Experimentally constrained (p,γ)89Y and (n,γ)89Y reaction rates relevant to p-process nucleosynthesis

被引:30
|
作者
Larsen, A. C. [1 ]
Guttormsen, M. [1 ]
Schwengner, R. [2 ]
Bleuel, D. L. [3 ]
Goriely, S. [4 ]
Harissopulos, S. [5 ]
Garrote, F. L. Bello [1 ]
Byun, Y. [6 ]
Eriksen, T. K. [1 ]
Giacoppo, F. [1 ]
Gorgen, A. [1 ]
Hagen, T. W. [1 ]
Klintefjord, M. [1 ]
Renstrom, T. [1 ]
Rose, S. J. [1 ]
Sahin, E. [1 ]
Siem, S. [1 ]
Tornyi, T. G. [1 ]
Tveten, G. M. [1 ]
Voinov, A. V. [6 ]
Wiedeking, M. [7 ]
机构
[1] Univ Oslo, Dept Phys, POB 1048, N-0316 Oslo, Norway
[2] Helmholtz Zentrum Dresden Rossendorf, D-01328 Dresden, Germany
[3] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA
[4] Univ Libre Bruxelles, Inst Astron & Astrophys, Brussels, Belgium
[5] NCSR Demokritos, Inst Nucl & Particle Phys, Athens, Greece
[6] Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA
[7] IThemba LABS, POB 722, ZA-7129 Somerset West, South Africa
基金
新加坡国家研究基金会;
关键词
PHOTONEUTRON CROSS-SECTIONS; MODEL-CALCULATIONS; STRENGTH FUNCTION; LEVEL DENSITY; ASTROPHYSICS; ELEMENTS; SPECTRA; LIBRARY; NUCLEI; SYSTEM;
D O I
10.1103/PhysRevC.93.045810
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 nuclear level density and the gamma-ray strength function have been extracted for Y-89 by using the Oslo method on Y-89(p,p gamma')Y-89 coincidence data. The gamma-ray strength function displays a low-energy enhancement consistent with previous observations in this mass region (Mo93-98). Shell-model calculations support the conclusion that the observed enhancement is due to strong, low-energy M1 transitions at high excitation energies. The data were further used as input for calculations of the Sr-88(p,gamma)Y-89 and Y-88(n,gamma)Y-89 cross sections with the TALYS reaction code. Comparison with cross-section data, where available, as well as with values from the BRUSLIB library, shows a satisfying agreement.
引用
收藏
页数:13
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