Normal and inverted neutrino mass orderings tend to occupy different regions in ternary space when supernova neutrino flavor compositions are plotted across several models.
Potential to identify the neutrino mass ordering with reactor antineutrinos in juno
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 3verdicts
UNVERDICTED 3roles
background 1polarities
support 1representative citing papers
Future MeV telescopes could constrain axion-photon couplings to 1.61 × 10^{-13} GeV^{-1} for ALP masses below 10^{-9} eV using signals from galactic supernovae.
Inelasticity and neutron multiplicity distributions differ between neutrino and antineutrino charged-current events in liquid scintillator, enabling quantitative discrimination for atmospheric oscillation studies.
citing papers explorer
-
Investigating the Neutrino Mass Ordering Problem via Ternary Plots
Normal and inverted neutrino mass orderings tend to occupy different regions in ternary space when supernova neutrino flavor compositions are plotted across several models.
-
Unveiling axion signals in galactic supernovae with future MeV telescopes
Future MeV telescopes could constrain axion-photon couplings to 1.61 × 10^{-13} GeV^{-1} for ALP masses below 10^{-9} eV using signals from galactic supernovae.
-
Atmospheric Neutrino Charged-Current Interactions at Large Liquid-Scintillator Detectors: I. Physics of Neutrino-Antineutrino Discrimination
Inelasticity and neutron multiplicity distributions differ between neutrino and antineutrino charged-current events in liquid scintillator, enabling quantitative discrimination for atmospheric oscillation studies.