EPJ Web of Conferences (Jan 2017)
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 S.,
- de Séréville N.,
- Haas F.,
- Hammache F.,
- Kirsebom O.S.,
- Lesrel J.,
- Meyer A.,
- Montanari D.,
- Auranen K.,
- Avila M.L.,
- Ayangeakaa A.D.,
- Back B.B.,
- Bottoni S.,
- Carpenter M.,
- Dickerson C.,
- DiGiovine B.,
- 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 J.,
- Seweryniak D.,
- Talwar R.,
- Ugalde C.,
- Zhu S.,
- Deibel C.M.,
- Marley S.T.,
- Bourgin D.,
- Stodel C.,
- Lefebvre-Schuhl A.,
- Almaraz-Calderon S.,
- Fang X.,
- Tang X.D.,
- Alcorta M.,
- Bucher B.,
- Albers M.,
- Bertone P.
Affiliations
- 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 S.
- de Séréville N.
- Haas F.
- Hammache F.
- Kirsebom O.S.
- Lesrel J.
- Meyer A.
- Montanari D.
- Auranen K.
- Avila M.L.
- Ayangeakaa A.D.
- Back B.B.
- Bottoni S.
- Carpenter M.
- Dickerson C.
- DiGiovine B.
- 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 J.
- Seweryniak D.
- Talwar R.
- Ugalde C.
- Zhu S.
- Deibel C.M.
- Marley S.T.
- Bourgin D.
- Stodel C.
- Lefebvre-Schuhl A.
- Almaraz-Calderon S.
- Fang X.
- Tang X.D.
- Alcorta M.
- Bucher B.
- Albers M.
- Bertone P.
- DOI
- https://doi.org/10.1051/epjconf/201716501015
- Journal volume & issue
-
Vol. 165
p. 01015
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.
