REACTION-RATES OF THE S-PROCESS NEUTRON SOURCES NE-22(ALPHA,N)MG-25 AND C-13(ALPHA,N)O-16(1)

被引:141
作者
DROTLEFF, HW
DENKER, A
KNEE, H
SOINE, M
WOLF, G
HAMMER, JW
GRIEFE, U
ROLFS, C
TRAUTVETTER, HP
机构
[1] UNIV STUTTGART,INST STRAHLENPHYS,W-7000 STUTTGART 80,GERMANY
[2] RUHR UNIV BOCHUM,INST EXPTL PHYS 3,W-4630 BOCHUM 1,GERMANY
关键词
NUCLEAR REACTIONS; NUCLEOSYNTHESIS; ABUNDANCES; STARS; CHEMICALLY PECULIAR; EVOLUTION; GIANT; INTERIORS;
D O I
10.1086/173119
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The excitation function of the s-process neutron source reactions Ne-22(alpha, n)Mg-25 and C-13(alpha, n)O-16 has been measured using improved ion-beam, target, and detection techniques, reaching a sensitivity limit of 50 picobarns in the best cases. For Ne-22(alpha, n)Mg-25 the new data cover the energy range from threshold (E(alpha,lab) = 570 keV) up to E(alpha,lab) = 2300 keV. From these experiments some of the parameters of the Ne-22(alpha, n)Mg-25 resonances have been determined using unfolding techniques. A resonance at about E(alpha,lab) = 620 keV could clearly be ascribed to the background reaction B-11(alpha, n)N-14. The excitation function of C-13(alpha, n)O-16 has been measured over the energy range E(alpha, lab) = 350-1400 keV, where the cross section varies over eight orders of magnitude. The S-factor of this reaction indicates an increase toward lower energies, possibly due to a state in O-17 below the (C-13 + alpha) threshold leading to a higher reaction rate. On the basis of the experimental data the reaction rates at helium-burning temperatures were determined for these two reactions: both rates are increased compared with previous evaluations.
引用
收藏
页码:735 / 739
页数:5
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