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Coulomb breakup of {sup 7}Li for nuclear astrophysics

Journal Article · · Physical Review C
A new Coulomb breakup experiment was performed for {sup 7}Li with an improved experimental technique and theoretical treatment. Energy spectra of {alpha} particles and tritons were examined to find the signature of post-Coulomb acceleration in the breakup of {sup 7}Li at E{sub {alpha}t}=0. The data revealed the delayed nature of nonresonant breakup of astrophysical relevance that stems from quantum tunneling. Semiclassical discussions are presented of the lifetime of continuum states in {sup 7}Li and distortion of relative kinetic energies between {alpha} and t by post-Coulomb acceleration. Dynamical calculations of Coulomb breakup were performed by solving a time-dependent Schro''dinger equation. A simple potential model of {sup 7}Li was employed. The dynamical calculations reasonably reproduced experimental cross sections for both resonant and nonresonant breakup with two key ingredients: higher order effects and mixture of E1 and E2 multipoles. Considering the dominant role of the first-order E1 nature in adiabatic Coulomb breakup, cross sections in the v{sub {alpha}}{>=}v{sub t} branch at 7{sup o}--15{sup o} for {sup 64}Zn and {sup 90}Zr were used to deduce astrophysical S factors S(E) for t({alpha},{gamma}){sup 7}Li. They exhibit a moderate energy dependence at small energies. The strongly energy-dependent S(E) resulted from the previous Coulomb breakup experiment based on cross sections with v{sub {alpha}}{<=}v{sub t}; they are most likely Coulomb distorted and are revised in the present work.
Sponsoring Organization:
(US)
OSTI ID:
40206160
Journal Information:
Physical Review C, Journal Name: Physical Review C Journal Issue: 3 Vol. 63; ISSN 0556-2813
Publisher:
The American Physical Society
Country of Publication:
United States
Language:
English

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