Astrophysical S factor for C-13(p,gamma)N-14 and asymptotic normalization coefficients

作者：Mukhamedzhanov AM^*; Azhari A; Burjan V; Gagliardi CA; Kroha V; Sattarov A; Tang X; Trache L; Tribble RE

来源：Physical Review C, 2002, 66(2): 027602.

DOI：10.1103/PhysRevC.66.027602

We reanalyze the C-13(p,gamma)N-14 radiative capture reaction within the R-matrix approach. The low-energy astrophysical S factor has important contributions from both resonant and onresonant captures. The normalization of the nonresonant component of the transition to a particular N-14 bound state is expressed in terms of the asymptotic normalization coefficient (ANC). In the analysis we use the experimental ANC's inferred from the C-13(N-14,C-13)N-14 and C-13(He-3,d)N-14 reactions. The fits of the calculated S factors to the experimental data are sensitive to the ANC values and are used to test the extracted ANC's. We find that for transitions to all the states in N-14, except the third excited state, the ANC's determined from the transfer reactions provide the best fit. The astrophysical factor we obtain, S(0)=7.7+/-1.1 keV b, is in excellent agreement with previous results.

• 出版日期2002-8