Coulomb dissociation of unstable nuclei - simulation for radiative captures of astrophysical interest

Details Coulomb dissociation of unstable nuclei - simulation for radiative captures of astrophysical interest Coulomb dissociation of unstable nuclei - simulation for radiative captures of astrophysical interest

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998nupha.630..328m&link_type=abstract

Nuclear Physics A, Volume 630, Issue 1-2, p. 328-339.

Physics

Nuclear Physics

1

Scientific paper

Several radiative-capture processes of astrophysical interest have been studied by the Coulomb dissociation method. The method has an advantage of high experimental efficiency, which allows measurements with radioactive nuclear beams. Some discussion on the reaction mechanism is presented together with recent experimental results of the breakup of 14O and 8B studied with intermediate-energy radioactive beams.

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