@misc{10481/62028,
year = {2019},
url = {http://hdl.handle.net/10481/62028},
abstract = {73Ge(n, γ) cross sections were measured at the neutron time-of-flight facility n_TOF at CERN up to neutron energies of 300keV, providing for the first time experimental data above 8keV. Results indicate that the stellar cross section at kT=30keV is 1.5 to 1.7 times higher than most theoretical predictions. The new cross sections result in a substantial decrease of 73Ge produced in stars, which would explain the low isotopic abundance of 73Ge in the solar system.},
organization = {This work was supported by the Austrian Science Fund FWF (J3503), the Adolf Messer Foundation (Germany), the UK Science and Facilities Council (ST/M006085/1), and the European Research Council ERC-2015-StG Nr.677497.},
publisher = {Elsevier Inc.},
keywords = {Nucleosynthesis},
keywords = {Neutron capture},
keywords = {Germanium},
title = {Measurement of 73Ge(n,γ) cross sections and implications for stellar nucleosynthesis},
doi = {10.1016/j.physletb.2019.01.045},
author = {Porras Sánchez, José Ignacio and Lederer Woods, C.},
}