Research output per year
Research output per year
Xiao Dong Tang, B. Bucher, Xiao Fang, A. Heger, S. Almaraz-Calderon, A. Alongi, A. D. Ayangeakaa, M. Beard, Andreas Best, J. Browne, C. Cahillane, M. Couder, R. J. DeBoer, A. Kontos, L. Lamm, Yunju Li, Alexander Makenzie Long, Wenting Lu, Shawn M Lyons, M. Notani
Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Other › peer-review
Neutrons produced by the carbon fusion reaction 12C(12C,n)23Mg play an important role in stellar nucleosynthesis. Past studies have shown large discrepancies between experimental data and theory, leading to an uncertain cross section extrapolation at astrophysical energies. We present the first direct measurement which extends deep into the astrophysical energy range along with a new and improved extrapolation technique based on experimental data from the mirror reaction 12C(12C,p)23Na. The new reaction rate has been determined with a well-defined uncertainty which exceeds the precision required by astrophysics models. Using our constrained rate, we find that 12C(12C,n)23Mg is crucial to the production of Na and Al in Pop-III Pair Instability Supernovae.
Original language | English |
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Title of host publication | EPJ Web of Conferences |
Number of pages | 6 |
Volume | 109 |
DOIs | |
Publication status | Published - 12 Feb 2016 |
Event | International Symposium on Origin of Matter and Evolution of Galaxies (OMEG) 2015 - Prime Hotel, Beijing, China Duration: 24 Jun 2015 → 27 Jun 2015 Conference number: 13th http://esic.ciae.ac.cn/omeg2015/ http://inspirehep.net/record/1409580 |
Conference | International Symposium on Origin of Matter and Evolution of Galaxies (OMEG) 2015 |
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Abbreviated title | OMEG 2015 |
Country/Territory | China |
City | Beijing |
Period | 24/06/15 → 27/06/15 |
Internet address |
Research output: Contribution to journal › Article › Research › peer-review
Heger, A.
Australian Research Council (ARC)
27/08/12 → 25/05/18
Project: Research