Abstract
Neutrinos play the critical roles in nucleosynthesis of light-to-heavy mass nuclei like 7Li, 11B, 138La and 180Ta in core-collapse supernovae. We find average neutrino temperatures of three flavor neutrinos so that the supernova nucleosynthesis models of the neutrino-process and the r-process can explain the observed solar-system abundance and Galactic chemical evolution of these isotopes. We propose a method to determine the unknown neutrino oscillation parameters θ 13 and mass hierarchy by the use of the MSW effects on the supernova nucleosynthesis.
Original language | English |
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Title of host publication | AIP Conference Proceedings |
Pages | 375-377 |
Number of pages | 3 |
Volume | 1441 |
DOIs | |
Publication status | Published - 2012 |
Externally published | Yes |
Event | 19th Particles and Nuclei International Conference, PANIC11 - Cambridge, MA Duration: 2011 Jul 24 → 2011 Jul 29 |
Other
Other | 19th Particles and Nuclei International Conference, PANIC11 |
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City | Cambridge, MA |
Period | 11/7/24 → 11/7/29 |
Keywords
- neutrino
- nucleosynthesis
- supernovae
ASJC Scopus subject areas
- Physics and Astronomy(all)