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Neutrinos propagating in a dense neutrino gas, such as those expected in core-collapse supernovae (CCSNe) and neutron star mergers (NSMs), can experience fast flavor conversions on relatively short scales.
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O. Just, S. Abbar, M.-R. Wu, I. Tamborra, H.-T. Janka, F. Capozzi, Fast neutrino conversion in hydrodynamic simulations of neutrino-cooled accretion disks, Phys. Rev. D105 (8) (2022) 083024 · 2022
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M. C. Volpe, Neutrinos from dense: flavor mechanisms, theoretical approaches, observations, new directions (1 2023) · 2023
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J. Ehring, S. Abbar, H.-T. Janka, G. Raffelt, Fast Neutrino Flavor Conversion in Core-Collapse Supernovae: A Parametric Study in 1D Models (1 2023) · 2023
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B. T. H. Tsang, D. Vartanyan, A. Burrows, Applications of Machine Learning to Predicting Core-collapse Supernova Explosion Outcomes, Astrophys. J. Lett. 937 (1) (2022) L15 · 2041
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