The s process in massive stars, a benchmark for neutron capture reaction rates
Marco Pignatari,
Roberto Gallino,
Rene Reifarth
Abstract:A clear definition of the contribution from the slow neutron-capture process (s process) to the solar abundances between Fe and the Sr-Zr region is a crucial challenge for nuclear astrophysics. Robust s-process predictions are necessary to disentangle the contribution from other stellar processes producing elements in the same mass region. Nuclear uncertainties are affecting s-process calculations, but most of the needed nuclear input are accessible to present nuclear experiments or they will be in the near fu… Show more
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