BETA-DELAYED ALPHA-SPECTRUM OF N-16 AND THE C-12(ALPHA,GAMMA)O-16 CROSS-SECTION AT LOW ENERGIES

被引:87
作者
BUCHMANN, L
AZUMA, RE
BARNES, CA
DAURIA, JM
DOMBSKY, M
GIESEN, U
JACKSON, KP
KING, JD
KORTELING, RG
MCNEELY, P
POWELL, J
ROY, G
VINCENT, J
WANG, TR
WONG, SSM
WREAN, PR
机构
[1] UNIV TORONTO,TORONTO M5S 1A7,ONTARIO,CANADA
[2] CALTECH,WK KELLOGG LAB,PASADENA,CA 91125
[3] SIMON FRASER UNIV,BURNABY V5A 1S6,BC,CANADA
[4] UNIV ALBERTA,EDMONTON T6G 2G1,ALBERTA,CANADA
关键词
D O I
10.1103/PhysRevLett.70.726
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The alpha spectrum following the beta decay of N-16 from the isotope separator TISOL has been measured by detecting 10(6) alpha particles in coincidence with C-12 nuclei. These data, which show a low-energy interference anomaly accompanying the main alpha peak, permit a more precise determination of the p-wave amplitude of the astrophysically important reaction C-12(alpha, gamma)O-16. The alpha spectrum and previous gamma-ray data have been fitted simultaneously by a K-matrix parametrization; a value of S(E = 0.3 MeV)= 57 +/- 13 keV b has been obtained for the E1 part of the C-12(alpha, gamma)O-16 reaction.
引用
收藏
页码:726 / 729
页数:4
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