Astrophysical neutron capture rates in s- and r-process nucleosynthesis

Details Astrophysical neutron capture rates in s- and r-process nucleosynthesis Astrophysical neutron capture rates in s- and r-process nucleosynthesis

1997-06-05

arxiv.org/abs/nucl-ex/9706002v1

Physics

Nuclear Physics

Nuclear Experiment

10 pages, uses LaTeX2e with epsf.sty and camready.sty (included), 10 postscript figures with psfig (included), Proceedings of

Scientific paper

Astrophysical neutron capture rates of light and heavy nuclei have been measured and calculated. For the measurements the activation technique was applied at the 3.75 MV Karlsruhe Van de Graaff accelerator, and at the Geel electron linear accelerator (GELINA) the time-of-flight (TOF) method was used. The calculations were performed using direct and compound nuclear capture models.

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