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• W2347168047 abstract "The astrophysical capture process $ensuremath{alpha}+densuremath{rightarrow}^{6}mathrm{Li}$ is studied in a three-body model. The initial state is factorized into the deuteron bound state and the ($ensuremath{alpha}+d$)-scattering state. The final nucleus $^{6}mathrm{Li}({1}^{+})$ is described as a three-body bound state $ensuremath{alpha}+n+p$ in the hyperspherical Lagrange-mesh method. The contribution of the $E1$-transition operator from the initial isosinglet states to the isotriplet components of the final state is estimated to be negligible. An estimation of the forbidden $E1$ transition to the isosinglet components of the final state is comparable with the corresponding results of the two-body model. However, the contribution of the $E2$-transition operator is found to be much smaller than the corresponding estimations of the two-body model. The three-body model perfectly matches the new experimental data of the LUNA Collaboration with the spectroscopic factor of 2.586 estimated from the bound-state wave functions of $^{6}mathrm{Li}$ and a deuteron." @default.
• W2347168047 created "2016-06-24" @default.
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• W2347168047 date "2016-07-13" @default.
• W2347168047 modified "2023-10-10" @default.
• W2347168047 title "Theoretical study of the<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mrow><mml:mi>α</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>→</mml:mo><mml:mrow><mml:mmultiscripts><mml:mi mathvariant=normal>Li</mml:mi><mml:mprescripts /><mml:none /><mml:mrow><mml:mn>6</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow><mml:mo>+</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>astrophysical capture process in a three-body model" @default.
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• W2347168047 doi "https://doi.org/10.1103/physrevc.94.015801" @default.
• W2347168047 hasPublicationYear "2016" @default.
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