DC pole | Wartość | Język |
dc.contributor.author | Antonello, M. | - |
dc.contributor.author | Aprili, P. | - |
dc.contributor.author | Baiboussinov, B. | - |
dc.contributor.author | Baldo Ceolin, M. | - |
dc.contributor.author | Benetti, P. | - |
dc.contributor.author | Calligarich, E. | - |
dc.contributor.author | Cancia, N. | - |
dc.contributor.author | Centro, S. | - |
dc.contributor.author | Cesanae, A. | - |
dc.contributor.author | Cieślik, K. | - |
dc.contributor.author | Clineg, D.B. | - |
dc.contributor.author | Cocco, A.G. | - |
dc.contributor.author | Dabrowska, A. | - |
dc.contributor.author | Dequal, D. | - |
dc.contributor.author | Dermenevh, A. | - |
dc.contributor.author | Dolfini, R. | - |
dc.contributor.author | Farnese, C. | - |
dc.contributor.author | Favab, A. | - |
dc.contributor.author | Ferrarii, A. | - |
dc.contributor.author | Fiorillo, G. | - |
dc.contributor.author | Gibin, D. | - |
dc.contributor.author | Gigli Berzolari, A. | - |
dc.contributor.author | Gninenko, S. | - |
dc.contributor.author | Guglielmi, A. | - |
dc.contributor.author | Haranczyk, M. | - |
dc.contributor.author | Holeczek, Jacek | - |
dc.contributor.author | Ivashkin, A. | - |
dc.contributor.author | Kisiel, Jan | - |
dc.contributor.author | Kochanek, Izabela | - |
dc.contributor.author | Lagodak, J. | - |
dc.contributor.author | Mania, Sławomir | - |
dc.contributor.author | Mannocchi, G. | - |
dc.contributor.author | Menegolli, A. | - |
dc.contributor.author | Meng, G. | - |
dc.contributor.author | Montanari, C. | - |
dc.contributor.author | Otwinowski, S. | - |
dc.contributor.author | Periale, L. | - |
dc.contributor.author | Piazzoli, A. | - |
dc.contributor.author | Picchi, P. | - |
dc.contributor.author | Pietropaolo, F. | - |
dc.contributor.author | Plonski, P. | - |
dc.contributor.author | Rappoldi, A. | - |
dc.contributor.author | Raselli, G.L. | - |
dc.contributor.author | Rossella, M. | - |
dc.contributor.author | Rubbia, C. | - |
dc.contributor.author | Salae, P. | - |
dc.contributor.author | Scantamburlo, E. | - |
dc.contributor.author | Scaramelli, A. | - |
dc.contributor.author | Segreto, E. | - |
dc.contributor.author | Sergiampietri, F. | - |
dc.contributor.author | Stefan, D. | - |
dc.contributor.author | Stepaniak, J. | - |
dc.contributor.author | Sulej, R. | - |
dc.contributor.author | Szarska, M. | - |
dc.contributor.author | Terranie, M. | - |
dc.contributor.author | Varanini, F. | - |
dc.contributor.author | Ventura, S. | - |
dc.contributor.author | Vignoli, C. | - |
dc.contributor.author | Wangg, H.G. | - |
dc.contributor.author | Zalewska, A. | - |
dc.contributor.author | Zaremba, K. | - |
dc.contributor.author | Alvarez Sanchez, P. | - |
dc.contributor.author | Serrano, J. | - |
dc.date.accessioned | 2019-05-30T11:08:57Z | - |
dc.date.available | 2019-05-30T11:08:57Z | - |
dc.date.issued | 2012 | - |
dc.identifier.citation | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Vol. 713, iss. 1 (2012), s. 17-22 | pl_PL |
dc.identifier.issn | 0370-2693 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12128/9252 | - |
dc.description.abstract | At the end of the 2011 run, the CERN CNGS neutrino beam has been briefly operated in lower intensity
mode with ∼ 1012 p.o.t./pulse and with a proton beam structure made of four LHC-like extractions,
each with a narrow width of ∼ 3 ns, separated by 524 ns. This very tightly bunched beam allowed a
very accurate time-of-flight measurement of neutrinos from CERN to LNGS on an event-by-event basis.
The ICARUS T600 detector (CNGS2) has collected 7 beam-associated events, consistent with the CNGS
collected neutrino flux of 2.2 × 1016 p.o.t. and in agreement with the well-known characteristics of
neutrino events in the LAr-TPC. The time of flight difference between the speed of light and the arriving
neutrino LAr-TPC events has been analysed. The result δt = 0.3 ± 4.9(stat.) ± 9.0(syst.) ns is compatible
with the simultaneous arrival of all events with speed equal to that of light. This is in a striking difference
with the reported result of OPERA (OPERA Collaboration, 2011) [1] claiming that high energy neutrinos
from CERN arrive at LNGS ∼ 60 ns earlier than expected from luminal speed. | pl_PL |
dc.language.iso | en | pl_PL |
dc.rights | Uznanie autorstwa 3.0 Polska | * |
dc.rights.uri | http://creativecommons.org/licenses/by/3.0/pl/ | * |
dc.subject | Liquefied gases | pl_PL |
dc.subject | argon | pl_PL |
dc.subject | argon time | pl_PL |
dc.title | Measurement of the neutrino velocity with the ICARUS detector at the CNGS beam | pl_PL |
dc.type | info:eu-repo/semantics/article | pl_PL |
dc.relation.journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics | pl_PL |
dc.identifier.doi | 10.1016/j.physletb.2012.05.033 | - |
Pojawia się w kolekcji: | Artykuły (WNŚiT)
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