291 citations · 1.9k across the 61 of their papers we have counts for
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High precision In()In elastic scattering at energies around the Coulomb barrier for the astrophysical process
G. G. Kiss, P. Mohr, Zs. Fülöp +9
The process in supernova explosions is thought to explain the origin of proton-rich isotopes between Se and Hg, the so-called nuclei. The majority of the reaction rates for…
Measurement of the Zr(p,)Nb reactions for the nucleosynthesis of elements around A=90
A. Spyrou, S. J. Quinn, A. Simon +24
Cross section measurements of the reactions Zr(p,)Nb were performed using the NSCL SuN detector at the University of Notre Dame. These reactions are part of…
Nuclear astrophysics with radioactive ions at FAIR
R. Reifarth, S. Altstadt, K. Göbel +317
The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those proces…
Revision of the derivation of stellar rates from experiment and impact on Eu s-process contributions
T. Rauscher
A new, general formalism to include experimental data in revised stellar rates is discussed, containing revised uncertainties. Application to the s-process shows that the actual un…
Suppression of Excited-State Contributions to Stellar Reaction Rates
T. Rauscher
It has been shown in previous work [Phys. Rev. Lett. 101, 191101 (2008); Phys. Rev. C 80, 035801 (2009)] that a suppression of the stellar enhancement factor (SEF) occurs in some e…
Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data
T. Rauscher, N. Dauphas, I. Dillmann +3
A small number of naturally occurring, proton-rich nuclides (the p-nuclei) cannot be made in the s- and r-process. Their origin is not well understood. Massive stars can produce p-…