First Accurate Normalization of the $\beta$-delayed $\alpha$ Decay of $^{16}$N and Implications for the $^{12}$C$(\alpha,\gamma)^{16}$O Astrophysical Reaction Rate

The C12(α,γ)O16 reaction plays a central role in astrophysics, but its cross section at energies relevant for astrophysical applications is only poorly constrained by laboratory data. The reduced α width, γ11, of the bound 1- level in O16 is particularly important to determine the cross section. The...

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Detalles Bibliográficos
Autores principales: Kirsebom, O.S., Tengblad, O., Lica, R., Munch, M., Riisager, K., Fynbo, H.O.U., Borge, M.J.G., Madurga, M., Marroquin, I., Andreyev, A.N., Berry, T.A., Christensen, E.R., Fernández, P. Díaz, Doherty, D.T., Van Duppen, P., Fraile, L.M., Gallardo, M.C., Greenlees, P.T., Harkness-Brennan, L.J., Hubbard, N., Huyse, M., Jensen, J.H., Johansson, H., Jonson, B., Judson, D.S., Konki, J., Lazarus, I., Lund, M.V., Marginean, N., Marginean, R., Perea, A., Mihai, C., Negret, A., Page, R.D., Pucknell, V., Rahkila, P., Sorlin, O., Sotty, C., Swartz, J.A., Sørensen, H.B., Törnqvist, H., Vedia, V., Warr, N., De Witte, H.
Lenguaje:eng
Publicado: 2018
Materias:
nucl-ex
Nuclear Physics - Experiment
Acceso en línea:https://dx.doi.org/10.1103/PhysRevLett.121.142701
http://cds.cern.ch/record/2312305

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