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• W3112566374 endingPage "45" @default.
• W3112566374 startingPage "34" @default.
• W3112566374 abstract "Cross sections for the production of $^{6}mathrm{He}$, $^{6}mathrm{Li}$, $^{7}mathrm{Li}$, and $^{7}mathrm{Be}$ produced in the $ensuremath{alpha}+ensuremath{alpha}$ reaction have been measured over the energy range 60---160 MeV. Detailed angular distributions are presented for exit channels leading to $^{7}mathrm{Li}$, $^{7}mathrm{Be}$, and $^{6}mathrm{Li}$(g.s.), along with cross sections for the three-body exit channels leading to the production of $^{6}mathrm{He}$ and $^{6}mathrm{Li}$. The astrophysical significance of the $ensuremath{alpha}+ensuremath{alpha}$ reaction is discussed with particular emphasis on the production of $^{7}mathrm{Li}$ in the interaction of galactic cosmic rays with the interstellar medium. In addition, two-nucleon-transfer distorted-wave Born approximation calculations are presented in an attempt to understand the reaction mechanism operating in the $ensuremath{alpha}(ensuremath{alpha},d)^{6}mathrm{Li}(mathrm{g}.mathrm{s}.)$ reaction.NUCLEAR REACTIONS $^{4}mathrm{He}$($^{4}mathrm{He}$,HI), HI=$^{6}mathrm{He}$, $^{6}mathrm{Li}$, $^{7}mathrm{Li}$, and $^{7}mathrm{Be}$; $E=60ensuremath{-}160$ MeV; measured $frac{{d}^{2}ensuremath{sigma}}{densuremath{Omega}mathrm{dE}}$ and $ensuremath{sigma}(E)$; astrophysical relevance discussed; DWBA calculations for $^{4}mathrm{He}$($^{4}mathrm{He}$,$d$)$^{6}mathrm{Li}$." @default.
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• W3112566374 date "1982-01-01" @default.
• W3112566374 modified "2023-09-24" @default.
• W3112566374 title "Production ofHe6,Li6,Li7, andBe7in theα+areaction between 60—160 MeV" @default.
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• W3112566374 doi "https://doi.org/10.1103/physrevc.25.34" @default.
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