The Dy163-Ho163 branching: An s-process barometer

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150<=A<=189, Radiative Capture, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

The neutron capture cross sections of Dy163 and Er164 have been measured to analyse the s-process branching at Dy163-Ho163. The reproduction of the s-process abundance of Er164 via this branching is sensitive to temperature kT, neutron density, and electron density ne. The calculations using information from other branchings on kT and the neutron density nn give constraints for ne at the site of the s-process.

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