The RICH detector of the AMS-02 experiment: status and physics prospects
/ Authors
R. Pereira, M. Aguilar-Benitez, L. Arruda, F. Barão, B. Baret, A. Barrau, G. Barreira, E. Belmont, J. Berdugo, J. Borges
and 30 more authors
M. Buénerd, D. Casadei, J. Casaus, E. Cortina, M. Costado, D. Crespo, C. Delgado, C. Díaz, L. Derome, P. Gonçalves, R. García-López, C. D. Guía, A. Herrero, E. Lanciotti, G. Laurenti, A. Malinin, C. Mañá, J. Marin, M. Mangin-Brinet, G. Martinez, A. Menchaca-Rocha, C. Palomares, M. Pimenta, A. Putze, Y. Sallaz-Damaz, E. Seo, I. Sevilla, A. Torrentó, M. Vargas-Treviño, O. Veziant
/ Abstract
The Alpha Magnetic Spectrometer (AMS), whose final version AMS-02 is to be installed on the International Space Station (ISS) for at least 3 years, is a detector designed to measure charged cosmic ray spectra with energies up to the TeV region and with high energy photon detection capability up to a few hundred GeV. It is equipped with several subsystems, one of which is a proximity focusing RICH detector with a dual radiator (aerogel+NaF) that provides reliable measurements for particle velocity and charge. The assembly and testing of the AMS RICH is currently being finished and the full AMS detector is expected to be ready by the end of 2008. The RICH detector of AMS-02 is presented. Physics prospects are briefly discussed.
Journal: arXiv: Astrophysics