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Published in 2021 at "General Relativity and Gravitation"
DOI: 10.1007/s10714-021-02872-6
Abstract: We study the effect of gravity on neutrino flavor oscillations when each mass eigenstate is described by a wave packet instead of a plane wave. Two different approaches for implementing the wave packet formalism in…
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Keywords:
flavor oscillations;
neutrino flavor;
wave packet;
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Published in 2021 at "Physical Review D"
DOI: 10.1103/physrevd.103.083014
Abstract: In an environment with high-density neutrinos formed in a core-collapse supernova (CCSN), the neutrinos exhibit nonlinear and complex oscillation behaviors due to their self-interactions. The onset of this nonlinear oscillation can be investigated by linearizing…
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Keywords:
flavor;
flavor conversion;
dimensional spacetime;
neutrino flavor ... See more keywords
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Published in 2023 at "Physical Review D"
DOI: 10.1103/physrevd.107.103034
Abstract: We explore the impact of small-scale flavor conversions of neutrinos, the so-called fast flavor conversions (FFCs), on the dynamical evolution and neutrino emission of core-collapse supernovae (CCSNe). In order to do that, we implement FFCs…
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Keywords:
collapse supernovae;
core collapse;
neutrino flavor;
flavor ... See more keywords
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Published in 2017 at "Physical Review D"
DOI: 10.1103/physrevd.96.083008
Abstract: Author(s): Armstrong, Eve; Patwardhan, Amol V; Johns, Lucas; Kishimoto, Chad T; Abarbanel, Henry DI; Fuller, George M
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Keywords:
approach calculating;
optimization based;
based approach;
neutrino flavor ... See more keywords
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Published in 2022 at "Physical review letters"
DOI: 10.1103/physrevlett.129.261101
Abstract: Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs iin core-collapse supernovae and binary neutron star mergers, the lack of global simulations has been the greatest obstacle to study their astrophysical consequences. In…
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Keywords:
fast neutrino;
flavor conversion;
neutrino flavor;
time dependent ... See more keywords
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Published in 2023 at "Physical Review Letters"
DOI: 10.1103/physrevlett.130.211401
Abstract: One of the greatest uncertainties in any modeling of inner engine of core-collapse supernova (CCSN) is neutrino flavor conversions driven by neutrino self-interactions. We carry out large-scale numerical simulations of multi-energy, multi-angle, three-flavor framework, and…
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Keywords:
core collapse;
neutrino flavor;
neutrino heating;
collapse supernova ... See more keywords