TY - JOUR AU - n_TOF Collaboration AU - Kappeler, F. AU - Mengoni, A. AU - Mosconi, M. AU - Fujii, K. AU - Heil, M. AU - Domingo-Pardo, C. PY - 2011 DA - 2011// TI - Neutron Studies for Dating the Universe T2 - J. Korean Phys. Soc. JO - Journal of the Korean Physical Society SP - 2094 EP - 2099 VL - 59 IS - 2 PB - Korean Physical Soc KW - Neutron capture and inelastic scattering cross sections KW - Re/Os cosmo-chronometer AB - The neutron capture cross sections of (186)Os and (187)Os are of key importance for defining the 8-process abundance of (187)Os at the formation of the solar system. This quantity can be used to determine the radiogenic abundance component of (187)Os from the decay of (187)Re (t(1/2) = 41.2 Gyr) and to infer the time-duration of the nucleosynthesis in our galaxy (Re/Os cosmochronometer). The neutron capture cross sections of (186)Os, (187)Os, and (188)Os have been measured at the CERN n_TOF facility from 1 eV to 1 MeV, covering the entire energy range of astrophysical interest. From these data Maxwellian averaged capture cross sections have been calculated with uncertainties between 3.3 and 4.7%. Additional information was obtained by measuring the inelastic scattering cross section of (187)Os at the Karlsruhe 3.7 MV Van de Graaff accelerator and by neutron resonance analyses of the n_TOF capture data to establish a comprehensive experimental basis for the Hauser-Feshbach statistical model. Consistent I-IF calculations for the capture and inelastic reaction channels were performed to determine the stellar enhancement factors, which are required to correct the Maxwellian averaged cross sections for the effect of thermally populated excited states. The consequences of this analysis for the s-process component of the (187)Os abundance and the related impact on the evaluation of the time-duration of Galactic nucleosynthesis via the Re/Os cosmo-chronometer are discussed. SN - 0374-4884 UR - https://doi.org/10.3938/jkps.59.2094 DO - 10.3938/jkps.59.2094 LA - English N1 - WOS:000294080700156 ID - n_TOFCollaboration_etal2011 ER -