Asymptotic normalization coefficients for 14N⇆13C+p from 13C(3He,d)14N -: art. no. 024320

被引:31
作者
Bém, P
Burjan, V
Kroha, V
Novák, J
Piskor, S
Simecková, E
Vincour, J
Gagliardi, CA [1 ]
Mukhamedzhanov, AM
Tribble, RE
机构
[1] Acad Sci Czech Republ, Inst Nucl Phys, Prague, Czech Republic
[2] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA
来源
PHYSICAL REVIEW C | 2000年 / 62卷 / 02期
关键词
D O I
10.1103/PhysRevC.62.024320
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The C-13(He-3,d) N-14 proton transfer reaction has been measured at an incident energy of 26.3 MeV. Angular distributions for proton transfer to the ground state and excited states at 2.313 and 3.948 MeV in N-14 are analyzed within the framework of the modified DWBA. Asymptotic normalization coefficients (ANC's) defining the amplitude of the tails of the N-14 bound-state wave functions in the C-13+p channel are extracted that are in excellent agreement with values found previously with the C-13(N-14,C-13)N-14 reaction. We conclude that C-p1/2(2)=18.2(9) fm(-1) and C-p3/2(2) = 0.91(14) fm(-1) for the virtual decay N-14(g.s.) --> C-13+p. These are necessary for the analysis of the N-14(Be-7, B-8)C-13 and N-14( C-11, N-12) C-13 reactions to extract the ANC's far Be-7+p --> B-8 and C-11+p-->N-12, which determine the direct radiative capture cross sections Be-7(p,gamma)B-8 and C-11(p,gamma)N-12 at astrophysical energies.
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