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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 2022 at "Physical Review D"
DOI: 10.1103/physrevd.107.103022
Abstract: Neutrino-neutrino forward scatterings potentially induce collective neutrino oscillation in dense neutrino gases in astrophysical sites such as core-collapse supernovae (CCSN) and binary neutron star mergers (BNSM). In this paper, we present a detailed study of…
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Keywords:
eln;
flavor;
flavor conversion;
asymptotic states ... 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