The astrophysical reaction 8Li(n,gamma)9Li from measurements by reverse kinematics

Abstract

We study the breakup of 9Li projectiles in high energy (28.5 MeV/u) collisions with heavy nuclear targets (208Pb). The wave functions are calculated using a single-particle model for 9Li, and a simple optical potential model for the scattering part. A good agreement with measured data is obtained with insignificant E2 contribution.

4 pages, 3 figures

References in corpus (1)

• Energy Dependence of Breakup Cross Sections of Halo Nucleus 8B and Effective Interactions

Cited by in corpus (10)

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• Structural effects of ${}^{34}$Na in the ${}^{33}$Na(n,$\gamma {)}^{34}$Na radiative capture reaction
• Gamow shell model description of the radiative capture reaction ${}^8$Li$(n,\gamma )$${}^9$Li