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18–23 Aug 2024
Whistler Conference Centre
America/Vancouver timezone
Proceedings deadline: OCTOBER 18, 2024

Demonstration of Nuclear Gamma-Ray Polarimetry Based on a Multi-Layer CdTe Compton Camera

21 Aug 2024, 09:35
15m
Harmony B

Harmony B

Contributed Oral Instrumentation and Facilities Applications, Facilities & Instrumentation

Speaker

Shintaro Go (RIKEN Cluster for Pioneering Research, RIKEN)

Description

To detect and track structural changes in atomic nuclei, the systematic study of nuclear levels with firm spin-parity assignments is important. While linear polarization measurements have been applied to determine the electromagnetic character of gamma-ray transitions, the applicable range is strongly limited due to the low efficiency of the detection system.The multi-layer Cadmium-Telluride (CdTe) Compton camera can be a state-of-the-art gamma-ray polarimeter for nuclear spectroscopy with the high position sensitivity and the detection efficiency. We demonstrated the capability to operate this detector as a reliable gamma-ray polarimeter by using polarized 847-keV gamma rays produced by the $^{56}\rm{Fe}({\it p},{\it p'}\gamma)$ reaction [1]. By combining the experimental data and simulated calculations, the modulation curve for the gamma ray was successfully obtained. A remarkably high polarization sensitivity was achieved, compatible with a reasonable detection efficiency. Based on the obtained results, a possible future gamma-ray polarimetery is discussed in the presentation.
[1] S. Go et al., accepted in Scientific Reports (2023) DOI: 10.1038/s41598-024-52692-2

Email Address go@riken.jp

Primary author

Shintaro Go (RIKEN Cluster for Pioneering Research, RIKEN)

Co-authors

Aiko Takamine (RIKEN Cluster for Pioneering Research, RIKEN) Daiki Nishimura (Department of Natural Sciences, Tokyo City University) Hideki Ueno (RIKEN Cluster for Pioneering Research, RIKEN) Hiroki Yoneda (Julius-Maximilians-Universit\"{a}t W\"{u}rzburg, Fakult\"{a}t f\"{u}r Physik und Astronomie, Institut f\"{u}r Theoretische Physik und Astrophysik, Lehrstuhl f\"{u}r Astronomie) Kei Imamura (RIKEN Cluster for Pioneering Research, RIKEN) Megumi Niikura (RIKEN Nishina Center for Accelerator-Based Science) Nobuaki Imai (Center for Nuclear Study, the University of Tokyo) Rurie Mizuno (Department of Physics, The University of Tokyo) Shin Watanabe (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) Shinichiro Takeda (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo) Susumu Shimoura (Center for Nuclear Study, the University of Tokyo, Saitama, Japan) Tadayuki Takahashi (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo) Takeshi Saito (Center for Nuclear Study, the University of Tokyo, Saitama, Japan) Tokihiro Ikeda (RIKEN Nishina Center for Accelerator-Based Science, RIKEN) Yuichi Ichikawa (Department of Physics, Kyushu University) Yutaka Tsuzuki (RIKEN Cluster for Pioneering Research, RIKEN)

Presentation materials