Three flavor neutrino conversions in supernovae: slow & fast instabilities

DOI10.1088/1475-7516/2020/01/005zbMath1489.85003arXiv1909.10420OpenAlexW2974291498MaRDI QIDQ5067789

Madhurima Chakraborty, Sovan Chakraborty

Publication date: 4 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1909.10420

zbMATH Keywords

supernova neutrinosneutrino theorycore-collapse supernovas

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Oscillation, zeros of solutions, mean value theorems, etc. in context of PDEs (35B05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Weak interaction in quantum theory (81V15) Galactic and stellar dynamics (85A05) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Collective neutrino flavor conversion: recent developments
• Fast neutrino flavor conversion: collective motion vs. decoherence

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