C. Barbieri, B. K. Jennings
Published 2004-08-05Version 1
The Feshbach theory of the optical potential naturally leads to a microscopic description of scattering in terms of the many-body self-energy. We consider a recent calculation of this quantity for 16O and study the possibility of applying it at astrophysical energies. The results obtained for the phase shifts and the 16O(p,\gamma) capture suggest that such studies are feasible but the calculations require some improvement geared to this specific task.
Comments: 4 pages, 3 figures; Proceedings of Nuclei In The Cosmos VIII, to appear in Nucl. Phys. A
Journal: Nucl.Phys. A758 (2005) 395-398
$Λ$-hypernuclear production in ($K^-_{\rm stop}, π$) reactions
Radiative neutron capture on 9be, 14c, 14n, 15n and 16o at thermal and astrophysical energies
Study of the neutron and proton capture reactions 10,11b(n, g), 11b(p, g), 14c(p, g), and 15n(p, g) at thermal and astrophysical energies
