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

    Access Status
    Fulltext not available
    Authors
    Tursunov, E.
    Turakulov, S.
    Kadyrov, Alisher
    Bray, Igor
    Date
    2018
    Type
    Journal Article
    
    Metadata
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    Citation
    Tursunov, E. and Turakulov, S. and Kadyrov, A. and Bray, I. 2018. Theoretical study of the α+d→6Li+γ astrophysical capture process in a three-body model. II. Reaction rates and primordial abundance. Physical Review C. 98 (5): Article ID 055803.
    Source Title
    Physical Review C
    DOI
    10.1103/PhysRevC.98.055803
    ISSN
    2469-9985
    School
    School of Electrical Engineering, Computing and Mathematical Science (EECMS)
    URI
    http://hdl.handle.net/20.500.11937/74653
    Collection
    • Curtin Research Publications
    Abstract

    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 as a three-body bound state a+n+p in the hyperspherical Lagrange-mesh method. Corrections to the asymptotics of the overlap integral in the S and D waves have been done for the E2 S factor. The isospin forbidden E1 S factor is calculated from the initial isosinglet states to the small isotriplet components of the final Li6(1+) bound state. It is shown that the three-body model is able to reproduce the newest experimental data of the LUNA Collaboration for the astrophysical S factor and the reaction rates within the experimental error bars. The estimated Li6/H abundance ratio of (0.67±0.01)×10-14 is in a very good agreement with the recent measurement (0.80±0.18)×10-14 of the LUNA Collaboration.

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