K. Vogt et al., Measurement of the (gamma,n) reaction rates of the nuclides Pt-190, Pt-192, and Pt-198 in the astrophysical gamma process - art. no. 055802, PHYS REV C, 6305(5), 2001, pp. 5802
The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon b
ath at the temperatures relevant for the astrophysical gamma process was in
vestigated. In order to derive (gamma ,n) cross sections and reaction rates
, the stellar photon bath was simulated by the superposition of several bre
msstrahlung spectra with different endpoint energies. As a first test for t
his method, the (gamma ,n) reaction rates of the platinum isotopes Pt-190,
Pt-192, and Pt-198 were derived. The results are compared to other experime
ntal data and theoretical calculations.