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 DG: Mini-Symposium on Fundamental Symmetries (Many-body Systems) II
9:00 AM–10:45 AM,
Thursday, October 25, 2018
Hilton
Room: King's 3
Chair: John Behr, TRIUMF
Abstract ID: BAPS.2018.HAW.DG.2
Abstract: DG.00002 : Branching-Ratio Measurements for Superallowed β Emitters at NIRS-HIMAC*
9:15 AM–9:30 AM
Presenter:
Daiki Nishimura
(Dept. of Physics, Tokyo City University)
Authors:
Daiki Nishimura
(Dept. of Physics, Tokyo City University)
Mitsunori Fukuda
(Dept. of Physics, Osaka Univ.)
Akira Honma
(Dept. of Physics, Niigata Univ.)
Yuichi Ichikawa
(RIKEN Nishina Center/Tokyo Tech.)
Atsushi Kitagawa
(QST)
Kensaku Matsuta
(Dept. of Physics, Osaka Univ.)
Mototsugu Mihara
(Dept. of Physics, Osaka Univ.)
Takashi Ohtsubo
(Dept. of Physics, Niigata Univ.)
Masaomi Tanaka
(Dept. of Physics, Osaka Univ.)
Shinji Sato
(QST)
The ft values for the superallowed 0+ → 0+ Fermi β decays provide valuable information on the CVC hypothesis, the unitarity of CKM matrix, and the isospin-symmetry breaking. The ft values for the 13 superallowed β emitters have been already determined very precisely. However, the emitters of 18Ne and 30S have not been determined yet due to large uncertainties of the branching ratios. Because they have the β feeding to both of the excited states including the 0+ state and the ground state, we have to measure not relative gamma intensities but absolute ones. The new precise branching-ratio measurement system is being developed. Our test measurement was carried out at NIRS-HIMAC. The secondary beam including 18Ne(30S) was produced with the projectile fragmentation reaction of 20Ne(36Ar) on a polyethylene target. The beam was separated and identified by passing through the secondary beam line and was implanted in a 6-mm-thick GSO active stopper surrounded by four clover Ge detectors. The β particles and γ rays were detected by the GSO stopper and the Ge detectors, respectively. We will report the current status of our results and a future plan to improve performance with movable active stoppers.
*This work is supported by JSPS KAKENHI Grant Number 17H14299.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.DG.2
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