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Go S, Tsuzuki Y, Yoneda H, Ichikawa Y, Ikeda T, Imai N, Imamura K, Niikura M, Nishimura D, Mizuno R, Takeda S, Ueno H, Watanabe S, Saito TY, Shimoura S, Sugawara S, Takamine A, Takahashi T. Demonstration of nuclear gamma-ray polarimetry based on a multi-layer CdTe Compton camera. Sci Rep 2024; 14:2573. [PMID: 38336981 PMCID: PMC11294463 DOI: 10.1038/s41598-024-52692-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/05/2023] [Accepted: 01/22/2024] [Indexed: 02/12/2024] Open
Abstract
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 [Formula: see text]([Formula: see text]) reaction. 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.
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Affiliation(s)
- S Go
- RIKEN Cluster for Pioneering Research, RIKEN, Wako, Saitama, Japan.
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan.
| | - Y Tsuzuki
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
- Department of Physics, The University of Tokyo, Tokyo, Japan
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Chiba, Japan
| | - H Yoneda
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
- Lehrstuhl für Astronomie, Fakultät für Physik und Astronomie, Institut für Theoretische Physik und Astrophysik, Julius-Maximilians-Universität Würzburg, Emil-Fischer-Str. 31, 97074, Würzburg, Germany
| | - Y Ichikawa
- Department of Physics, Kyushu University, Fukuoka, Japan
| | - T Ikeda
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
| | - N Imai
- Center for Nuclear Study, The University of Tokyo, Wako, Saitama, Japan
| | - K Imamura
- RIKEN Cluster for Pioneering Research, RIKEN, Wako, Saitama, Japan
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
| | - M Niikura
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
| | - D Nishimura
- Department of Natural Sciences, Tokyo City University, Tokyo, Japan
| | - R Mizuno
- Department of Physics, The University of Tokyo, Tokyo, Japan
| | - S Takeda
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Chiba, Japan
| | - H Ueno
- RIKEN Cluster for Pioneering Research, RIKEN, Wako, Saitama, Japan
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
| | - S Watanabe
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Kanagawa, Japan
| | - T Y Saito
- Center for Nuclear Study, The University of Tokyo, Wako, Saitama, Japan
- Atomic, Molecular, and Optical Physics Laboratory, RIKEN, Wako, Saitama, Japan
| | - S Shimoura
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
- Center for Nuclear Study, The University of Tokyo, Wako, Saitama, Japan
| | - S Sugawara
- Department of Natural Sciences, Tokyo City University, Tokyo, Japan
| | - A Takamine
- RIKEN Cluster for Pioneering Research, RIKEN, Wako, Saitama, Japan
- RIKEN Nishina Center for Accelerator-Based Science, RIKEN, Wako, Saitama, Japan
| | - T Takahashi
- Department of Physics, The University of Tokyo, Tokyo, Japan
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo, Chiba, Japan
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Parajuli RK, Sakai M, Parajuli R, Tashiro M. Development and Applications of Compton Camera-A Review. SENSORS (BASEL, SWITZERLAND) 2022; 22:7374. [PMID: 36236474 PMCID: PMC9573429 DOI: 10.3390/s22197374] [Citation(s) in RCA: 7] [Impact Index Per Article: 3.5] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 08/11/2022] [Revised: 09/08/2022] [Accepted: 09/20/2022] [Indexed: 06/16/2023]
Abstract
The history of Compton cameras began with the detection of radiation sources originally for applications in astronomy. A Compton camera is a promising γ-ray detector that operates in the wide energy range of a few tens of keV to MeV. The γ-ray detection method of a Compton camera is based on Compton scattering kinematics, which is used to determine the direction and energy of the γ-rays without using a mechanical collimator. Although the Compton camera was originally designed for astrophysical applications, it was later applied in medical imaging as well. Moreover, its application in environmental radiation measurements is also under study. Although a few review papers regarding Compton cameras have been published, they either focus very specifically on the detectors used in such cameras or the particular applications of Compton cameras. Thus, the aim of this paper is to review the features and types of Compton cameras and introduce their applications, associated imaging algorithms, improvement scopes, and their future aspects.
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Affiliation(s)
- Raj Kumar Parajuli
- Department of Molecular Imaging and Theranostics, National Institutes for Quantum Science and Technology, 4-9-1 Anagawa, Inage, Chiba 263-8555, Japan
- Gunma University Heavy Ion Medical Center, Gunma University, 3-39-22 Showa-machi, Maebashi 371-8511, Japan
| | - Makoto Sakai
- Gunma University Heavy Ion Medical Center, Gunma University, 3-39-22 Showa-machi, Maebashi 371-8511, Japan
| | | | - Mutsumi Tashiro
- Gunma University Heavy Ion Medical Center, Gunma University, 3-39-22 Showa-machi, Maebashi 371-8511, Japan
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Compton imaging for medical applications. Radiol Phys Technol 2022; 15:187-205. [PMID: 35867197 DOI: 10.1007/s12194-022-00666-2] [Citation(s) in RCA: 10] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/04/2022] [Revised: 07/04/2022] [Accepted: 07/04/2022] [Indexed: 12/18/2022]
Abstract
Compton imaging exploits inelastic scattering, known as Compton scattering, using a Compton camera consisting of a scatterer detector in the front layer and an absorber detector in the back layer. This method was developed for astronomy, and in recent years, research and development for environmental and medical applications has been actively conducted. Compton imaging can discriminate gamma rays over a wide energy range from several hundred keV to several MeV. Therefore, it is expected to be applied to the simultaneous imaging of multiple nuclides in nuclear medicine and prompt gamma ray imaging for range verification in particle therapy. In addition, multiple gamma coincidence imaging is expected to be realized, which allows the source position to be determined from a single coincidence event using nuclides that emit multiple gamma rays simultaneously, such as nuclides that emit a single gamma ray simultaneously with positron decay. This review introduces various efforts toward the practical application of Compton imaging in the medical field, including in vivo studies, and discusses its prospects.
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