Test of the CRASH experiment counters at GSI

Aglietta, M. and Castagnoli, C. and Castellina, A. and Emling, H. and Fujii, W. and Fujimoto, Y. and Fulgione, W. and Hasebe, T. and Hatano, Y. and Nakamura, T. and Osawa, A. and Saavedra, O. and Saito, T. and Sasaki, H. and Trinchero, G. C. and Vernetto, S. and Vigorito, C. and Yamamoto, K. and Yanagita, T. (1997) Test of the CRASH experiment counters at GSI. Il nuovo cimento C, 20 C (5). pp. 679-684. ISSN 1826-9885

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Abstract

The CRASH (Cosmic RAys and Strange Hadronic matter) balloonborne experiment is specifically designed for the detection of the Strange Quark Matter, which according to theory is probably present in the cosmic-ray radiation at the top of the atmosphere. The detection technique is based on the measure of the AOZ ratio of the nuclei crossing the detector. The charge, the velocity and the mass of the incoming nuclei are determined using both active and passive detectors. First results of the tests of the Cˇerenkov and scintillation counters performed at GSI Darmstadt with heavy ions (Ar and Ni) of different energies are reported.

Item Type: Article
Additional Information: Paper presented at the VII Cosmic Physics National Conference, Rimini, October 26-28, 1994.
Uncontrolled Keywords: Cosmic rays; conference proceedings
Subjects: 500 Scienze naturali e Matematica > 530 Fisica
500 Scienze naturali e Matematica > 550 Scienze della Terra > 551 Geologia, Idrologia, Meteorologia > 551.5 Meteorologia (Classificare qui l'atmosfera) (Classificare la previsione e le previsioni di specifici fenomeni meteorologici in 551.64; classificare la Micrometeorologia in 551.66) > 551.52 Termodinamica, interazioni atmosferiche con la superficie terrestre, temperature, radiazioni > 551.527 Radiazioni (per fenomeni ottici, vedi 551.565) > 551.5276 Radiazioni cosmiche (Include il rumore cosmico) (Classificare qui i raggi cosmici)
Depositing User: Marina Spanti
Date Deposited: 08 Feb 2018 09:49
Last Modified: 08 Feb 2018 09:49
URI: http://eprints.bice.rm.cnr.it/id/eprint/12272

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