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Neutron capture cross sections and solar abundances of /sup 160,161/Dy, /sup 170,171/Yb, /sup 175,176/Lu, and /sup 176,177/Hf have been measured

Journal Article · · Phys. Rev. C; (United States)
The neutron capture cross sections and solar abundances of /sup 160,161/Dy, /sup 170,171/Yb, /sup 175,176/Lu, and /sup 176,177/Hf have been measured. With this data base s-process studies have been carried out to determine the s-process neutron density and temperature and to investigate the s-process nucleosynthesis of the /sup 176/Lu clock. From various branchings the neutron density was found to be (0.8--1.8) x 10/sup 8/ neutrons per cm/sup 3/ and the temperature kT to be 18--28 keV. On the basis of the present data, /sup 176/Lu proved not to be applicable as a cosmic clock because of the temperature sensitivity of the /sup 176/Lu half-life but can be used instead as a stellar thermometer. Constraints for the s-process temperature (kT = 20--28 keV) were found to be in good agreement with the investigated branchings.
Research Organization:
Kernforschungszentrum Karlsruhe, Institut fuer Kernphysik III, D-7500 Karlsruhe, Federal Republic of Germany
OSTI ID:
6543947
Journal Information:
Phys. Rev. C; (United States), Journal Name: Phys. Rev. C; (United States) Vol. 30:2; ISSN PRVCA
Country of Publication:
United States
Language:
English

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