At the long-wavelength approximation, electric dipole transitions are forbidden between isospin-zero states. In an (formula presented) model with (formula presented) contributions, the (formula presented)Li astrophysical S-factor is in agreement with the experimental data of the LUNA collaboration, without adjustable parameter. The exact-masses prescription used to avoid the disappearance of E1 transitions in potential models is not founded at the microscopic level.SCOPUS: cp.pinfo:eu-repo/semantics/publishe
The thesis deals with the study of the radiative capture α + d → 6Li + γ, (1) where α and d indicate...
The 6Li(p,alpha )3He bare nucleus cross-section at astrophysical energies has been indirectly measur...
The astrophysical S factor of the [Formula Presented] radiative capture reaction is analyzed at zero...
At the long-wavelength approximation, E1 transitions are forbidden between isospin-zero states. Henc...
The alpha+d->6Li+gamma radiative capture is studied in order to predict the Li6 primordial abundance...
Journals published by the American Physical Society can be found at http://publish.aps.org/We consid...
Open access article distributed under the terms of the Creative Commons Attribution License 4.0, whi...
International audienceWe have applied the Gamow shell model (GSM) in the coupled-channel representat...
We propose a physically transparent analytic model of astrophysical S factors as a function of a cen...
The low-energy behavior of the astrophysical S-factor for E1 direct radiative captures a(p,gamma)b l...
We present a new calculation of the Li6(p,γ) 7 Be radiative capture astrophysical S-factor in a clus...
The astrophysical S-factors of thermonuclear reactions, including radiative capture reactions and th...
The astrophysical S-factor for the6Li(p,Υ)7Be reaction is calculated in a cluster-model framework. T...
We have applied the Gamow shell model (GSM) in the coupled-channel representation to study the astro...
We have applied the Gamow shell model (GSM) in the coupled-channel representation to study the astro...
The thesis deals with the study of the radiative capture α + d → 6Li + γ, (1) where α and d indicate...
The 6Li(p,alpha )3He bare nucleus cross-section at astrophysical energies has been indirectly measur...
The astrophysical S factor of the [Formula Presented] radiative capture reaction is analyzed at zero...
At the long-wavelength approximation, E1 transitions are forbidden between isospin-zero states. Henc...
The alpha+d->6Li+gamma radiative capture is studied in order to predict the Li6 primordial abundance...
Journals published by the American Physical Society can be found at http://publish.aps.org/We consid...
Open access article distributed under the terms of the Creative Commons Attribution License 4.0, whi...
International audienceWe have applied the Gamow shell model (GSM) in the coupled-channel representat...
We propose a physically transparent analytic model of astrophysical S factors as a function of a cen...
The low-energy behavior of the astrophysical S-factor for E1 direct radiative captures a(p,gamma)b l...
We present a new calculation of the Li6(p,γ) 7 Be radiative capture astrophysical S-factor in a clus...
The astrophysical S-factors of thermonuclear reactions, including radiative capture reactions and th...
The astrophysical S-factor for the6Li(p,Υ)7Be reaction is calculated in a cluster-model framework. T...
We have applied the Gamow shell model (GSM) in the coupled-channel representation to study the astro...
We have applied the Gamow shell model (GSM) in the coupled-channel representation to study the astro...
The thesis deals with the study of the radiative capture α + d → 6Li + γ, (1) where α and d indicate...
The 6Li(p,alpha )3He bare nucleus cross-section at astrophysical energies has been indirectly measur...
The astrophysical S factor of the [Formula Presented] radiative capture reaction is analyzed at zero...