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First Measurement of $^{72}$Ge$(n,γ)$ at n_TOF
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 $^{72}$Ge($\eta, \gamma$) cross section has...
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Lenguaje: | eng |
Publicado: |
2018
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1051/epjconf/201718402005 http://cds.cern.ch/record/2677365 |
Sumario: | 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 $^{72}$Ge($\eta, \gamma$) cross section has an important influence on production of isotopes between Ge and Zr during s-process in massive stars and therefore experimental data are urgently required. $^{72}$Ge($\eta, \gamma$) was measured at the neutron time-of-flight facility n_TOF (CERN) for the first time at stellar energies. The measurement was performed using an enriched $^{72}$GeO$_2$ sample at a flight path of 185m with a set of liquid scintillation detectors (C$_6$D$_6$). The motivation, experiment and current status of the data analysis are reported. |
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