THE FE-54,FE-56)(N, P) MN-54,MN-56 REACTIONS AT E(N)=97 MEV

被引:79
作者
RONNQVIST, T
CONDE, H
OLSSON, N
RAMSTROM, E
ZORRO, R
BLOMGREN, J
HAKANSSON, A
RINGBOM, A
TIBELL, G
JONSSON, O
NILSSON, L
RENBERG, PU
VANDERWERF, SY
UNKELBACH, W
BRADY, FP
机构
[1] UNIV UPPSALA,DEPT RADIAT SCI,S-75121 UPPSALA,SWEDEN
[2] UNIV UPPSALA,SVEDBERG LAB,S-75121 UPPSALA,SWEDEN
[3] KERNFYS VERSNELLER INST,9747 AA GRONINGEN,NETHERLANDS
[4] INDIANA UNIV,CTR NUCL THEORY,BLOOMINGTON,IN 47408
[5] UNIV CALIF DAVIS,DEPT PHYS,DAVIS,CA 95616
关键词
FE-54(56)(N; P); E=97 MEV; MEASURED SIGMA(EP; THETA) DEDUCED GAMOW-TELLER AND DIPOLE STRENGTHS STATISTICAL MULTISTEP DIRECT DWBA CALCULATIONS MULTIPOLE DECOMPOSITION; COMPARISON WITH RPA CALCULATIONS;
D O I
10.1016/0375-9474(93)90603-U
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
Double-differential cross sections of the Fe-54,Fe-56(n, p) reactions have been measured at 97 MeV in the angular range 0-30-degrees for excitation energies up to 40 MeV. The spectra have been decomposed into different multipolarities by a technique based on the use of sample angular distributions calculated within the distorted-wave Born approximation. From the identified Gamow-Teller strength, S(beta)+ values were obtained for Fe-54 Fe and Fe-56. Comparisons with available shell-model calculations of the GT strength were made. The results are important for models of supernova explosions since electron-capture rates, which are proportional to S(beta)+, in 1f2p-shell nuclei affect the dynamics of the star. At higher excitation energies, the spectra are dominated by L = 1 strength in broad distributions with a maximum at about 12 MeV. Microscopic calculations based on the random-phase approximation were performed and compared with the experimental data.
引用
收藏
页码:225 / 246
页数:22
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