@misc{10481/68951,
year = {2021},
month = {4},
url = {http://hdl.handle.net/10481/68951},
abstract = {The 72Ge(n, γ ) cross section was measured for neutron energies up to 300 keV at the neutron time-of-flight
facility n_TOF (CERN), Geneva, for the first time covering energies relevant to heavy-element synthesis in stars.
The measurement was performed at the high-resolution beamline EAR-1, using an isotopically enriched 72GeO2
sample. The prompt capture γ rays were detected with four liquid scintillation detectors, optimized for low
neutron sensitivity. We determined resonance capture kernels up to a neutron energy of 43 keV, and averaged
cross sections from 43 to 300 keV. Maxwellian-averaged cross section values were calculated from kT = 5
to 100 keV, with uncertainties between 3.2% and 7.1%. The new results significantly reduce uncertainties of
abundances produced in the slow neutron capture process in massive stars.},
organization = {Adolf Messer Foundation},
organization = {Austrian Science Fund (FWF)

J 3503},
organization = {UK Research & Innovation (UKRI)

Science & Technology Facilities Council (STFC)

ST/M006085/1},
organization = {European Research Council (ERC)},
organization = {European Commission

677497},
organization = {Croatian Science Foundation 

8570},
organization = {Ministry of Education, Youth & Sports - Czech Republic},
organization = {Charles University 

UNCE/SCI/013},
publisher = {American Physical Society},
title = {Measurement of the 72Ge(n, γ) cross section over a wide neutron energy range at the CERN n_TOF facility},
doi = {10.1103/PhysRevC.103.045809},
author = {Dietz, M. and Porras Sánchez, José Ignacio and Praena Rodríguez, Antonio Javier and TOF Collaboration},
}