论文标题
低能和核天体物理学的电荷颗粒转移反应的分散（渐近）理论：ii。渐近归一化系数及其核粪便应用
Dispersion (asymptotic) theory of charged particle transfer reactions at low energies and nuclear astrophysics: II. the asymptotic normalization coefficients and their nuclear-astrophysical application
论文作者
论文摘要
在作者R. Yarmukhamedov和K.I.提出的渐近理论中Tursunmakhatov [Phys。 Rev. C (submitted 2019)] for the peripheral sub- and above-barrier transfer $A$($x$, $y$)$B$ reaction in the three-body ($A$, $a$ and $y$) model ($ x$= $y$ + $a$ and $B$= $A$ + $a$, and $ a$ is a transferred particle), the analysis of the experimental angular distributions of the differential cross sections is performed for the外围质子和Triton转移$ {\ rm {^9be（^{10} b，\，^9be）^{10} b}} $，$ {\ rm {\ rm {^{16} {16} o（^3he}}} $ {\ rm {^{^{19} f（}} p，\，α{\ rm {）^{16} o}} $ reactions $ reactions $ reactions在上述和子弹药弹能。对于$ {\ rm {^9be}} \，+p \ to \ t \ t \ t \ t \ t \ rm {\ rm {^rm {^{10} b}} $，$ {10} b}} $，+rmmmmmm { \ to \，{\ rm {^{17} f}} $和$ {\ rm {^{^{16} o}}} \，+\，t \ to {\ rm {^rm {^{19} f}}} $。它们用于用于计算核胃物理$ {\ rm {^9BE（}}} p，\，γ{\ rm {）^{10} b}}} $， $ {\ rm {^{16} o（}} p，\，γ{\ rm {）^{17} f}} $和$ {\ rm {^rm {^{19} f（}} f（}} p，\，\，\，\，α{\ rm {\ rm {\ rm {16}}}对于恒星能量的天体物理$ s $因素，获得了新的值及其不确定性。
Within the asymptotic theory proposed by authors R. Yarmukhamedov and K.I. Tursunmakhatov [Phys. Rev. C (submitted 2019)] for the peripheral sub- and above-barrier transfer $A$($x$, $y$)$B$ reaction in the three-body ($A$, $a$ and $y$) model ($ x$= $y$ + $a$ and $B$= $A$ + $a$, and $ a$ is a transferred particle), the analysis of the experimental angular distributions of the differential cross sections is performed for the peripheral proton and triton transfer ${\rm{^9Be(^{10}B,\,^9Be)^{10}B}}$, ${\rm{^{16}O(^3He}},\,d{\rm{)^{17}F}}$ and ${\rm{^{19}F(}}p,\,α{\rm{)^{16}O}}$ reactions at above-and sub-barrier projectile energies, respectively. New estimates and their uncertainties are obtained for magnitudes of the asymptotic normalization coefficients (respective the nuclear vertex constants) for ${\rm{^9Be}} \,+p \to\,{\rm{^{10}B}}$, ${\rm{^{16}O}} \,+\,p \to\, {\rm{^{17}F}}$ and ${\rm{^{16}O}} \,+\,t\to{\rm{^{19}F}}$. They are applied for calculations of the astrophysical $S$ factors for the nuclear-astrophysical ${\rm{^9Be(}}p,\,γ{\rm{)^{10}B}} $, ${\rm{^{16}O(}}p,\,γ{\rm{)^{17}F}}$ and ${\rm{^{19}F(}}p,\,α{\rm{)^{16}O)}}$ reactions at thermonuclear energies. New values and their uncertainties are obtained for the astrophysical $S$ factors at stellar energies.
