Study of GSO scintillator for upgrade of LHCf detectors

K. Kawade; O. Adriani; L. Bonechi; M. Bongi; G. Castellini; R. D'alessandro; K. Fukatsu; M. Haguenauer; Y. Itow; K. Kasahara; D. Macina; T. Mase; K. Masuda; H. Menjo; G. Mitsuka; Y. Muraki; K. Noda; P. Papini; A. L. Perrot; S. Ricciarini; T. Sako; Y. Shimizu; K. Suzuki; T. Suzuki; K. Taki; T. Tamura; Shoji Torii; A. Tricomi; W. C. Turner; K. Yoshida

doi:10.7529/ICRC2011/V05/0959

Study of GSO scintillator for upgrade of LHCf detectors

K. Kawade, O. Adriani, L. Bonechi, M. Bongi, G. Castellini, R. D'alessandro, K. Fukatsu, M. Haguenauer, Y. Itow, K. Kasahara, D. Macina, T. Mase, K. Masuda, H. Menjo, G. Mitsuka, Y. Muraki, K. Noda, P. Papini, A. L. Perrot, S. RicciariniT. Sako, Y. Shimizu, K. Suzuki, T. Suzuki, K. Taki, T. Tamura, Shoji Torii, A. Tricomi, W. C. Turner, K. Yoshida

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

1 Citation (Scopus)

Abstract

Gd₂SiO₅ (GSO) scintillator has very excellent radiation resistance with fast decay time and large amount of light yield. The radiation hardness of GSO was examined by using Carbon ion beams at Heavy Ion Medical Accelerator in Chiba (HIMAC). Through two nights of irradiation a GSO scintillator was received 7 × 10⁵ Gy of total dose and no decrease of light yield was observed. On the other hand an increase of light yield by 25% was observed. The increase is marginally proportional to the total dose at the rate of 0.025%/Gy and it is saturated at 1 kGy. Recovery to the initial light yield was also observed during the day between two nights. The time scale of recovery is about 15,000 seconds. In case of the LHCf experiment, very forward region (pseudo-rapidity > 8.4) experiment at the LHC, the irradiation rate is expected to about 100Gy for 10nb^-1 of data taking at vs = 14TeV proton-proton collisions. Expected increase of less than a few % will not be a big problem for the LHCf experiment.

Original language	English
Title of host publication	Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011
Publisher	Institute of High Energy Physics
Pages	55-58
Number of pages	4
Volume	5
DOIs	https://doi.org/10.7529/ICRC2011/V05/0959
Publication status	Published - 2011
Event	32nd International Cosmic Ray Conference, ICRC 2011 - Beijing Duration: 2011 Aug 11 → 2011 Aug 18

Other

Other	32nd International Cosmic Ray Conference, ICRC 2011
City	Beijing
Period	11/8/11 → 11/8/18

Keywords

GSO scintillator
LHC
Radiation resistivity

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.7529/ICRC2011/V05/0959

Cite this

Kawade, K., Adriani, O., Bonechi, L., Bongi, M., Castellini, G., D'alessandro, R., Fukatsu, K., Haguenauer, M., Itow, Y., Kasahara, K., Macina, D., Mase, T., Masuda, K., Menjo, H., Mitsuka, G., Muraki, Y., Noda, K., Papini, P., Perrot, A. L., ... Yoshida, K. (2011). Study of GSO scintillator for upgrade of LHCf detectors. In Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011 (Vol. 5, pp. 55-58). Institute of High Energy Physics. https://doi.org/10.7529/ICRC2011/V05/0959

Kawade, K, Adriani, O, Bonechi, L, Bongi, M, Castellini, G, D'alessandro, R, Fukatsu, K, Haguenauer, M, Itow, Y, Kasahara, K, Macina, D, Mase, T, Masuda, K, Menjo, H, Mitsuka, G, Muraki, Y, Noda, K, Papini, P, Perrot, AL, Ricciarini, S, Sako, T, Shimizu, Y, Suzuki, K, Suzuki, T, Taki, K, Tamura, T, Torii, S, Tricomi, A, Turner, WC & Yoshida, K 2011, Study of GSO scintillator for upgrade of LHCf detectors. in Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011. vol. 5, Institute of High Energy Physics, pp. 55-58, 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, 11/8/11. https://doi.org/10.7529/ICRC2011/V05/0959

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title = "Study of GSO scintillator for upgrade of LHCf detectors",

abstract = "Gd2SiO5 (GSO) scintillator has very excellent radiation resistance with fast decay time and large amount of light yield. The radiation hardness of GSO was examined by using Carbon ion beams at Heavy Ion Medical Accelerator in Chiba (HIMAC). Through two nights of irradiation a GSO scintillator was received 7 × 105 Gy of total dose and no decrease of light yield was observed. On the other hand an increase of light yield by 25% was observed. The increase is marginally proportional to the total dose at the rate of 0.025%/Gy and it is saturated at 1 kGy. Recovery to the initial light yield was also observed during the day between two nights. The time scale of recovery is about 15,000 seconds. In case of the LHCf experiment, very forward region (pseudo-rapidity > 8.4) experiment at the LHC, the irradiation rate is expected to about 100Gy for 10nb-1 of data taking at vs = 14TeV proton-proton collisions. Expected increase of less than a few % will not be a big problem for the LHCf experiment.",

keywords = "GSO scintillator, LHC, Radiation resistivity",

author = "K. Kawade and O. Adriani and L. Bonechi and M. Bongi and G. Castellini and R. D'alessandro and K. Fukatsu and M. Haguenauer and Y. Itow and K. Kasahara and D. Macina and T. Mase and K. Masuda and H. Menjo and G. Mitsuka and Y. Muraki and K. Noda and P. Papini and Perrot, {A. L.} and S. Ricciarini and T. Sako and Y. Shimizu and K. Suzuki and T. Suzuki and K. Taki and T. Tamura and Shoji Torii and A. Tricomi and Turner, {W. C.} and K. Yoshida",

year = "2011",

doi = "10.7529/ICRC2011/V05/0959",

language = "English",

volume = "5",

pages = "55--58",

booktitle = "Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011",

publisher = "Institute of High Energy Physics",

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AU - Kawade, K.

AU - Adriani, O.

AU - Bonechi, L.

AU - Bongi, M.

AU - Castellini, G.

AU - D'alessandro, R.

AU - Fukatsu, K.

AU - Haguenauer, M.

AU - Itow, Y.

AU - Kasahara, K.

AU - Macina, D.

AU - Mase, T.

AU - Masuda, K.

AU - Menjo, H.

AU - Mitsuka, G.

AU - Muraki, Y.

AU - Noda, K.

AU - Papini, P.

AU - Perrot, A. L.

AU - Ricciarini, S.

AU - Sako, T.

AU - Shimizu, Y.

AU - Suzuki, K.

AU - Suzuki, T.

AU - Taki, K.

AU - Tamura, T.

AU - Torii, Shoji

AU - Tricomi, A.

AU - Turner, W. C.

AU - Yoshida, K.

PY - 2011

Y1 - 2011

N2 - Gd2SiO5 (GSO) scintillator has very excellent radiation resistance with fast decay time and large amount of light yield. The radiation hardness of GSO was examined by using Carbon ion beams at Heavy Ion Medical Accelerator in Chiba (HIMAC). Through two nights of irradiation a GSO scintillator was received 7 × 105 Gy of total dose and no decrease of light yield was observed. On the other hand an increase of light yield by 25% was observed. The increase is marginally proportional to the total dose at the rate of 0.025%/Gy and it is saturated at 1 kGy. Recovery to the initial light yield was also observed during the day between two nights. The time scale of recovery is about 15,000 seconds. In case of the LHCf experiment, very forward region (pseudo-rapidity > 8.4) experiment at the LHC, the irradiation rate is expected to about 100Gy for 10nb-1 of data taking at vs = 14TeV proton-proton collisions. Expected increase of less than a few % will not be a big problem for the LHCf experiment.

AB - Gd2SiO5 (GSO) scintillator has very excellent radiation resistance with fast decay time and large amount of light yield. The radiation hardness of GSO was examined by using Carbon ion beams at Heavy Ion Medical Accelerator in Chiba (HIMAC). Through two nights of irradiation a GSO scintillator was received 7 × 105 Gy of total dose and no decrease of light yield was observed. On the other hand an increase of light yield by 25% was observed. The increase is marginally proportional to the total dose at the rate of 0.025%/Gy and it is saturated at 1 kGy. Recovery to the initial light yield was also observed during the day between two nights. The time scale of recovery is about 15,000 seconds. In case of the LHCf experiment, very forward region (pseudo-rapidity > 8.4) experiment at the LHC, the irradiation rate is expected to about 100Gy for 10nb-1 of data taking at vs = 14TeV proton-proton collisions. Expected increase of less than a few % will not be a big problem for the LHCf experiment.

KW - GSO scintillator

KW - LHC

KW - Radiation resistivity

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DO - 10.7529/ICRC2011/V05/0959

M3 - Conference contribution

AN - SCOPUS:84899569032

VL - 5

SP - 55

EP - 58

BT - Proceedings of the 32nd International Cosmic Ray Conference, ICRC 2011

PB - Institute of High Energy Physics

T2 - 32nd International Cosmic Ray Conference, ICRC 2011

Y2 - 11 August 2011 through 18 August 2011

ER -

Study of GSO scintillator for upgrade of LHCf detectors

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