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• W1514096893 abstract "$^{13}$N($p,gamma$)$^{14}$O is one of the key reactions in the hot CNO cycle which occurs at stellar temperatures around $T_9$ $geq$ 0.1. Up to now, some uncertainties still exist for the direct capture component in this reaction, thus an independent measurement is of importance. In present work, the angular distribution of the $^{13}$N($d,n$)$^{14}$O reaction at $E_{rm{c.m.}}$ = 8.9 MeV has been measured in inverse kinematics, for the first time. Based on the distorted wave Born approximation (DWBA) analysis, the nuclear asymptotic normalization coefficient (ANC), $C^{^{14}O}_{1,1/2}$, for the ground state of $^{14}$O $to$ $^{13}$N + $p$ is derived to be $5.42 pm 0.48$ fm$^{-1/2}$. The $^{13}$N($p,gamma$)$^{14}$O reaction is analyzed with the R-matrix approach, its astrophysical S-factors and reaction rates at energies of astrophysical relevance are then determined with the ANC. The implications of the present reaction rates on the evolution of novae are then discussed with the reaction network calculations." @default.
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• W1514096893 date "2006-09-18" @default.
• W1514096893 modified "2023-10-18" @default.
• W1514096893 title "N13(d,n)O14reaction and the astrophysicalN13(p,γ)O14reaction rate" @default.
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• W1514096893 doi "https://doi.org/10.1103/physrevc.74.035801" @default.
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