17 págs.; 9 figs.; 3 tabs.We investigate even-even two-proton Borromean systems at prominent intermediate heavy waiting points for the rapid proton capture process. The most likely single-particle levels are used to calculate three-body energy and structure as a function of proton-core resonance energy. We establish a linear dependence between two- and three-body energies with the same slope, but the absolute value slightly dependent on partial wave structure. Using these relations we estimate low-lying excited states in the isotones following the critical waiting points. The capture rate for producing a Borromean bound state is described based on a full three-body calculation for temperatures about 0.1¿10 GK. In addition, a simple rate exp...
7 pags., 3 figs. -- PACS :21.45.+v; 31.15.Ja; 25.70.EfThe complex energies of the three-body resonan...
International audienceThe slow β-decay of the 68Se waiting point in the astrophysical rp-process can...
AbstractThe slow β-decay of the 68Se waiting point in the astrophysical rp-process can in principle ...
4 pags., 3 figs. -- 11th International Conference on Clustering Aspects of Nuclear Structure and Dyn...
4 pags., 3 figs. -- This article belongs to the Topical Collection “The 23rd European Conference on ...
We investigate the two-proton capture reaction of the prominent rapid proton capture waiting point n...
The slow β-decay of the 68Se waiting point in the astrophysical rp-process can in principle be bypas...
This research was sponsored by the National Science Foundation Grant NSF PHY-931478
Radiative capture reaction rates for 6He, 9Be and 17Ne formation at astrophysical conditions are stu...
12 pags., 6 figs., 2 tabs.We investigate four-body nuclear reactions in stellar environments contrib...
Background: The breakout from the hot Carbon-Nitrogen-Oxigen (CNO) cycles can trigger the rp-process...
For the first time Borromean nucleus induced reactions have been measured below the three-body break...
The structure of the Borromean nucleus 9Be (α+α+n) is addressed within a three-body approach using t...
We report on the first direct measurement of the proton separation energy for the proton-unbound nuc...
Microscopic optical potentials obtained by folding the DDM3Y interaction with the densities from the...
7 pags., 3 figs. -- PACS :21.45.+v; 31.15.Ja; 25.70.EfThe complex energies of the three-body resonan...
International audienceThe slow β-decay of the 68Se waiting point in the astrophysical rp-process can...
AbstractThe slow β-decay of the 68Se waiting point in the astrophysical rp-process can in principle ...
4 pags., 3 figs. -- 11th International Conference on Clustering Aspects of Nuclear Structure and Dyn...
4 pags., 3 figs. -- This article belongs to the Topical Collection “The 23rd European Conference on ...
We investigate the two-proton capture reaction of the prominent rapid proton capture waiting point n...
The slow β-decay of the 68Se waiting point in the astrophysical rp-process can in principle be bypas...
This research was sponsored by the National Science Foundation Grant NSF PHY-931478
Radiative capture reaction rates for 6He, 9Be and 17Ne formation at astrophysical conditions are stu...
12 pags., 6 figs., 2 tabs.We investigate four-body nuclear reactions in stellar environments contrib...
Background: The breakout from the hot Carbon-Nitrogen-Oxigen (CNO) cycles can trigger the rp-process...
For the first time Borromean nucleus induced reactions have been measured below the three-body break...
The structure of the Borromean nucleus 9Be (α+α+n) is addressed within a three-body approach using t...
We report on the first direct measurement of the proton separation energy for the proton-unbound nuc...
Microscopic optical potentials obtained by folding the DDM3Y interaction with the densities from the...
7 pags., 3 figs. -- PACS :21.45.+v; 31.15.Ja; 25.70.EfThe complex energies of the three-body resonan...
International audienceThe slow β-decay of the 68Se waiting point in the astrophysical rp-process can...
AbstractThe slow β-decay of the 68Se waiting point in the astrophysical rp-process can in principle ...