학술논문
Cross section measurements in the 12C+12C system
Document Type
article
Author
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.; 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.
Source
EPJ Web of Conferences, Vol 165, p 01015 (2017)
Subject
Language
English
ISSN
2100-014X
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.