Theoretical study of the α+d→6Li+γ astrophysical capture process in a three-body model. II. Reaction rates and primordial abundance
The astrophysical S factor and reaction rate of the direct capture process a+d?Li6+?, as well as the abundance of the Li6 element, are estimated in a three-body model. The initial state is factorized into the deuteron bound state and the a+d scattering state. The final nucleus Li6(1+) is described a...
| Main Authors: | , , , |
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| Format: | Journal Article |
| Published: |
The American Physical Society
2018
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| Online Access: | http://hdl.handle.net/20.500.11937/74653 |