@Article{n_TOFCollaborationLederer-Woods_etal2019,
author="n{\_}TOF Collaboration (Lederer-Woods, C. et al
and Domingo-Pardo, C.
and Tain, J. L.
and Tarife{\~{n}}o-Saldivia, A.",
title="Measurement of Ge-73(n, gamma) cross sections and implications for stellar nucleosynthesis",
journal="Physics Letters B",
year="2019",
publisher="Elsevier Science Bv",
volume="790",
pages="458--465",
optkeywords="Nucleosynthesis; Neutron capture; s process; Germanium; n{\_}TOF",
abstract="Ge-73(n, gamma) cross sections were measured at the neutron time-of-flight facility n{\_}TOF at CERN up to neutron energies of 300 keV, providing for the first time experimental data above 8 keV. Results indicate that the stellar cross section at kT = 30 keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of Ge-73 produced in stars, which would explain the low isotopic abundance of Ge-73 in the solar system.",
optnote="WOS:000460118200058",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3936), last updated on Fri, 07 Jun 2019 07:03:20 +0000",
issn="0370-2693",
doi="10.1016/j.physletb.2019.01.045",
opturl="https://arxiv.org/abs/1901.10207",
opturl="https://doi.org/10.1016/j.physletb.2019.01.045",
language="English"
}