English

Experimental (n,$\gamma$) cross sections of the p-process nuclei $^{74}$Se and $^{84}$Sr

Astrophysics 2009-06-30 v1 Nuclear Experiment

Abstract

The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small amount of stable isotopes on the proton-rich side cannot be made by neutron capture and are thought to be produced by photodisintegration reactions on existing seed nuclei in the so-called "p process". So far most of the p-process reactions are not yet accessible by experimental techniques and have to be inferred from statistical Hauser-Feshbach model calculations. The parametrization of these models has to be constrained by measurements on stable proton-rich nuclei. A series of (n,γ\gamma) activation measurements, related by detailed balance to the respective photodisintegrations, were carried out at the Karlsruhe Van de Graaff accelerator using the 7^7Li(p,n)7^7Be source for simulating a Maxwellian neutron distribution of kT= 25 keV. First results for the experimental (n,γ\gamma) cross sections of the light p nuclei 74^{74}Se and 84^{84}Sr are reported. These experimental values were used for an extrapolation to the Maxwellian averaged cross section at 30 keV, <σ>30<\sigma>_{30}, yielding 271±\pm15 mb for 74^{74}Se, and 300±\pm17 mb for the total capture cross section of 84^{84}Sr. The partial cross section to the isomer in 85^{85}Sr was found to be 190±\pm10 mb.

Keywords

Cite

@article{arxiv.0805.4747,
  title  = {Experimental (n,$\gamma$) cross sections of the p-process nuclei $^{74}$Se and $^{84}$Sr},
  author = {I. Dillmann and M. Heil and F. Käppeler and T. Rauscher and F. -K. Thielemann},
  journal= {arXiv preprint arXiv:0805.4747},
  year   = {2009}
}

Comments

10 pages, 5 figures