Proton and $\gamma$- partial widths of astrophysically important states of $^{30}$S studied by the $\beta$-delayed decay of $^{31}$Ar

Resonances just above the proton threshold in $^{30}$S affect the $^{29}$P$(p,\gamma)^{30}$S reaction under astrophysical conditions. The ($p,\gamma$)-reaction rate is currently determined indirectly and depends on the properties of the relevant resonances. We present here a method for finding the r...

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Detalles Bibliográficos
Autores principales: Koldste, G.T., Blank, B., Borge, M.J.G., Briz, J.A., Carmona-Gallardo, M., Fraile, L.M., Fynbo, H.O.U., Giovinazzo, J., Johansen, J.G., Jokinen, A., Jonson, B., Kurturkian-Nieto, T., Kusk, J.H., Nilsson, T., Perea, A., Pesudo, V., Picado, E., Riisager, K., Saastamoinen, A., Tengblad, O., Thomas, J.C., Van de Walle, J.
Lenguaje:eng
Publicado: 2013
Materias:
Nuclear Physics - Experiment
Acceso en línea:https://dx.doi.org/10.1103/PhysRevC.87.055808
http://cds.cern.ch/record/1525846

Internet

https://dx.doi.org/10.1103/PhysRevC.87.055808
http://cds.cern.ch/record/1525846

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