Abstract
The 12C+12C fusion reaction is one of the most important for nuclear astrophysics since it determines the carbon ignition in stellar environments. Two experiments which make use of the gamma-particle coincidence technique to measure the 12C+12C S-factors at deep sub barrier energies are discussed. Results are presented showing a decrease of the S-factor below Ec.m. = 3 MeV.
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CITATION STYLE
APA
Courtin, S., Jiang, C. L., Fruet, G., Heine, M., Jenkins, D. G., Adsley, P., … Bertone, P. (2017). Cross section measurements in the 12C+12C system. In EPJ Web of Conferences (Vol. 165). EDP Sciences. https://doi.org/10.1051/epjconf/201716501015
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