The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universo.
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April 1, 2020 (v1)PublicationUploaded on: March 25, 2023
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June 11, 2021 (v1)Publication
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 stable isotopes are a key nuclear physics input for s-process studies. The 72Ge(n, γ) cross section has an important influence on production of isotopes between Ge...
Uploaded on: December 4, 2022 -
February 7, 2022 (v1)Publication
The 72 Ge ( 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 72 Ge O 2 ...
Uploaded on: March 25, 2023