In:
EPJ Web of Conferences, EDP Sciences, Vol. 184 ( 2018), p. 02005-
Abstract:
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( n, γ ) 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( n, γ ) 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.
Type of Medium:
Online Resource
ISSN:
2100-014X
DOI:
10.1051/epjconf/201718402005
Language:
English
Publisher:
EDP Sciences
Publication Date:
2018
detail.hit.zdb_id:
2595425-8
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