Study of GSO scintillator for the LHCf upgrade
- Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya (Japan)
- Research Institute for Science and Engineering, Waseda University, Tokyo (Japan)
- Universita degli Studi di Firenze and INFN Sezione di Firenze, Firenze (Italy)
- INFN Sezione di Firenze, Firenze (Italy)
The GSO scintillator has a very excellent radiation resistance, fast decay time and large amounts of light yield. Because of these features, GSO will be used to upgrade the current LHCf detector. We examined the features of GSO by using heavy ion beam at Heavy Ion Medical Accelerator in Chiba (HIMAC) Japan. The linearity of PMT R7400 for the large light yield of GSO with a {sup 132}Xe beam and the radiation hardness with a {sup 12}C beam were measured. As a result, GSO scintillator showed a good linearity up to the signal corresponding to 6 TeV EM-shower maximum in the LHCf detector, and a good radiation hardness up to 7x10{sup 5} Gy. For the LHCf Arm1 detector, small scaled GSO crystals (GSO bars), have been fabricated for the position determination detector. 5 GSO bars have been manufactured and its performance have been evaluated using {sup 12}C beam. Its light yield and position dependency have been evaluated.
- OSTI ID:
- 21608329
- Journal Information:
- AIP Conference Proceedings, Vol. 1367, Issue 1; Conference: International symposium on the recent progress of ultra-high energy cosmic ray observation, Aichi (Japan), 10-12 Dec 2010; Other Information: DOI: 10.1063/1.3628750; (c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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