Bulletin of the American Physical Society
APS April Meeting 2019
Volume 64, Number 3
Saturday–Tuesday, April 13–16, 2019; Denver, Colorado
Session Y12: Nuclear Astrophysics III
1:30 PM–2:42 PM,
Tuesday, April 16, 2019
Sheraton
Room: Plaza Court 1
Sponsoring
Unit:
DNP
Chair: Andrew Steiner, University of Tennessee
Abstract: Y12.00005 : A new measurement of the 17O(α,n)20Ne cross section *
2:18 PM–2:30 PM
Presenter:
Kevin T Macon
(University of Notre Dame)
Authors:
Kevin T Macon
(University of Notre Dame)
Axel Boeltzig
(University of Notre Dame)
Richard J DeBoer
(University of Notre Dame)
Michael T Febbraro
(Oak Ridge National Laboratory)
Qian Liu
(University of Notre Dame)
Rebecca Toomey
(Rutgers University, New Brunswick)
Sean P Burcher
(University of Tennessee)
Rebeka Kelmar
(University of Notre Dame)
August C Gula
(University of Notre Dame)
Jerome Kovoor
(University of Tennessee)
Craig Reingold
(University of Notre Dame)
Shane Moylan
(University of Notre Dame)
Shea Mosby
(Los Alamos National Laboratory)
Kate L Jones
(University of Tennessee)
Michael C F Wiescher
(University of Notre Dame)
Karl Smith
(Los Alamos National Laboratory)
The 17O(α,n) reaction recycles neutrons for the most efficient neutron absorber 16O(n,γ)17O during the core He-burning and shell C-burning phases of the weak s-process. A recent evaluation of previous measurements combined with statistical model calculations by P. Mohr point out a discrepancy in the experimental data. Thus, we have performed (α,nγ) and (α,n) cross section measurements at the 5U accelerator of the Notre Dame Nuclear Science Laboratory. We measured angular distributions of secondary gamma rays from Eα > 1.4 MeV using the HAGRiD (LaBr3:Ce) array and neutrons from 0.8 < Eα < 1.5 MeV with an array of deuterated liquid scintillator detectors. The use of digital electronics allow for pulse shape discrimination in both detector arrays, and spectrum unfolding is used to obtain neutron energy information from the observed light output spectrum in the liquid scintillators. We will present new cross section results from the secondary gamma and neutron measurements.
*National Science Foundation U.S. Department of Energy National Nuclear Security Administration U.S. Department of Energy Office of Nuclear Physics
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