Measurement of (alpha,n) reaction cross sections of erbium isotopes for testing astrophysical rate predictions
arXiv:1503.01853 · doi:10.1088/0954-3899/42/5/055103
Abstract
The -process in core-collapse and/or type Ia supernova explosions is thought to explain the origin of the majority of the so-called nuclei (the 35 proton-rich isotopes between Se and Hg). Reaction rates for -process reaction network studies have to be predicted using Hauser-Feshbach statistical model calculations. Recent investigations have shown problems in the prediction of -widths at astrophysical energies which are an essential input for the statistical model. It has an impact on the reliability of abundance predictions in the upper mass range of the nuclei. With the measurement of the Er(,n)Yb reaction cross sections at energies close to the astrophysically relevant energy range we tested the recently suggested low energy modification of the +nucleus optical potential in a mass region where -process calculations exhibit an underproduction of the nuclei. Using the same optical potential for the -width which was derived from combined Er(,n) and Er(,) measurement makes it plausible that a low-energy modification of the optical +nucleus potential is needed.
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- Analysis of uncertainties in alpha-particle optical-potential assessment below the Coulomb barrier
- Experimental study of the astrophysical gamma-process reaction 124Xe(alpha,gamma)128Ba
- Experimental techniques to study the process for nuclear astrophysics at the Cologne accelerator laboratory
- An ERC Starting Grant project on p-process nucleosynthesis concluded