002239982 001__ 2239982
002239982 005__ 20240409050457.0
002239982 0248_ $$aoai:cds.cern.ch:2239982$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:FULLTEXT
002239982 0247_ $$2DOI$$a10.1088/1748-0221/12/04/P04010
002239982 037__ $$9arXiv$$aarXiv:1612.07715$$cphysics.ins-det
002239982 035__ $$9arXiv$$aoai:arXiv.org:1612.07715
002239982 035__ $$9Inspire$$aoai:inspirehep.net:1505598$$d2024-04-08T14:11:50Z$$h2024-04-09T02:09:26Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002239982 035__ $$9Inspire$$a1505598
002239982 041__ $$aeng
002239982 100__ $$aAntonello, M.$$uGran Sasso$$vINFN—Laboratori Nazionali del Gran Sasso - Assergi - Italy
002239982 245__ $$9arXiv$$aMuon momentum measurement in ICARUS-T600 LAr-TPC via multiple scattering in few-GeV range
002239982 246__ $$9arXiv$$aMuon momentum measurement in ICARUS-T600 LAr-TPC via multiple scattering in few-GeV range
002239982 269__ $$c2016-12-22
002239982 260__ $$c2017-04-10
002239982 300__ $$a22 p
002239982 500__ $$9arXiv$$a20 pages, 20 figures
002239982 520__ $$9IOP$$aThe measurement of muon momentum by Multiple Coulomb Scattering is a crucial ingredient to the reconstruction of ν(μ) CC events in the ICARUS-T600 liquid argon TPC in absence of magnetic field, as in the search for sterile neutrinos at Fermilab where ICARUS will be exposed to ~ 1 GeV Booster neutrino beam. A sample of ~ 1000 stopping muons produced by charged current interactions of CNGS ν(μ)( ) in the surrounding rock at the INFN Gran Sasso underground Laboratory provides an ideal benchmark in the few-GeV range since their momentum can be directly and independently obtained by the calorimetric measurement. Stopping muon momentum in the 0.5–4.5 GeV/c range has been reconstructed via Multiple Coulomb Scattering with resolution ranging from 10 to 25% depending on muon energy, track length and uniformity of the electric field in the drift volume.
002239982 520__ $$9arXiv$$aThe measurement of muon momentum by Multiple Coulomb Scattering is a crucial ingredient to the reconstruction of {\nu}{\mu} CC events in the ICARUS-T600 liquid argon TPC in absence of magnetic field, as in the search for sterile neutrinos at Fermilab where ICARUS will be exposed to ~1 GeV Booster neutrino beam. A sample of ~1000 stopping muons produced by charged current interactions of CNGS {\nu}{\mu} in the surrounding rock at the INFN Gran Sasso underground Laboratory provides an ideal benchmark in the few-GeV range since their momentum can be directly and independently obtained by the calorimetric measurement. Stopping muon momentum in the 0.5- 4.5 GeV/c range has been reconstructed via Multiple Coulomb Scattering with resolution ranging from 10 to 25 % depending on muon energy, track length and uniformity of the electric field in the drift volume.
002239982 540__ $$aarXiv nonexclusive-distrib. 1.0$$barXiv$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
002239982 540__ $$3publication$$aCC-BY-3.0
002239982 542__ $$3publication$$dThe Author(s)$$g2017
002239982 65017 $$2arXiv$$ahep-ex
002239982 65017 $$2SzGeCERN$$aParticle Physics - Experiment
002239982 65017 $$2arXiv$$aphysics.ins-det
002239982 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
002239982 693__ $$aCERN SPS$$eICARUS-T600
002239982 690C_ $$aCERN
002239982 690C_ $$aARTICLE
002239982 695__ $$2INSPIRE$$9bibclassify$$amuon: momentum
002239982 695__ $$2INSPIRE$$9bibclassify$$ascattering: Coulomb
002239982 695__ $$2INSPIRE$$9bibclassify$$amuon: energy
002239982 695__ $$2INSPIRE$$9bibclassify$$atime projection chamber: liquid argon
002239982 695__ $$2INSPIRE$$9bibclassify$$aneutrino: sterile: search for
002239982 695__ $$2INSPIRE$$9bibclassify$$aneutrino: beam
002239982 695__ $$2INSPIRE$$9bibclassify$$atracks: length
002239982 695__ $$2INSPIRE$$9bibclassify$$amultiple scattering
002239982 695__ $$2INSPIRE$$9bibclassify$$acharged current
002239982 695__ $$2INSPIRE$$9bibclassify$$amagnetic field
002239982 695__ $$2INSPIRE$$9bibclassify$$aelectric field
002239982 695__ $$2INSPIRE$$9bibclassify$$acalorimeter
002239982 695__ $$2INSPIRE$$9bibclassify$$aGran Sasso
002239982 695__ $$2INSPIRE$$9bibclassify$$aresolution
002239982 695__ $$2INSPIRE$$9bibclassify$$abenchmark
002239982 695__ $$2INSPIRE$$9bibclassify$$abooster
002239982 695__ $$2INSPIRE$$9bibclassify$$aICARUS
002239982 695__ $$2INSPIRE$$9bibclassify$$aCNGS
002239982 700__ $$aBaibussinov, B.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aBellini, V.$$uCatania U.$$uINFN, Catania$$vDipartimento di Fisica e Astronomia Università di Catania and INFN,Catania,Italy
002239982 700__ $$aBenetti, P.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aBoffelli, F.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aBubak, A.$$uSilesia U.$$vInstitute of Physics,University of Silesia,Katowice,Poland
002239982 700__ $$aCalligarich, E.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aCentro, S.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aCervi, T.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aCesana, A.$$uINFN, Milan$$vINFN,Milano,Italy
002239982 700__ $$aCieslik, K.$$uCracow, INP$$vH. Niewodniczanski Institute of Nuclear Physics,Polish Academy of Science,Krakow,Poland
002239982 700__ $$aCocco, A.G.$$uINFN, Naples$$uNaples U.$$vDipartimento di Scienze Fisiche Università Federico II di Napoli and INFN,Napoli,Italy
002239982 700__ $$aCline, D.B.$$uUCLA$$vDepartment of Physics and Astronomy,UCLA,Los Angeles,USA
002239982 700__ $$aDabrowska, A.$$uCracow, INP$$vH. Niewodniczanski Institute of Nuclear Physics,Polish Academy of Science,Krakow,Poland
002239982 700__ $$aDermenev, A.$$uMoscow, INR$$vINR RAS,Moscow,Russia
002239982 700__ $$aFalcone, A.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aFarnese, C.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aFava, A.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aFerrari, A.$$uCERN$$vCERN,Geneva,Switzerland
002239982 700__ $$aGibin, D.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aGninenko, S.$$uCERN$$vCERN,Geneva,Switzerland
002239982 700__ $$aGuglielmi, A.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aHaranczyk, M.$$uCracow, INP$$vH. Niewodniczanski Institute of Nuclear Physics,Polish Academy of Science,Krakow,Poland
002239982 700__ $$aHoleczek, J.$$uSilesia U.$$vInstitute of Physics,University of Silesia,Katowice,Poland
002239982 700__ $$aJanik, M.$$uSilesia U.$$vInstitute of Physics,University of Silesia,Katowice,Poland
002239982 700__ $$aKirsanov, M.$$uCERN$$vCERN,Geneva,Switzerland
002239982 700__ $$aKisiel, J.$$uSilesia U.$$vInstitute of Physics,University of Silesia,Katowice,Poland
002239982 700__ $$aKochanek, I.$$uSilesia U.$$vInstitute of Physics,University of Silesia,Katowice,Poland
002239982 700__ $$aLagoda, J.$$uSoltan Inst., Swierk$$vNational Centre for Nuclear Research,Otwock/Swierk,Poland
002239982 700__ $$aMenegolli, A.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aMeng, G.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aMontanari, C.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aOtwinowski, S.$$uUCLA$$vDepartment of Physics and Astronomy,UCLA,Los Angeles,USA
002239982 700__ $$aPicchi, P.$$uFrascati$$vINFN Laboratori Nazionali di Frascati,Frascati,Italy
002239982 700__ $$aPietropaolo, F.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aPlonski, P.$$uWarsaw U. of Tech.$$vInstitute of Radioelectronics,Warsaw University of Technology,Warsaw,Poland
002239982 700__ $$aRappoldi, A.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aRaselli, G.L.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aRossella, M.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aRubbia, C.$$uGran Sasso$$uCERN$$uINFM, L'Aquila$$vINFN - Laboratori Nazionali del Gran Sasso,Assergi,Italy$$vCERN,Geneva,Switzerland$$vGSSI,L’Aquila,Italy
002239982 700__ $$aSala, P.$$uINFN, Milan$$vINFN,Milano,Italy
002239982 700__ $$aScaramelli, A.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aSergiampietri, F.$$uINFN, Pisa$$vINFN,Pisa,Italy
002239982 700__ $$aSpanu, M.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aStefan, D.$$uINFN, Milan$$vINFN,Milano,Italy
002239982 700__ $$aSulej, R.$$uSilesia U.$$vInstitute of Physics,University of Silesia,Katowice,Poland
002239982 700__ $$aSzarska, M.$$uCracow, INP$$vH. Niewodniczanski Institute of Nuclear Physics,Polish Academy of Science,Krakow,Poland
002239982 700__ $$aTerrani, M.$$uINFN, Milan$$vINFN,Milano,Italy
002239982 700__ $$aTorti, M.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aTortorici, F.$$uCatania U.$$uINFN, Catania$$vDipartimento di Fisica e Astronomia Università di Catania and INFN,Catania,Italy
002239982 700__ $$aVaranini, Filippo$$iINSPIRE-00477465$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aVentura, S.$$uINFN, Padua$$uPadua U.$$vDipartimento di Fisica e Astronomia Università di Padova and INFN,Padova,Italy
002239982 700__ $$aVignoli, C.$$uGran Sasso$$vINFN - Laboratori Nazionali del Gran Sasso,Assergi,Italy
002239982 700__ $$aWang, H.$$uUCLA$$vDepartment of Physics and Astronomy,UCLA,Los Angeles,USA
002239982 700__ $$aYang, X.$$uUCLA$$vDepartment of Physics and Astronomy,UCLA,Los Angeles,USA
002239982 700__ $$aZalewska, A.$$uCracow, INP$$vH. Niewodniczanski Institute of Nuclear Physics,Polish Academy of Science,Krakow,Poland
002239982 700__ $$aZani, A.$$uINFN, Pavia$$uPavia U.$$vDipartimento di Fisica Università di Pavia and INFN,Pavia,Italy
002239982 700__ $$aZaremba, K.$$uWarsaw U. of Tech.$$vInstitute of Radioelectronics,Warsaw University of Technology,Warsaw,Poland
002239982 710__ $$gICARUS Collaboration
002239982 773__ $$cP04010$$n04$$pJINST$$v12$$y2017
002239982 8564_ $$81266532$$s4108576$$uhttps://cds.cern.ch/record/2239982/files/arXiv:1612.07715.pdf
002239982 8564_ $$81307020$$s3258039$$uhttps://cds.cern.ch/record/2239982/files/Antonello_2017_J._Inst._12_P04010.pdf$$ySpringer Open Access article
002239982 8564_ $$81307020$$s2863492$$uhttps://cds.cern.ch/record/2239982/files/Antonello_2017_J._Inst._12_P04010.pdf?subformat=pdfa$$xpdfa$$ySpringer Open Access article
002239982 8564_ $$81371870$$s3258036$$uhttps://cds.cern.ch/record/2239982/files/10.1088_1748-0221_12_04_P04010.pdf$$yFulltext
002239982 960__ $$a13
002239982 980__ $$aARTICLE