期刊
PHYSICAL REVIEW D
卷 87, 期 8, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.87.085037
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资金
- NSF at UCSD [PHY-09-70064]
- DOE at UNM Albuquerque [DE-SC0008142]
- DOE Office of Science
- LDRD Program
- LANL
- UC office of the President
- U.S. Department of Energy (DOE) [DE-SC0008142] Funding Source: U.S. Department of Energy (DOE)
- Direct For Mathematical & Physical Scien
- Division Of Physics [0970064] Funding Source: National Science Foundation
We give the first self-consistent calculation of the effect of the scattered neutrino halo on flavor evolution in supernovae. Our example case is an O-Ne-Mg core collapse supernova neutronization neutrino burst. We find that the addition of the halo neutrinos produces qualitative and quantitative changes in the final flavor states of neutrinos. We also find that the halo neutrinos produce a novel distortion of the neutrino flavor swap. Our results provide strong motivation for tackling the full multidimensional and composition-dependent aspects of this problem in the future. DOI: 10.1103/PhysRevD.87.085037
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