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 |
|---|---|
| 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 |
|---|---|
| City | Cambridge, MA |
| Period | 11/7/24 → 11/7/29 |
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Keywords
- neutrino
- nucleosynthesis
- supernovae
ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
Supernova nucleosynthesis and neutrino oscillation. / Kajino, T.; Aoki, W.; Cheoun, M. K.; Chiba, S.; Fujiya, W.; Hayakawa, T.; Mathews, G. J.; Nakamura, K.; Shaku, K.; Yoshida, T.
AIP Conference Proceedings. Vol. 1441 2012. p. 375-377.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - Supernova nucleosynthesis and neutrino oscillation
AU - Kajino, T.
AU - Aoki, W.
AU - Cheoun, M. K.
AU - Chiba, S.
AU - Fujiya, W.
AU - Hayakawa, T.
AU - Mathews, G. J.
AU - Nakamura, K.
AU - Shaku, K.
AU - Yoshida, T.
PY - 2012
Y1 - 2012
N2 - 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.
AB - 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.
KW - neutrino
KW - nucleosynthesis
KW - supernovae
UR - http://www.scopus.com/inward/record.url?scp=84860641971&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84860641971&partnerID=8YFLogxK
U2 - 10.1063/1.3700559
DO - 10.1063/1.3700559
M3 - Conference contribution
AN - SCOPUS:84860641971
SN - 9780735410367
VL - 1441
SP - 375
EP - 377
BT - AIP Conference Proceedings
ER -