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Comparison between proton capture on N-13 and Coulomb breakup of O-14

Bibliographic reference
Permanent URL http://hdl.handle.net/2078/31538
  1. Fernandez P. B., Adelberger E. G., Garcia A., γwidth of the unbound 5.17 MeV level ofO14and the ‘‘hot’’ CNO cycle, 10.1103/physrevc.40.1887
  2. Decrock P., Delbar Th., Duhamel P., Galster W., Huyse M., Leleux P., Licot I., Liénard E., Lipnik P., Loiselet M., Michotte C., Ryckewaert G., Van Duppen P., Vanhorenbeeck J., Vervier J., Determination of theN13(p,γ)14O reaction cross section using aN13radioactive ion beam, 10.1103/physrevlett.67.808
  3. Motobayashi T., Takei T., Kox S., Perrin C., Merchez F., Rebreyend D., Ieki K., Murakami H., Ando Y., Iwasa N., Kurokawa M., Shirato S., Ruan J., Ichihara T., Kubo T., Inabe N., Goto A., Kubono S., Shimoura S., Ishihara M., Determination of the astrophysical 13N (p, γ) 14O cross section through the Coulomb dissociation method, 10.1016/0370-2693(91)90345-q
  4. Baur G., Bertulani C.A., Rebel H., Coulomb dissociation as a source of information on radiative capture processes of astrophysical interest, 10.1016/0375-9474(86)90290-3
  5. Descouvemont P., Baye D., Microscopic description of the 13N(p, γ)14O reaction at astrophysical energies, 10.1016/0375-9474(89)90135-8
  6. Hirabayashi Y., Sakuragi Y., Evidence for strong nuclear-breakup contribution toα6+dbreakup byPb208at forward angles, 10.1103/physrevlett.69.1892