期刊
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
卷 384, 期 1-2, 页码 1-84出版社
ELSEVIER
DOI: 10.1016/S0370-1573(03)00242-4
关键词
solar system; composition; stellar nucleosynthesis; p-process; nuclear reactions; statistical model
The p-process of stellar nucleosynthesis is aimed at explaining the production of the stable neutron-deficient nuclides heavier than iron that are observed up to now in the solar system exclusively. Various scenarios have been proposed to account for the bulk p-nuclide content of the solar system, as well as for deviations ('anomalies') with respect to the bulk p-isotope composition of some elements discovered in primitive meteorites. The astrophysics of these models is reviewed, and the involved nuclear physics is discussed, including a brief account of recent experimental efforts. Already published results are complemented with new ones. A specific attention is paid to the very rare odd-odd nuclides La-138 and Ta-180(m), as well as to the puzzling case of the light Mo and Ru isotopes. Astrophysics and nuclear physics prospects of improvements in the p-process modeling are presented. (C) 2003 Elsevier B.V. All rights reserved.
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