001562756 001__ 1562756
001562756 003__ SzGeCERN
001562756 005__ 20210716013742.0
001562756 0247_ $$2DOI$$a10.1140/epjc/s10052-013-2599-z
001562756 0248_ $$aoai:cds.cern.ch:1562756$$pcerncds:FULLTEXT$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT
001562756 035__ $$9arXiv$$aoai:arXiv.org:1307.4699
001562756 035__ $$9Inspire$$a1243162
001562756 037__ $$9arXiv$$aarXiv:1307.4699$$chep-ex
001562756 041__ $$aeng
001562756 084__ $$2PDG$$9PDG$$aS067S1
001562756 084__ $$2PDG$$9PDG$$aS067S2
001562756 100__ $$aAntonello, M.$$uGran Sasso
001562756 245__ $$aSearch for anomalies in the $\nu_e$ appearance from a $\nu_\mu$ beam
001562756 260__ $$c2013-10-17
001562756 269__ $$c17 Jul 2013
001562756 300__ $$a9 p
001562756 500__ $$9arXiv$$a
001562756 520__ $$aWe report an updated result from the ICARUS experiment on the search for {\nu}{\mu} ->{\nu}e anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and travelling 730 km to the Gran Sasso Laboratory. The present analysis is based on a total sample of 1995 events of CNGS neutrino interactions, which corresponds to an almost doubled sample with respect to the previously published result. Four clear {\nu}e events have been visually identified over the full sample, compared with an expectation of 6.4 +- 0.9 events from conventional sources. The result is compatible with the absence of additional anomalous contributions. At 90% and 99% confidence levels the limits to possible oscillated events are 3.7 and 8.3 respectively. The corresponding limit to oscillation probability becomes consequently 3.4 x 10-3 and 7.6 x 10-3 respectively. The present result confirms, with an improved sensitivity, the early result already published by the ICARUS collaboration.
001562756 520__ $$9Inspire$$aWe report an updated result from the ICARUS experiment on the search for {\nu}{\mu} ->{\nu}e anomalies with the CNGS beam, produced at CERN with an average energy of 20 GeV and travelling 730 km to the Gran Sasso Laboratory. The present analysis is based on a total sample of 1995 events of CNGS neutrino interactions, which corresponds to an almost doubled sample with respect to the previously published result. Four clear {\nu}e events have been visually identified over the full sample, compared with an expectation of 6.4 +- 0.9 events from conventional sources. The result is compatible with the absence of additional anomalous contributions. At 90% and 99% confidence levels the limits to possible oscillated events are 3.7 and 8.3 respectively. The corresponding limit to oscillation probability becomes consequently 3.4 x 10-3 and 7.6 x 10-3 respectively. The present result confirms, with an improved sensitivity, the early result already published by the ICARUS collaboration.
001562756 540__ $$aarXiv nonexclusive-distrib. 1.0$$barXiv$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
001562756 595__ $$aINSPIRE-PUBL-2013
001562756 65017 $$2arXiv$$aParticle Physics - Experiment
001562756 65027 $$2arXiv$$aDetectors and Experimental Techniques
001562756 695__ $$9LANL EDS$$ahep-ex
001562756 690C_ $$aARTICLE
001562756 690C_ $$aCERN
001562756 693__ $$aCERN SPS$$eICARUS CNGS2
001562756 700__ $$aBaibussinov, B.$$uINFN, Padua
001562756 700__ $$aBenetti, P.$$uINFN, Pavia
001562756 700__ $$aBoffelli, F.$$uINFN, Pavia
001562756 700__ $$aBubak, A.$$uSilesia U.
001562756 700__ $$aCalligarich, E.$$uINFN, Pavia
001562756 700__ $$aCanci, N.$$uGran Sasso
001562756 700__ $$aCentro, S.$$uINFN, Padua
001562756 700__ $$aCesana, A.$$uINFN, Milan
001562756 700__ $$aCieslik, K.$$uCracow, INP
001562756 700__ $$aCline, D.B.$$uUCLA
001562756 700__ $$aCocco, A.G.$$uINFN, Naples
001562756 700__ $$aDabrowska, A.$$uCracow, INP
001562756 700__ $$aDequal, D.$$uINFN, Padua
001562756 700__ $$aDermenev, A.$$uMoscow, INR
001562756 700__ $$aDolfini, R.$$uINFN, Pavia
001562756 700__ $$aFalcone, A.$$uINFN, Pavia
001562756 700__ $$aFarnese, C.$$uINFN, Padua
001562756 700__ $$aFava, A.$$uINFN, Padua
001562756 700__ $$aFerrari, A.$$uCERN
001562756 700__ $$aFiorillo, G.$$uINFN, Naples
001562756 700__ $$aGibin, D.$$uINFN, Padua
001562756 700__ $$aGninenko, S.$$uMoscow, INR
001562756 700__ $$aGuglielmi, A.$$uINFN, Padua
001562756 700__ $$aHaranczyk, M.$$uCracow, INP
001562756 700__ $$aHoleczek, J.$$uSilesia U.
001562756 700__ $$aIvashkin, A.$$uMoscow, INR
001562756 700__ $$aKirsanov, M.$$uMoscow, INR
001562756 700__ $$aKisiel, J.$$uSilesia U.
001562756 700__ $$aKochanek, I.$$uSilesia U.
001562756 700__ $$aLagoda, J.$$uSoltan Inst., Swierk
001562756 700__ $$aMania, S.$$uSilesia U.
001562756 700__ $$aMenegolli, A.$$uINFN, Pavia
001562756 700__ $$aMeng, G.$$uINFN, Padua
001562756 700__ $$aMontanari, C.$$uINFN, Pavia
001562756 700__ $$aOtwinowski, S.$$uUCLA
001562756 700__ $$aPicchi, P.$$uFrascati
001562756 700__ $$aPietropaolo, F.$$uINFN, Padua
001562756 700__ $$aPlonski, P.$$uWarsaw U. of Tech.
001562756 700__ $$aRappoldi, A.$$uINFN, Pavia
001562756 700__ $$aRaselli, G.L.$$uINFN, Pavia
001562756 700__ $$aRossella, M.$$uINFN, Pavia
001562756 700__ $$aRubbia, C.$$uGSSI, Aquila$$uGran Sasso
001562756 700__ $$aSala, P.$$uINFN, Milan
001562756 700__ $$aScaramelli, A.$$uINFN, Milan
001562756 700__ $$aSegreto, E.$$uGran Sasso
001562756 700__ $$aSergiampietri, F.$$uINFN, Pisa
001562756 700__ $$aStefan, D.$$uGran Sasso
001562756 700__ $$aSulej, R.$$uSoltan Inst., Swierk
001562756 700__ $$aSzarska, M.$$uCracow, INP
001562756 700__ $$aTerrani, M.$$uINFN, Milan
001562756 700__ $$aTorti, M.$$uINFN, Pavia
001562756 700__ $$aVaranini, F.$$uINFN, Padua
001562756 700__ $$aVentura, S.$$uINFN, Padua
001562756 700__ $$aVignoli, C.$$uGran Sasso
001562756 700__ $$aWang, H.$$uUCLA
001562756 700__ $$aYang, X.$$uUCLA
001562756 700__ $$aZalewska, A.$$uCracow, INP
001562756 700__ $$aZani, A.$$uINFN, Pavia
001562756 700__ $$aZaremba, K.$$uWarsaw U. of Tech.
001562756 710__ $$gICARUS collaboration
001562756 773__ $$c2599$$pEur. Phys. J. C$$v73$$y2013
001562756 8564_ $$uhttp://arxiv.org/pdf/1307.4699.pdf$$yPreprint
001562756 8564_ $$82215741$$s2036486$$uhttps://cds.cern.ch/record/1562756/files/arXiv:1307.4699.pdf
001562756 916__ $$sn$$w201328$$ya2013
001562756 960__ $$a13
001562756 980__ $$aARTICLE