Machine Learning Detection of Non-Axisymmetric Fast Flavor Instabilities in Compact Objects
Madhurima Chakraborty, Sajad Abbar, Meng-Ru Wu, Francois Foucart, Zewei Xiong
astro-ph.HE, hep-ph
Submitted: 2026-07-14
Comments: 14 pages, 2 figures, 7 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Core-Collapse Supernova Explosion Theory
- Explosion Mechanisms of Core-Collapse Supernovae
- Core Collapse Supernova Modeling: The Next Ten Years
- Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling
- Merger and Mass Ejection of Neutron-Star Binaries
- The Dynamics of Binary Neutron Star Mergers and of GW170817
- Neutrino transport in general relativistic neutron star merger simulations
- Neutrinos and nucleosynthesis of elements
- Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background
- Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment I: Correlated Neutrino Trajectories
- Coherent Development of Neutrino Flavor in the Supernova Environment
- Collective Neutrino Oscillations
- Supernova Neutrinos: Production, Oscillations and Detection
- Neutrinos from dense environments : Flavor mechanisms, theoretical approaches, observations, and new directions
- Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers
- Speed-up of neutrino transformations in a supernova environment
- Neutrino cloud instabilities just above the neutrino sphere of a supernova
- Self-induced neutrino flavor conversion without flavor mixing
- Three flavor neutrino conversions in supernovae: Slow $\&$ Fast instabilities
- Fast flavor conversions in supernovae: the rise of mu-tau neutrinos
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