RPC radiation background simulations for the high luminosity phase in the CMS experiment

C. Uribe Estrada,S. Carpinteyro Bernardino,A. Castaneda Hernandez,A. Fagot,M. Gul,C. Roskas, M. Tytgat, N. Zaganidis,S. Fonseca De Souza, A. Santoro,F. Torres Da Silva De Araujo, A. Aleksandrov,R. Hadjiiska, P. Iaydjiev,M. Rodozov,M. Shopova, G. Sultanov, A. Dimitrov,L. Litov,B. Pavlov,P. Petkov,A. Petrov, S.J. Qian,D. Han W. Yi,C. Avila,A. Cabrera,C. Carrillo, M. Segura,S. Aly,Y. Assran,A. Mahrous,A. Mohamed,C. Combaret, M. Gouzevitch, G. Grenier, F. Lagarde, I.B. Laktineh,H. Mathez, L. Mirabito,K. Shchablo,I. Bagaturia,D. Lomidze,I. Lomidze, L.M. Pant,V. Bhatnagar,R. Gupta,R. Kumari,M. Lohan, J.B. Singh,V. Amoozegar,B. Boghrati,H. Ghasemy,S. Malmir,M. Mohammadi Najafabadi,M. Abbrescia, A. Gelmi,G. Iaselli,S. Lezki,G. Pugliese, L. Benussi,S. Bianco, D. Piccolo, F. Primavera, S. Buontempo,A. Crescenzo,G. Galati, F. Fienaga,I. Orso, L. Lista, S. Meola,P. Paolucci,E. Voevodina, A. Braghieri, P. Montagna, M. Ressegotti,C. Riccardi, P. Salvini,P. Vitulo, S. W. Cho,S. Y. Choi,B. Hong,K. S. Lee,J. H. Lim, S. K. Park,J. Goh, T. J. Kim,S. Carrillo Moreno,O. Miguel Colin,F. Vazquez Valencia, J. Eysermans, I. Pedraza, R. Reyes-Almanza, M.C. Duran-Osuna,M. Ramirez-Garcia,G. Ramirez-Sanchez,A. Sanchez-Hernandez, R.I. Rabadan-Trejo, H. Castilla-Valdez,A. Radi,H. Hoorani,S. Muhammad,M.A. Shah,I. Crotty

JOURNAL OF INSTRUMENTATION(2019)

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摘要
The high luminosity expected from the HL-LHC will be a challenge for the CMS detector. The increased rate of particles coming from the collisions and the radioactivity induced in the detector material could cause significant damage and result in a progressive degradation of its performance. Simulation studies are very useful in these scenarios as they allow one to study the radiation environment and the impact on detector performance. Results are presented for CMS RPC stations considering the operating conditions expected at the HL-LHC.
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关键词
Muon spectrometers,Radiation calculations,Models and simulations
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