Cargando…
Low energy behavior of astrophysical S factor in radiative captures to loosely bound final states
The low-energy behavior of the astrophysical S-factor for E1 direct radiative captures a(p,gamma)b leading to loosely bound final states (b=a+p) is investigated. We derive a first-order integral representation for S(E) and focus on the properties around zero energy. We show that it is the competitio...
Autores principales: | Mukhamedzhanov, A M, Nunes, F M |
---|---|
Lenguaje: | eng |
Publicado: |
2002
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0375-9474(02)01011-4 http://cds.cern.ch/record/551759 |
Ejemplares similares
-
Exploratory coupled channels calculations for loosely bound carbon isotopes
por: Ridikas, D, et al.
Publicado: (1997) -
Inclusive deuteron-induced reactions and final neutron states
por: Potel, Gregory, et al.
Publicado: (2015) -
Loosely bound state production
por: Blum, Kfir
Publicado: (2021) -
Nuclear reactions for astrophysics: principles, calculation and applications of low-energy reactions
por: Thompson, Ian J, et al.
Publicado: (2009) -
Measurement of the radiative neutron capture cross section of 206Pb and its astrophysical implications
por: Domingo-Pardo, C., et al.
Publicado: (2007)