Pairing instabilities in neutrino plasmas arise only with occupation number discontinuities and are spurious artifacts of energy discretization that disappear in the continuum.
Title resolution pending
6 Pith papers cite this work. Polarity classification is still indexing.
6
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
roles
background 2polarities
background 2representative citing papers
A WKB ray-tracing framework shows that supernova matter gradients sweep flavomons through the unstable wavenumber range, strongly limiting slow-instability growth below the shock while leaving growth outside it largely intact.
In a neutrino-gas model, the many-body Hamiltonian yields different evolution timescales and asymptotics than the quantum kinetic approach with collisions, while quantum resources for the full case sit at the low end for HEP problems and mid-to-high for quantum chemistry.
Many-body neutrino calculations in simple momentum-state configurations yield helicity conversion probabilities orders of magnitude above mean-field results due to momentum exchange.
Small initial flavor perturbations in an inhomogeneous neutrino distribution exhibit chaotic divergence at small scales while domain-averaged density matrices stay stable.
Core collapse supernova models have demonstrated the neutrino shock reheating mechanism in three dimensions but require substantially more rigorous treatments of neutrino kinetics, fluid instabilities, magnetic fields, strong gravity, and nuclear physics to achieve quantitative predictive power.
citing papers explorer
-
Neutrino-antineutrino superfluidity
Pairing instabilities in neutrino plasmas arise only with occupation number discontinuities and are spurious artifacts of energy discretization that disappear in the continuum.
-
Flavomons in Matter Gradients: Ray Tracing and Amplitude Evolution
A WKB ray-tracing framework shows that supernova matter gradients sweep flavomons through the unstable wavenumber range, strongly limiting slow-instability growth below the shock while leaving growth outside it largely intact.
-
Collective neutrino oscillations: Many-body non-forward effects and non-classicality
In a neutrino-gas model, the many-body Hamiltonian yields different evolution timescales and asymptotics than the quantum kinetic approach with collisions, while quantum resources for the full case sit at the low end for HEP problems and mid-to-high for quantum chemistry.
-
Neutrino helicity oscillations in astrophysical environments: a many-body approach
Many-body neutrino calculations in simple momentum-state configurations yield helicity conversion probabilities orders of magnitude above mean-field results due to momentum exchange.
-
Chaos in Inhomogeneous Neutrino Fast Flavor Instability
Small initial flavor perturbations in an inhomogeneous neutrino distribution exhibit chaotic divergence at small scales while domain-averaged density matrices stay stable.
-
Core Collapse Supernova Modeling: The Next Ten Years
Core collapse supernova models have demonstrated the neutrino shock reheating mechanism in three dimensions but require substantially more rigorous treatments of neutrino kinetics, fluid instabilities, magnetic fields, strong gravity, and nuclear physics to achieve quantitative predictive power.