MEASUREMENT OF O-15 (ALPHA, GAMMA) NE-19 RESONANCE STRENGTHS

被引:61
作者
MAGNUS, PV [1 ]
SMITH, MS [1 ]
HOWARD, AJ [1 ]
PARKER, PD [1 ]
CHAMPAGNE, AE [1 ]
机构
[1] PRINCETON UNIV,DEPT PHYS,PRINCETON,NJ 08544
基金
美国国家科学基金会;
关键词
Nuclear reactions;
D O I
10.1016/0375-9474(90)90390-8
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
States in 19Ne above the 15O + α threshold were populated by means of the 19F(3He,t)19Ne* reaction, and their alpha-particle decays to the 15O ground state were measured. The branching ratios Γα/Γtotal for the Ec.m. = 850-, 1020-, 1971-, 1183- and 1563-keV resonances in 19O + α were determined. This information together with alpha-particle and/or gamma-ray partial widths (determined from knowledge of these quantities for the mirror states in 19F) determines the strengths of these 15O(α,γ)19Ne resonances and the 15O(α, γ)19Ne reaction rate for temperatures between 7 × 108 and3 × 109K. © 1990.
引用
收藏
页码:332 / 345
页数:14
相关论文
共 24 条
[1]   ENERGY-LEVELS OF LIGHT-NUCLEI A=18-20 [J].
AJZENBERGSELOVE, F .
NUCLEAR PHYSICS A, 1987, 475 (01) :1-198
[2]  
ANTILLA A, 1980, NUCL PHYS A, V334, P205
[3]  
CLAYTON DD, 1982, PRINCIPLES STELLAR E
[4]   LIFETIME OF 3907 KEV STATE OF F-19 [J].
DIXON, WR ;
SYMONS, TJM ;
PILT, AA ;
ALLEN, KW ;
ZIMMERMAN, CH ;
WATT, F ;
DOLAN, SP .
PHYSICS LETTERS A, 1977, 62 (07) :479-482
[5]  
FORTUNE HT, 1986, COMMUNICATION
[6]   DYNAMICAL PHASES OF ROTATING SUPERMASSIVE STARS [J].
FRICKE, KJ .
ASTROPHYSICAL JOURNAL, 1974, 189 (03) :535-542
[7]   MICROSCOPIC STUDY OF THE O-14(ALPHA,P)F-17 REACTION AT STELLAR ENERGIES [J].
FUNCK, C ;
LANGANKE, K .
NUCLEAR PHYSICS A, 1988, 480 (01) :188-204
[8]  
GERTZ RD, 1986, AP J, V308, pL63
[9]  
KUBONO S, I NUCLEAR STUDY U TO
[10]   A NEW ESTIMATE OF THE NE-19(P, GAMMA)NA-20 AND O-15(ALPHA, GAMMA)NE-19 REACTION-RATES AT STELLAR ENERGIES [J].
LANGANKE, K ;
WIESCHER, M ;
FOWLER, WA ;
GORRES, J .
ASTROPHYSICAL JOURNAL, 1986, 301 (02) :629-633