Stellar s-process neutron capture cross sections of Ga69,71

M. Tessler, M. Paul, S. Halfon, Y. Kashiv, D. Kijel, A. Kreisel, A. Shor, and L. Weissman
Phys. Rev. C 105, 035801 – Published 8 March 2022

Abstract

The stable gallium isotopes, Ga69,71, are mostly produced by the weak slow (s) process in massive stars. We report here on measurements of astrophysically relevant neutron capture cross sections of the Ga69,71(n,γ) reactions. The experiments were performed by the activation technique using a high-intensity (35×1010 n/s), quasi-Maxwellian neutron beam that closely mimics conditions of stellar s-process nucleosynthesis at kT 40 keV. The neutron field was produced by a mA proton beam at Ep=1925 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 Ga2O3 of natural isotopic composition was activated in the LiLiT neutron field and the activities of Ga70,72 were measured by decay counting via γ spectrometry with a high-purity germanium detector. The Maxwellian-averaged cross sections at kT=30keV of Ga69 and Ga71 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.

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  • Received 10 September 2021
  • Revised 29 November 2021
  • Accepted 2 February 2022

DOI:https://doi.org/10.1103/PhysRevC.105.035801

©2022 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

M. Tessler1,2,*, M. Paul2, S. Halfon1, Y. Kashiv3, D. Kijel1, A. Kreisel1, A. Shor1, and L. Weissman1

  • 1Soreq Nuclear Research Center, Yavne 81800, Israel
  • 2Racah Institute of Physics, Hebrew University, Jerusalem 91904, Israel
  • 3University of Notre Dame, Notre Dame, Indiana 46556, USA

  • *Corresponding author: moshe.tessler@mail.huji.ac.il

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Vol. 105, Iss. 3 — March 2022

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