Theoretical study of the α+d→6Li+γ astrophysical capture process in a three-body model. II. Reaction rates and primordial abundance

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...

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Bibliographic Details
Main Authors: Tursunov, E., Turakulov, S., Kadyrov, Alisher, Bray, Igor
Format: Journal Article
Published: The American Physical Society 2018
Online Access:http://hdl.handle.net/20.500.11937/74653

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