Cross section measurements in the 12C+12C system
- Courtin, S.
- Jiang, C. L.
- Fruet, G.
- Heine, M.
- Jenkins, D. G.
- Adsley, P.
- Morris, L. G.
- Regan, P. H.
- Rudigier, M.
- Montanari, D.
- Della Negra, Serge
- De Séréville, N.
- Haas, F.
- Hammache, F.
- Kirsebom, O. S.
- Lesrel, J.
- Meyer, Anne
- Montanari, D.
- Auranen, K.
- Avila, M. L.
- Ayangeakaa, A. D.
- Back, B. B.
- Bottoni, S.
- Carpenter, M
- Dickerson, C.
- DiGiovine, B. J.
- Greene, J. P.
- Henderson, D J
- Hoffman, C. R.
- Janssens, R. V F
- Kay, B. P.
- Kuvin, S. A.
- Lauritsen, T.
- Pardo, R. C.
- Rehm, K. E.
- Santiago-Gonzalez, D.
- Sethi, Jaswinder K
- Seweryniak, D.
- Talwar, R.
- Ugalde, C.
- Zhu, S.
- Deibel, C. M.
- Marley, S. T.
- Bourgin, D.
- Stodel, Christelle
- Lefebvre-Schuhl, A.
- Almaraz-Calderon, S.
- Tang, X. D.
- Alcorta, M.
- Bucher, B.
- Albers, M.
- Bertone, P.F.
DOIAbstract
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
Add to ORKG