Fusion Cross Sections of Astrophysics Interest Within the STELLA Project | Zendy

S. Courtin | Zendy; G. Fruet | Zendy; D. G. Jenkins | Zendy; M. Heine | Zendy; D. Montanari | Zendy; Luke Morris | Zendy; G. Lotay | Zendy; P. H. Regan | Zendy; O. S. Kirsebom | Zendy; S. DellaNegra | Zendy; F. Hammache | Zendy; N. de Séréville | Zendy; B. Bastin | Zendy; F. de Oliveira Santos | Zendy; G. Randisi | Zendy; C. Stödel | Zendy; Christian Beck | Zendy; F. Haas | Zendy

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Fusion Cross Sections of Astrophysics Interest Within the STELLA Project

Author(s) -

S. Courtin,

G. Fruet,

D. G. Jenkins,

M. Heine,

D. Montanari,

Luke Morris,

G. Lotay,

P. H. Regan,

O. S. Kirsebom,

S. DellaNegra,

F. Hammache,

N. de Séréville,

B. Bastin,

F. de Oliveira Santos,

G. Randisi,

C. Stödel,

Christian Beck,

F. Haas

Publication year - 2017

Publication title -

proceedings of the 14th international symposium on nuclei in the cosmos (nic2016)

Language(s) - English

Resource type - Conference proceedings

DOI - 10.7566/jpscp.14.021001

Subject(s) - stella (programming language) , computer science , astronomy , astrophysics , physics , artificial intelligence

Low energy fusion between light heavy-ions is a key feature of the evolution of massive stars. In systems of astrophysical interest, the process may be strongly affected by molecular configurations of the compound nucleus, leading to resonant S factors. In particular, the 12C+12C fusion reaction has been the object of numerous experimental investigations. The STELLA project has been developed to extend these investigations to lower energies towards the Gamow window

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