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 HA: Conference Experience for Undergraduates Poster Session (2:00pm - 3:45pm)
2:00 PM,
Friday, October 26, 2018
Hilton
Room: Grand Promenade
Abstract ID: BAPS.2018.HAW.HA.73
Abstract: HA.00073 : New Level Structure of 162,164Gd*
Presenter:
Christian Ross Brown
(Union University, Vanderbilt University)
Authors:
Christian Ross Brown
(Union University, Vanderbilt University)
Jonathan Mark Eldridge
(Vanderbilt University)
Enhong Wang
(Vanderbilt University)
Christopher J Zachary
(Vanderbilt University)
Akunuri V Ramayya
(Vanderbilt University)
Joseph H Hamilton
(Vanderbilt University)
Brooks M Musangu
(Vanderbilt University)
Thomas Henry Richards
(University of Alabama, Vanderbilt University)
Yixiao Luo
(Lawrence Berkeley National Laboratory, Vanderbilt University)
John Ramussen
(Lawrence Berkeley National Laboratory)
Shengjiang Zhu
(Tsinghua University)
Gurgen M Ter-Akopian
(Joint Institute for Nuclear Research)
Yuri Oganessian
(Joint Institute for Nuclear Research)
Levels in 162,164Gd were constructed via γ-γ-γ and γ-γ-γ-γ coincidence data from observations of 252Cf spontaneous fission. γ-rays from fission events of a 62 μCi 252Cf source were measured in the center of the Gammasphere detector array. This produced 5.7x1011 γ-γ-γ or higher coincidence events and 1.9x1011 γ-γ-γ-γ or higher coincidence events. This data set was analyzed to construct new energy level schemes for 162,164Gd. Levels and transitions previously identified in the ground state rotational bands have been confirmed. Additionally, several new transitions and levels are observed in both isotopes, including the establishment of a γ vibrational band from 2+ to 9+ for the first time, and the addition of a level in the yrast band of 162Gd.
*U.S. DOE Grant DE-FG05-88ER40407.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.HA.73
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