The astrophysical reactions 12C(α,γ)16O and 7Be(p,γ)8B and Coulomb dissociation experiments

Details The astrophysical reactions 12C(α,γ)16O and 7Be(p,γ)8B and Coulomb dissociation experiments The astrophysical reactions 12C(α,γ)16O and 7Be(p,γ)8B and Coulomb dissociation experiments

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvc..49.2688b&link_type=abstract

Physical Review C (Nuclear Physics), Volume 49, Issue 5, May 1994, pp.2688-2694

Physics

Nuclear Physics

43

Radiative Capture, 3H-, 3He-, And 4He-Induced Reactions, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, 6<=A<=19

Scientific paper

The use of the Coulomb dissociation method to obtain the cross sections for the radiative capture reactions 3C(α,γ) 16O and 7Be(p,γ) 8B is investigated. The contribution of the nuclear interaction to the breakup is included. Due to the low binding of the proton in 8B the second reaction is dominated by Coulomb breakup. The effects of Coulomb reacceleration of the fragments and of the excitation of states in the fragments are also studied. Ideal kinematical conditions for the experiments are investigated.

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