The Ge 76 (n, γ) reaction has been measured at the n_TOF facility at CERN via the time-of-
flight technique. Neutron capture cross sections on Ge 76 are of interest to a variety of low …

One of the critical aspects for the accurate determination of neutron capture cross sections
when combining time-of-flight and total energy detector techniques is the characterization …

Background: Approximately half of all atomic nuclei heavier than iron are synthesized by the
slow neutron-capture process. The weak component of this process is not well understood …

The Se 78 (n, γ) Se 79 cross section has a high impact on the abundances of Se 78
produced during the slow neutron capture process (s process) in massive stars. A …

The 78Se (n, γ) 79Se cross section has a high impact on the abundances of 78Se produced
during the slow neutron capture process (s-process) in massive stars. A measurement of the …

One of the critical aspects for the accurate determination of neutron capture cross sections
when combining time-of-flight and total energy detector techniques is the characterization …

The Se 77 (n, γ) reaction is of importance for Se 77 abundance during the slow neutron
capture process in massive stars. We have performed a new measurement of the Se 77 …

Neutron capture reaction cross sections on 74 Ge are of importance to determine 74 Ge
production during the astrophysical slow neutron capture process. We present new …

Neutron capture reaction cross sections on 74 Ge are of importance to determine 74 Ge
production during the astrophysical slow neutron capture process. We present new …

The slow neutron capture process (s-process) is responsible for producing about half of the
elemental abundances heavier than iron in the universe. Neutron capture cross sections on …