predecessors, Kamiokande, Super-Kamiokande and T2K, with a significant upgrade to a 258-kton water Cherenkov detector equipped with 20,000 PMTs.
Jesús-Valls César
doaj   +1 more source

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