Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session MB: Quiescent Stellar Burning
2:00 PM–4:30 PM,
Saturday, October 27, 2018
Hilton
Room: Kohala 1
Chair: Frank Strieder, South Dakota School of Mines & Technology
Abstract ID: BAPS.2018.HAW.MB.1
Abstract: MB.00001 : First Measurement of the Neutron Capture Cross Sections of Stable Germanium Isotopes*
2:00 PM–2:15 PM
Presenter:
Alexander Laminack
(Louisiana State Univ - Baton Rouge)
Authors:
Alexander Laminack
(Louisiana State Univ - Baton Rouge)
Jeffery C Blackmon
(Louisiana State Univ - Baton Rouge)
Aaron J Couture
(Los Alamos Natl Lab)
John Leonard Ullmann
(Los Alamos Natl Lab)
Kevin T Macon
(University of Notre Dame)
Ashley A Hood
(Louisiana State Univ - Baton Rouge)
Graeme Morgan
(Louisiana State Univ - Baton Rouge)
Erin Good
(Louisiana State Univ - Baton Rouge)
Scott T Marley
(Louisiana State Univ - Baton Rouge)
Catherine M Deibel
(Louisiana State Univ - Baton Rouge)
Gemma L Wilson
(Louisiana State Univ - Baton Rouge)
Nearly half of all elements heavier than iron are created during the s-process. The s-process can be broken into main and weak components. Because the weak s-process occurs out of statistical equilibrium and the cross sections involved are small, each isotope serves as a bottleneck. Therefore the neutron capture cross sections radically affect the abundance of all isotopes downstream. Almost all stable Germanium isotopes lie along the weak s-process path and yet no neutron time-of-flight measurements of their cross sections have been made. In January 2018, the Detector for Advanced Neutron Capture Experiments (DANCE) at the Los Alamos Neutron Science CEnter (LANSCE) was used to measure the neutron capture cross sections of 70Ge, 72Ge, and 73Ge. A follow up experiment to measure the cross sections of the remaining stable Germanium isotopes at the same facility is planned to occur in the near future. The results of these experiments, the astrophysical impact, and future work based on these results will be discussed.
*This work is supported by the USDOE under grant DE-FG02-96ER40978. This research used resources of LANL's LANSCE facility which is a DOE NNSA user facility.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.MB.1
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