Neutrino flavor conversion alters the lepton-emission self-sustained asymmetry in core-collapse supernovae

arXiv:2610.10685 · astro-ph.HE, hep-ph · Submitted 2026-10-07 · Read on arXiv

astro-ph.HE, hep-ph

Submitted: 2026-10-07

Updated: 2026-10-07

Terminology

• Decoupling — 34× in this paper · explained in 2 episodes
• Core — 29× in this paper · explained in 2 episodes
• Benchmark — 3× in this paper · explained in 2 episodes
• Symmetry Breaking — 2× in this paper · explained in 3 episodes
• Adam — 1× in this paper · explained in 2 episodes
• Anisotropy — 1× in this paper · explained in 3 episodes
• Boltzmann Equation — 1× in this paper · explained in 2 episodes
• Conservation Laws — 1× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Multi-messenger Astronomy — 1× in this paper · explained in 3 episodes

Sources

• Supernova Neutrinos: Production, Oscillations and Detection
• Neutrinos from core-collapse supernovae
• Neutrinos from explosive transients at the dawn of multi-messenger astronomy
• Long-Term Multidimensional Models of Core-Collapse Supernovae: Progress and Challenges
• Core-Collapse Supernova Explosion Theory
• Physical, numerical, and computational challenges of modeling neutrino transport in core-collapse supernovae
• New Developments in Flavor Evolution of a Dense Neutrino Gas
• Neutrinos from dense environments : Flavor mechanisms, theoretical approaches, observations, and new directions
• Neutrino Oscillations in Core-Collapse Supernovae and Neutron Star Mergers
• Collective Neutrino Oscillations
• Collective flavor conversion in dense neutrino plasmas
• Collisional flavor instabilities of supernova neutrinos
• Collisional instabilities of neutrinos and their interplay with fast flavor conversion in compact objects
• Self-induced neutrino flavor conversion without flavor mixing
• Collective neutrino flavor conversion: Recent developments
• Fast Pairwise Conversion of Supernova Neutrinos: A Dispersion-Relation Approach
• Neutrino-Mass-Driven Instabilities as the Earliest Flavor Conversion in Supernovae
• Dispersion relation of the neutrino plasma: Unifying fast, slow, and collisional instabilities
• Theory of neutrino fast flavor evolution. Part II. Solutions at the edge of instability
• Neutrino Fast Flavor Pendulum. Part 2: Collisional Damping

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