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

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dc.contributor.authorUribe Estrada, C.-
dc.contributor.authorCarpinteyro Bernardino, S.-
dc.contributor.authorCastaneda Hernandez, A.-
dc.contributor.authorFagot, A.-
dc.contributor.authorGul, M.-
dc.contributor.authorRoskas, C.-
dc.contributor.authorTytgat, M.-
dc.contributor.authorZaganidis, N.-
dc.contributor.authorFonseca De Souza, S.-
dc.contributor.authorSantoro, A.-
dc.contributor.authorDa Silva De Araujo, F. Torres-
dc.contributor.authorAleksandrov, A.-
dc.contributor.authorHadjiiska, R.-
dc.contributor.authorIaydjiev, P.-
dc.contributor.authorRodozov, M.-
dc.contributor.authorShopova, M.-
dc.contributor.authorSultanov, G.-
dc.contributor.authorDimitrov, A.-
dc.contributor.authorLitov, L.-
dc.contributor.authorPavlov, B.-
dc.contributor.authorPetkov, P.-
dc.contributor.authorPetrov, A.-
dc.contributor.authorQian, S. J.-
dc.contributor.authorHan, D.-
dc.contributor.authorYi, W.-
dc.contributor.authorAvila, C.-
dc.contributor.authorCabrera, A.-
dc.contributor.authorCarrillo, C.-
dc.contributor.authorSegura, M.-
dc.contributor.authorAly, S.-
dc.contributor.authorAssran, Y.-
dc.contributor.authorMahrous, A.-
dc.contributor.authorMohamed, A.-
dc.contributor.authorCombaret, C.-
dc.contributor.authorGouzevitch, M.-
dc.contributor.authorGrenier, G.-
dc.contributor.authorLagarde, F.-
dc.contributor.authorLaktineh, I. B.-
dc.contributor.authorMathez, H.-
dc.contributor.authorMirabito, L.-
dc.contributor.authorShchablo, K.-
dc.contributor.authorBagaturia, I.-
dc.contributor.authorLomidze, D.-
dc.contributor.authorLomidze, I.-
dc.contributor.authorPant, L. M.-
dc.contributor.authorBhatnagar, V.-
dc.contributor.authorGupta, R.-
dc.contributor.authorKumari, R.-
dc.contributor.authorLohan, M.-
dc.contributor.authorSingh, J. B.-
dc.contributor.authorAmoozegar, V.-
dc.contributor.authorBoghrati, B.-
dc.contributor.authorGhasemy, H.-
dc.contributor.authorMalmir, S.-
dc.contributor.authorNajafabadi, M. Mohammadi-
dc.contributor.authorAbbrescia, M.-
dc.contributor.authorGelmi, A.-
dc.contributor.authorIaselli, G.-
dc.contributor.authorLezki, S.-
dc.contributor.authorPugliese, G.-
dc.contributor.authorBenussi, L.-
dc.contributor.authorBianco, S.-
dc.contributor.authorPiccolo, D.-
dc.contributor.authorPrimavera, F.-
dc.contributor.authorBuontempo, S.-
dc.contributor.authorCrescenzo, A.-
dc.contributor.authorGalati, G.-
dc.contributor.authorFienaga, F.-
dc.contributor.authorOrso, I.-
dc.contributor.authorLista, L.-
dc.contributor.authorMeola, S.-
dc.contributor.authorPaolucci, P.-
dc.contributor.authorVoevodina, E.-
dc.contributor.authorBraghieri, A.-
dc.contributor.authorMontagna, P.-
dc.contributor.authorRessegotti, M.-
dc.contributor.authorRiccardi, C.-
dc.contributor.authorSalvini, P.-
dc.contributor.authorVitulo, P.-
dc.contributor.authorCho, S. W.-
dc.contributor.authorChoi, S. Y.-
dc.contributor.authorHong, B.-
dc.contributor.authorLee, K. S.-
dc.contributor.authorLim, J. H.-
dc.contributor.authorPark, S. K.-
dc.contributor.authorGoh, J.-
dc.contributor.authorKim, T. J.-
dc.contributor.authorMoreno, S. Carrillo-
dc.contributor.authorColin, O. Miguel-
dc.contributor.authorValencia, F. Vazquez-
dc.contributor.authorEysermans, J.-
dc.contributor.authorPedraza, I.-
dc.contributor.authorReyes-Almanza, R.-
dc.contributor.authorDuran-Osuna, M. C.-
dc.contributor.authorRamirez-Garcia, M.-
dc.contributor.authorRamirez-Sanchez, G.-
dc.contributor.authorSanchez-Hernandez, A.-
dc.contributor.authorRabadan-Trejo, R. I.-
dc.contributor.authorCastilla-Valdez, H.-
dc.contributor.authorRadi, A.-
dc.contributor.authorHoorani, H.-
dc.contributor.authorMuhammad, S.-
dc.contributor.authorShah, M. A.-
dc.contributor.authorCrotty, I.-
dc.date.accessioned2022-07-09T09:26:33Z-
dc.date.available2022-07-09T09:26:33Z-
dc.date.created2021-05-11-
dc.date.issued2019-09-
dc.identifier.issn1748-0221-
dc.identifier.urihttps://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/147257-
dc.description.abstractThe 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.-
dc.language영어-
dc.language.isoen-
dc.publisherIOP PUBLISHING LTD-
dc.titleRPC radiation background simulations for the high luminosity phase in the CMS experiment-
dc.typeArticle-
dc.contributor.affiliatedAuthorKim, T. J.-
dc.identifier.doi10.1088/1748-0221/14/09/C09045-
dc.identifier.scopusid2-s2.0-85074409352-
dc.identifier.wosid000519117900008-
dc.identifier.bibliographicCitationJOURNAL OF INSTRUMENTATION, v.14, no.9, pp.1 - 8-
dc.relation.isPartOfJOURNAL OF INSTRUMENTATION-
dc.citation.titleJOURNAL OF INSTRUMENTATION-
dc.citation.volume14-
dc.citation.number9-
dc.citation.startPage1-
dc.citation.endPage8-
dc.type.rimsART-
dc.type.docTypeArticle; Proceedings Paper-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaInstruments & Instrumentation-
dc.relation.journalWebOfScienceCategoryInstruments & Instrumentation-
dc.subject.keywordPlusLuminance-
dc.subject.keywordPlusParticle spectrometers-
dc.subject.keywordPlusDetector materials-
dc.subject.keywordPlusDetector performance-
dc.subject.keywordPlusMuon spectrometer-
dc.subject.keywordPlusOperating condition-
dc.subject.keywordPlusRadiation background-
dc.subject.keywordPlusRadiation calculations-
dc.subject.keywordPlusRadiation environments-
dc.subject.keywordPlusSimulation studies-
dc.subject.keywordPlusRadioactivity-
dc.subject.keywordAuthorMuon spectrometers-
dc.subject.keywordAuthorRadiation calculations-
dc.subject.keywordAuthorModels and simulations-
dc.identifier.urlhttps://iopscience.iop.org/article/10.1088/1748-0221/14/09/C09045-
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