Results 81 to 90 of about 74,471 (120)
Supernova neutrinos detection in JUNO [PDF]
JUNO is the acronym for Jiangmen Underground Neutrino Observatory, an underground neutrino observatory located close to Kaiping city, South China. It will be the largest detector to use a liquid scintillator to detect neutrinos.
Lombardo, C.
core +1 more source
Skyrme-RPA study of charged-current neutrino opacity in hot and dense supernova matter
Neutrino emission and their transport of energy to the supernova shock region are sensitive to the physics of hot and dense nuclear matter, which is a complex problem due to the strong correlations induced by nuclear forces.
Dzhioev Alan A. +1 more
doaj +1 more source
Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
Neutrino-nucleus reactions cross sections, obtained for neutrino energies in the range εν ≤ 100–120 MeV (low- and intermediate-energy range), which refer to promising neutrino detection targets of current terrestrial neutrino experiments, are presented ...
J. Sinatkas +3 more
doaj +1 more source
Hunting Supernova neutrinos with dark matter detectors
During a massive star’s death, 99% of its energy is released in the form of neutrinos. Neutrinos of all flavors escape the core well before any light.
Kara, Melih
core
Shedding light on the Δm212 tension with supernova neutrinos
One long-standing tension in the determination of neutrino parameters is the mismatched value of the solar mass square difference, Δm212, measured by different experiments: the reactor antineutrino experiment KamLAND finds a best fit larger than the one ...
Rasmi Hajjar +2 more
doaj +1 more source
Neutral-Current Neutrino-Nucleus Scattering off Xe Isotopes
Large liquid xenon detectors aiming for dark matter direct detection will soon become viable tools also for investigating neutrino physics. Information on the effects of nuclear structure in neutrino-nucleus scattering can be important in distinguishing ...
P. Pirinen, J. Suhonen, E. Ydrefors
doaj +1 more source
We make a consistency test for the general relativity (GR) through measuring the growth index γ in a universe with massive (sterile/active) neutrinos. We employ the redshift space distortion measurements to do the analysis.
Ming-Ming Zhao +2 more
doaj +1 more source
Production of unstable heavy neutrinos in proto-neutron stars
We discuss the production of a class of heavy sterile neutrinos νh in proto-neutron stars. The neutrinos, of mass around 50 MeV, have a negligible mixing with the active species but relatively large dimension-5 electromagnetic couplings. In particular, a
C. Albertus +2 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Performance of SK-Gd’s Upgraded Real-time Supernova Monitoring System
Among multimessenger observations of the next Galactic core-collapse supernova, Super-Kamiokande (SK) plays a critical role in detecting the emitted supernova neutrinos, determining the direction to the supernova (SN), and notifying the astronomical ...
Y. Kashiwagi +239 more
doaj +1 more source

