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 DP: The r-process
9:00 AM–11:45 AM,
Thursday, October 25, 2018
Hilton
Room: Kona 1
Chair: Anna Simon, University of Notre Dame
Abstract ID: BAPS.2018.HAW.DP.11
Abstract: DP.00011 : Structure of 135Xe from the (d,pγ) reaction with 134Xe beams and GODDESS*
11:30 AM–11:45 AM
Presenter:
Alexandre Lepailleur
(Rutgers University)
Authors:
Alexandre Lepailleur
(Rutgers University)
Jolie Antonia Cizewski
(Rutgers University)
Heather I Garland
(Rutgers University)
Harrison E Sims
(Rutgers University)
David G Walter
(Rutgers University)
Andrew Ratkiewicz
(Lawrence Livermore Natl Lab)
Travis Ray Baugher
(Los Alamos National Laboratory)
Michael T Febbraro
(Oak Ridge National Lab)
Steven D. Pain
(Oak Ridge National Lab)
Karl Smith
(University of Tennessee Knoxville)
About half of the elements heavier than iron are synthesized during the r-process that proceeds via (n,γ) reactions on neutron-rich nuclei. Direct-semidirect neutron captures are important, if not dominant, near the N=82 closed shell and are expected to have a significant impact during the late stages of the r-process, for example through 130Sn(n,γ)131Sn. Therefore, the evolution of the shell gap at N=82 and the single neutron 3p3/2 and 3p1/2 states are keys to a better understanding of the r-process and for constraining model parameters. To probe the 2f-3p single-neutron configurations in the N=81 isotone 135Xe, we have measured the 134Xe(d,pγ)135Xe reaction in inverse kinematics using GODDESS (Gammasphere ORRUBA: Dual Detectors for Experimental Structure Studies). The 134Xe beam was produced at ATLAS (Argonne National Laboratory) and impinged on a C2D4 target. Reaction protons were measured (ORRUBA) in coincidence with gamma rays (Gammasphere). Several single-neutron states, corresponding to the transfer of a neutron to the p-f configurations above the N=82 shell gap, have been observed for the first time.
In collaboration with the GODDESS team.
*This work is supported in part by the U.S. Department of Energy and National Science Foundation.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.DP.11
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