Title :
Simulation study for the higher sensitivity of an Electron-Tracking Compton Camera at over 1 MeV
Author :
Takada, A. ; Tanimori, T. ; Kubo, H. ; Miuchi, K. ; Kabuki, S. ; Parker, J.D. ; Kishimoto, Y. ; Mizumoto, T. ; Ueno, K. ; Kurosawa, S. ; Iwaki, S. ; Sawano, T. ; Taniue, K. ; Nakamura, K. ; Higashi, N. ; Matsuoka, Y. ; Komura, S. ; Sato, Y.
Author_Institution :
RISH, Kyoto Univ., Kyoto, Japan
Abstract :
We have developed an Electron-Tracking Compton Camera (ETCC) as a next-generation MeV gamma-ray telescope. Our detector consists of a gaseous electron tracker as a Compton-scattering target and a position sensitive scintillation camera as a scattered gamma ray absorber. We launched a small size (10 cm cubic) ETCC loaded on a balloon in 2006, and obtained the fluxes of diffuse cosmic and atmospheric gamma rays in the energy range between 125 keV and 1:25 MeV. However, for MeV gamma-ray astronomy, we need to detect the photons at higher energy, thus we must improve the sensitivity of the ETCC in the higher energy range above 1 MeV. For this purpose, we investigate an electron absorber, which is placed between the electron tracker and the photo-absorber. Using Geant4 simulation, we confirmed that the detection energy range is shifted to the range of 0:35-5:0 MeV for the new configuration of the ETCC.
Keywords :
Compton effect; cameras; gamma-ray astronomy; position sensitive particle detectors; scintillation counters; Compton scattering target; ETCC; Geant4 simulation; atmospheric gamma rays; detection energy range; diffuse cosmic rays; electron absorber; electron-tracking Compton camera; gamma-ray astronomy; gaseous electron tracker; next-generation gamma-ray telescope; photoabsorber; position sensitive scintillation camera; scattered gamma ray absorber; Argon; Compton Camera; MeV gamma-ray astronomy; TPC; gaseous detector;
Conference_Titel :
Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC), 2011 IEEE
Conference_Location :
Valencia
Print_ISBN :
978-1-4673-0118-3
DOI :
10.1109/NSSMIC.2011.6154605