AbstractAbstract
[en] The activation method is used to measure the stellar neutron capture rates of Re-185 and Re-187 at kT = 25 keV as 1677 + or - 65 and 1269 + or - 62 mbarn, respectively. The experimental setup and procedure are described, and the results are presented in tables and graphs. Also reported are calculations of the capture rates for the unstable isotopes, e.g., 597 + or - 85 mbarn for W-185 and 1775 + or - 265 mbarn for Re-186, again at kT = 25 keV. These results are then applied, using the classical method, to estimate the mean neutron density for the s-process nucleosynthesis branchings at W-185 and Re-186: n(n) = (4.1 + 1.2 or - 1.1) x 10 to the 8th/cu cm. 64 refs
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Journal Article
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Numerical Data
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ACTIVATION ANALYSIS, BARYON REACTIONS, BETA DECAY RADIOISOTOPES, BETA-MINUS DECAY RADIOISOTOPES, CHEMICAL ANALYSIS, DATA, DAYS LIVING RADIOISOTOPES, ELECTRON CAPTURE RADIOISOTOPES, EVEN-ODD NUCLEI, HADRON REACTIONS, HEAVY NUCLEI, INFORMATION, ISOMERIC TRANSITION ISOTOPES, ISOTOPES, MATHEMATICAL MODELS, MATHEMATICS, MINUTES LIVING RADIOISOTOPES, NONDESTRUCTIVE ANALYSIS, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, NUMERICAL DATA, ODD-ODD NUCLEI, QUANTITY RATIO, RADIOISOTOPES, RHENIUM ISOTOPES, STAR EVOLUTION, SYNTHESIS, TUNGSTEN ISOTOPES, YEARS LIVING RADIOISOTOPES
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