Abstract
The stable gallium isotopes, , are mostly produced by the weak slow () process in massive stars. We report here on measurements of astrophysically relevant neutron capture cross sections of the reactions. The experiments were performed by the activation technique using a high-intensity ( n/s), quasi-Maxwellian neutron beam that closely mimics conditions of stellar -process nucleosynthesis at 40 keV. The neutron field was produced by a mA proton beam at keV (beam power of 2–3 kW) from the Soreq Applied Research Accelerator Facility (SARAF), bombarding the liquid-lithium target (LiLiT). A 473-mg sample of of natural isotopic composition was activated in the LiLiT neutron field and the activities of were measured by decay counting via spectrometry with a high-purity germanium detector. The Maxwellian-averaged cross sections at of and determined in this work are 136(8) and 105(7) mb, respectively, in good agreement with previous experimental values. Astrophysical implications of the measurements are discussed.
3 More- Received 10 September 2021
- Revised 29 November 2021
- Accepted 2 February 2022
DOI:https://doi.org/10.1103/PhysRevC.105.035801
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