Symmetry breaking induced by pairwise conversion of neutrinos in compact sources
arXiv:2106.15622 · doi:10.1103/PhysRevD.105.043018
Abstract
A surprising consequence of non-linear flavor evolution is the spontaneous breaking of the initial symmetries of the neutrino gas propagating in a dense astrophysical environment. We explore the flavor conversion physics by taking into account the polar and azimuthal angular distributions of neutrinos and present the very first example of spontaneous symmetry breaking in the context of fast flavor mixing in the nonlinear regime. Intriguingly, we find that fast flavor mixing does not always develop in the proximity of the angular regions with vanishing electron lepton number, as commonly assumed, and large flavor mixing can rapidly spread through all neutrino modes. Such behavior cannot be predicted from the linear regime of the flavor evolution. These results can have major consequences on the physics of compact astrophysical objects.
9 pages, 6 figures, revtex4-1 two column format. Version accepted in Phys. Rev. D. Supplmental material: https://sid.erda.dk/share_redirect/hwp0WKuuk7/index.html
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- Dynamics of fast neutrino flavor conversions with scattering effects: a detailed analysis
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- Neutrino Flavor Conversion, Advection, and Collisions: Towards the Full Solution
- Neutrino Decoupling Is Altered by Flavor Conversion
- Fast Flavor Transformations
- Flavor conversions with energy-dependent neutrino emission and absorption
- Neutrino quantum kinetics in two spatial dimensions
- Quantum Closures for Neutrino Moment Transport
- Symmetry breaking due to multi-angle matter-neutrino resonance in neutron star merger remnants
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