Electron-muon identification by atmospheric shower in a new concept of an EAS detector

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dc.authorid0000-0001-5963-8306en_US
dc.authorid0000-0001-9856-9155en_US
dc.authorid0000-0002-6349-0380en_US
dc.authorid0000-0003-1570-0344en_US
dc.contributor.authorIori, M.
dc.contributor.authorArslan, E.
dc.contributor.authorDenizli, Haluk
dc.contributor.authorKaya, M.
dc.contributor.authorYılmaz, Ali
dc.contributor.authorRuss, James
dc.date.accessioned2021-06-23T19:28:55Z
dc.date.available2021-06-23T19:28:55Z
dc.date.issued2012
dc.departmentBAİBÜ, Fen Edebiyat Fakültesi, Fizik Bölümüen_US
dc.description3rd Roma International Conference on Astroparticle Physics (RICAP) -- MAY 24-27, 2011 -- Roma Tre Univ, Roma, ITALYen_US
dc.description.abstractWe show the test results for TOF resolution and mu/e separation capabilities of a prototype element (Iori and Sergi, 2008 [1]), intended for deployment in an array capable of measuring large zenith angle cosmic rays as well as detecting the signature of Ultra High Energy tau neutrino interactions using the Earth skimming strategy (Fargion et al., 2004 [2], Feng et al., 2002 [3], Beacom et al., 2003 [4], Zas, 2005 [5]). The module was designed to recognize single particles and determine the direction of motion (up/down) and measure the trajectory angles. It uses two pairs of scintillator counters, named towers, each composed by two tiles (20 x 20 cm(2), 1.4 cm thick), separated by 160 cm. Each tile is read by one low voltage R5783 Hamamatsu photomultiplier (PMT). Two PMT boxes are attached to a metal structure that defines the axis of the array. Each tile is embedded in a PVC box which also contains the PMT. The PMT has excellent time resolution (approximate to 400 ps) for good TOE precision. The PMT signal was digitized by the MATAQ board in coincidence with KASCADE-GRANDE (KG) shower Delagnes and Breton, 2001 [6]. (C) 2012 Published by Elsevier B.V.en_US
dc.description.sponsorshipUniv Sapienza, Univ Tor Vergataen_US
dc.identifier.doi10.1016/j.nima.2012.01.014
dc.identifier.endpage287en_US
dc.identifier.issn0168-9002
dc.identifier.scopus2-s2.0-84866629479en_US
dc.identifier.scopusqualityQ1en_US
dc.identifier.startpage285en_US
dc.identifier.urihttps://doi.org/10.1016/j.nima.2012.01.014
dc.identifier.urihttps://hdl.handle.net/20.500.12491/7087
dc.identifier.volume692en_US
dc.identifier.wosWOS:000309786000059en_US
dc.identifier.wosqualityQ2en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.institutionauthorArslan, E.
dc.institutionauthorDenizli, Haluk
dc.institutionauthorYılmaz, Ali
dc.language.isoenen_US
dc.publisherElsevier Science Bven_US
dc.relation.ispartofNuclear Instruments & Methods In Physics Research Section A-Accelerators Spectrometers Detectors And Associated Equipmenten_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectNeutrinoen_US
dc.subjectTauen_US
dc.subjectUHECRen_US
dc.subjectScintillatoren_US
dc.titleElectron-muon identification by atmospheric shower in a new concept of an EAS detectoren_US
dc.typeConference Objecten_US

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