Results 31 to 40 of about 23,101 (234)
Theia: an advanced optical neutrino detector
European Physical Journal C: Particles and Fields, 2020 New developments in liquid scintillators, high-efficiency, fast photon detectors, and chromatic photon sorting have opened up the possibility for building a large-scale detector that can discriminate between Cherenkov and scintillation signals.
M. Askins +80 more
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The Astrophysical Journal Letters, 2023 We report the first search result for the flux of astrophysical electron antineutrinos for energies ${ \mathcal O }(10)\,\mathrm{MeV}$ in the gadolinium-loaded Super-Kamiokande (SK) detector. In 2020 June, gadolinium was introduced to the ultrapure water
M. Harada +242 more
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Prospects for Extending the Core-collapse Supernova Detection Horizon Using High-energy Neutrinos
The Astrophysical Journal, 2023 Large neutrino detectors like IceCube monitor for core-collapse supernovae using low-energy (MeV) neutrinos with a detection reach from a supernova neutrino burst to the Magellanic Cloud. However, some models predict the emission of high-energy neutrinos
Nora Valtonen-Mattila, Erin O’Sullivan
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Searching for high-energy neutrinos from the most luminous supernovae with the IceCube Neutrino Observatory [PDF]
EPJ Web of Conferences, 2023 The sources of the astrophysical neutrino flux discovered by IceCube remain for the most part unresolved. Extragalactic core-collapse supernovae (CCSNe) have been suggested as potentially able to produce high-energy neutrinos.
Lincetto Massimiliano
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Superluminal neutrinos in long baseline experiments and SN1987a [PDF]
, 2011 Precise tests of Lorentz invariance in neutrinos can be performed using long baseline experiments such as MINOS and OPERA or neutrinos from astrophysical sources. The MINOS collaboration reported a measurement of the muonic neutrino velocities that hints
A Delgado +27 more
core +4 more sources
Advances in Astronomy, 2012 Core-collapse supernovae are dramatic explosions marking the catastrophic end of massive stars. The only means to get direct information about the supernova engine is from observations of neutrinos emitted by the forming neutron star, and through ...
Kei Kotake +6 more
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Neutrino Physics and Astrophysics with the JUNO Detector
Universe, 2018 The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator multi-purpose underground detector, under construction near the Chinese city of Jiangmen, with data collection expected to start in 2021.
Lino Miramonti
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SciPost Physics Proceedings, 2023 The upcoming Hyper-Kamiokande (HyperK) experiment is expected to detect the Diffuse Supernova Neutrino Background (DSNB). This requires to ponder all possible sources of background.
Sandra Robles
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Resonant neutrino spin-flavor precession and supernova shock revival [PDF]
, 1996 A new mechanism of supernova shock revival is proposed, which involves resonant spin--flavor precession of neutrinos with a transition magnetic moment in the magnetic field of the supernova.
A. Burrows +52 more
core +4 more sources
MEASURING NEUTRINO MASSES WITH SUPERNOVA NEUTRINOS [PDF]
The Tenth Marcel Grossmann Meeting, 2006 3 pages; contribution to the proceedings of X Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July ...
openaire +2 more sources