11B and Constraints on Neutrino Oscillations and Spectra from Neutrino Nucleosynthesis
arXiv:1102.4858 · doi:10.1103/PhysRevLett.106.152501
Abstract
We have studied the sensitivity to variations in the triple alpha and 12C(alpha, gamma)16O reaction rates, of the yield of the neutrino process isotopes 7Li,11B, 19F, 138La, and 180Ta in core collapse supernovae. Compared to solar abundances, less than 15% of 7Li, about 25-80% of 19F, and about half of 138La is produced in these stars. Over a range of two sigma for each helium-burning rate, 11B is overproduced and the yield varies by an amount larger than the variation caused by the effects of neutrino oscillations. The total 11B yield, however, may eventually provide constraints on supernova neutrino spectra.
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- Reconstruction of supernova ν_μ, ν_τ, anti-ν_μ, and anti-ν_τ neutrino spectra at scintillator detectors
- The -process with fully time-dependent supernova neutrino emission spectra
- The Impact of Helium-Burning Reaction Rates on Massive Star Evolution and Nucleosynthesis
- Exploring the Neutrino Mass Hierarchy Probability with Meteoritic Supernova Material, ν-Process Nucleosynthesis, and θ13 Mixing
- Supernova Neutrino Process of Li and B Revisited
- The Role of the Hadron-Quark Phase Transition in Core-Collapse Supernovae
- Neutrino self-interaction and MSW effects on the supernova neutrino-process
- Astrophysical S factor of {C()O} Calculated with the Reduced R-matrix Theory
- Comprehensive Analyses of the Neutrino-Process in the Core-collapsing Supernova
- Effective Helium Burning Rates and the Production of the Neutrino Nuclei
- New Primary Mechanisms for the Synthesis of Rare 9Be in Early Supernovae
- Neutrinos and Heavy Element Nucleosynthesis