BRIDGING THE WAITING POINTS - THE ROLE OF 2-PROTON CAPTURE REACTIONS IN THE RP-PROCESS

被引:102
作者
GORRES, J
WIESCHER, M
THIELEMANN, FK
机构
[1] HARVARD SMITHSONIAN CTR ASTROPHYS, CAMBRIDGE, MA 02138 USA
[2] UNIV BASEL, INST THEORET PHYS, CH-4056 BASEL, SWITZERLAND
来源
PHYSICAL REVIEW C | 1995年 / 51卷 / 01期
关键词
D O I
10.1103/PhysRevC.51.392
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 influence of two-proton capture reactions on long-lived waiting point isotopes near the proton drip line is discussed for the rp-process reaction flow. These reactions are characterized by two successive proton captures, where the first reaction product is unstable against proton emission, but the second reaction results in a particle stable nucleus. The reactions which have this character and involve long-lived waiting points in the rp process are O15(2p,γ)17Ne, Ne18(2p,γ)20Mg, and Ca38(2p,γ)40Ti. Their rates are presented and compared with the rates of alpha-induced reactions for stellar conditions at high temperatures and densities. We find that the two-proton captures on O15 and Ne18 can only compete for unrealistically high densities, but that Ca38(2p,γ)40Ti can act as an efficient reaction link at conditions typical for x-ray bursts on neutron stars. © 1995 The American Physical Society.
引用
收藏
页码:392 / 400
页数:9
相关论文
共 20 条
[1]   ENERGY-LEVELS OF LIGHT-NUCLEI A=18-20 [J].
AJZENBERGSELOVE, F .
NUCLEAR PHYSICS A, 1987, 475 (01) :1-198
[2]   ENERGY-LEVELS OF LIGHT-NUCLEI A=16-17 [J].
AJZENBERGSELOVE, F .
NUCLEAR PHYSICS A, 1986, 460 (01) :1-148
[3]   STRUCTURE OF MG-22, SI-26, AR-34 AND CA-38 VIA THE (HE-3, N) REACTION [J].
ALFORD, WP ;
CRAIG, P ;
LIND, DA ;
RAYMOND, RS ;
ULLMAN, J ;
ZAFIRATOS, CD ;
WILDENTHAL, BH .
NUCLEAR PHYSICS A, 1986, 457 (02) :317-336
[4]   THE R-PROCESS AND NUCLEOCHRONOLOGY [J].
COWAN, JJ ;
THIELEMANN, FK ;
TRURAN, JW .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1991, 208 (4-5) :267-394
[5]  
Endt P. M., 1979, Atomic Data and Nuclear Data Tables, V23, P3, DOI 10.1016/0092-640X(79)90020-2
[6]   ENERGY-LEVELS OF A = 21-44 NUCLEI (VII) [J].
ENDT, PM .
NUCLEAR PHYSICS A, 1990, 521 :1-830
[7]   STUDY OF NE-22 WIT NE-20 (T, P) REACTION [J].
FLYNN, ER ;
HANSEN, O ;
NATHAN, O .
NUCLEAR PHYSICS A, 1974, A228 (02) :189-204
[8]   THERMONUCLEAR REACTION RATES [J].
FOWLER, WA ;
CAUGHLAN, GR ;
ZIMMERMAN, BA .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1967, 5 :525-+
[9]   THE ASTROPHYSICAL IMPLICATIONS OF LOW-ENERGY RESONANCES IN NE-22+ALPHA [J].
GIESEN, U ;
BROWNE, CP ;
GORRES, J ;
GRAFF, S ;
ILIADIS, C ;
TRAUTVETTER, HP ;
WIESCHER, M ;
HARMS, W ;
KRATZ, KL ;
PFEIFFER, B ;
AZUMA, RE ;
BUCKBY, M ;
KING, JD .
NUCLEAR PHYSICS A, 1993, 561 (01) :95-111
[10]  
HALBERT EC, 1971, ADVANCES NUCLEAR STA, V4, P316