Final state three-body Coulomb effects in the ^208Pb(^8 B,^7Be p)^208Pb Coulomb breakup reaction

Astronomy and Astrophysics – Astrophysics

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The Coulomb breakup has been suggested as an indirect method to obtain information about radiative capture cross sections at astrophysically relevant energies. In particular, the dissociation of ^8B in the Coulomb field of heavy targets like ^208 Pb, is supposed to provide the information about the low-energy astrophysical factor for the ^7Be(p,γ)^8B radiative capture. The importance of the astrophysical information determined from the Coulomb dissociation and the future application of this indirect method to determine the astrophysical capture rates for 2s 1d-shell nuclei near proton drip line dictates the necessity of thoroughful investigations of the post-decay Coulomb acceleration (PCA) which can affect the accuracy of the indirect Coulomb dissociation method. In this paper we present the first genuine quantum-mechanical calculations of the three-body final-state Coulomb interaction which allows us to estimate the PCA in the breakup reactions. We present the PCA effect for the ^208Pb(^8 B,^7Be p)^208Pb double and single differential cross sections for experiments in RIKEN [1] and MSU kinematics [2]. We find that the effect depends on the scattering angle and relative kinetic energy of the fragments. [1] T. Motobayashi et al., Phys. Rev. Lett. 73, 2680 (1994). [2] Davids B. et al., Phys. Rev. C 63, 065806 (2001).

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