The s-process near the iron seed - Some improved capture cross sections

Details The s-process near the iron seed - Some improved capture cross sections The s-process near the iron seed - Some improved capture cross sections

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....37..197b&link_type=abstract

Astronomy and Astrophysics, vol. 37, no. 1, Dec. 1974, p. 197-200.

Astronomy and Astrophysics

Astrophysics

11

Iron Isotopes, Neutron Cross Sections, Nuclear Capture, Abundance, Chromium Isotopes, Fortran, Maxwell-Boltzmann Density Function, Neutron Flux Density, Nickel Isotopes, Time Of Flight Spectrometers, Van De Graaff Accelerators, Velocity Distribution

Scientific paper

Maxwellian averaged capture cross sections on the nuclei Cr-50,52,53; Fe-54,56,57; Co-59; and Ni-58,60,61,62,64 have been determined for temperatures between kT 5 keV and 75 keV. The abundance-times-cross-section curve of Fe-56, Fe-57, Co-59, Ni-60, Ni-61, Ni-62, and Ni-64 as a function of atomic weight shows a maximum at mass number 60. The smooth decrease of the curvature for the nickel isotopes was considered as an indication of the s-process origin of these nuclei.

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