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CERN Document Server Sök i 90 journaler efter:  1 - 10nästaslut  gå till journal: Sökningen tog 0.62 sekunder. 
1.
The active muon shield in the SHiP experiment / Akmete, A. (Middle East Tech. U., Ankara) ; Alexandrov, A. (INFN, Florence) ; Anokhina, A. (SINP, Moscow) ; Aoki, S. (Kobe U.) ; Atkin, E. (Moscow Phys. Eng. Inst.) ; Azorskiy, N. (Dubna, JINR) ; Back, J.J. (Warwick U.) ; Bagulya, A. (LPI, Moscow (main)) ; Baranov, A. (Yandex Sch. Data Anal., Moscow) ; Barker, G.J. (Warwick U.) et al. /SHiP
The SHiP experiment is designed to search for very weakly interacting particles beyond the Standard Model which are produced in a 400 GeV/c proton beam dump at the CERN SPS. An essential task for the experiment is to keep the Standard Model background level to less than 0.1 event after $2\times 10^{20}$ protons on target. [...]
arXiv:1703.03612.- 2017-05-17 - 10 p. - Published in : JINST 12 (2017) P05011 Fulltext: arXiv:1703.03612 - PDF; 10.1088_1748-0221_12_05_P05011 - PDF; IOP Open Acess article: PDF;
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2.
Discovery of tau neutrino appearance in the CNGS neutrino beam with the OPERA experiment / OPERA Collaboration
The OPERA experiment was designed to search for $\nu_{\mu} \rightarrow \nu_{\tau}$ oscillations in appearance mode, i.e. by detecting the $\tau$-leptons produced in charged current $\nu_{\tau}$ interactions. [...]
arXiv:1507.01417.- 2015-09-17 - 7 p. - Published in : Phys. Rev. Lett. 115 (2015) 121802 Fulltext: PDF; External links: Interactions.org article; Symmetry Magazine article
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3.
Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam / OPERA Collaboration
The OPERA experiment, exposed to the CERN to Gran Sasso $\nu_\mu$ beam, collected data from 2008 to 2012. Four oscillated $\nu_\tau$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with $\nu_\mu \to \nu_\tau$ oscillations at the atmospheric $\Delta m^2$ within the "standard" three-neutrino framework. [...]
arXiv:1503.01876.- 2015-06-11 - 11 p. Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
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4.
Observation of nu_tau appearance in the CNGS beam with the OPERA experiment / OPERA Collaboration
The OPERA experiment is searching for nu_mu -> nu_tau oscillations in appearance mode i.e. via the direct detection of tau leptons in nu_tau charged current interactions. [...]
arXiv:1407.3513.- 2014-10-27 - 10 p. - Published in : Prog. Theor. Exp. Phys. 2014 (2014) 101C01 Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
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5.
The Angular Matching Method for the Muon Charge Sign Measurement in the OPERA Experiment / OPERA Collaboration
The long baseline neutrino oscillation experiment OPERA is searching for $\nu_{\tau}$ appearance in the CNGS beam of $\nu_{\mu}$. The task of the two muon spectrometers of the OPERA detector is to clarify the signature of a muonic $\tau$ decay ($\mu^{-}$) and to reduce background originating from charmed particles produced in $\nu_{\mu}$ interactions ($\mu^{+}$). [...]
arXiv:1404.5933.- 2016-07-25 - 10 p. - Published in : JINST 11 (2016) P07022 Fulltext: PDF; External link: Preprint
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6.
Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays / OPERA Collaboration
The OPERA experiment, designed to perform the first observation of $\nu_\mu \rightarrow \nu_\tau$ oscillations in appearance mode through the detection of the $\tau$ leptons produced in $\nu_\tau$ charged current interactions, has collected data from 2008 to 2012. In the present paper, the procedure developed to detect $\tau$ particle decays, occurring over distances of the order of 1 mm from the neutrino interaction point, is described in detail. [...]
arXiv:1404.4357.- 2014-08-07 - 9 p. - Published in : Eur. Phys. J. C 74 (2014) 2986 Article from SCOAP3: PDF; Fulltext: PDF; Springer Open Access article: PDF; External link: Preprint
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7.
Measurement of TeV atmospheric muon charge ratio with the full OPERA data / OPERA Collaboration
The OPERA detector, designed to search for ν μ → ν τ oscillations in the CNGS beam, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scale cosmic rays. For the analysis here presented, the detector was used to measure the atmospheric muon charge ratio in the TeV region [...]
arXiv:1403.0244.- 2014-07-02 - 9 p. Article from SCOAP3: PDF; Fulltext: PDF;
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8.
Evidence for $\nu_\mu \to \nu_\tau$ appearance in the CNGS neutrino beam with the OPERA experiment / OPERA Collaboration
The OPERA experiment is designed to search for $\nu_{\mu} \rightarrow \nu_{\tau}$ oscillations in appearance mode i.e. through the direct observation of the $\tau$ lepton in $\nu_{\tau}$ charged current interactions. [...]
arXiv:1401.2079.- 2014-03-05 - 6 p. - Published in : Phys. Rev. D 89 (2014) 051102 Fulltext: PDF; External link: Preprint
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9.
Search for $\nu_\mu \rightarrow \nu_e$ oscillations with the OPERA experiment in the CNGS beam / OPERA collaboration
A first result of the search for \numu $\rightarrow$ \nue oscillations in the OPERA experiment, located at the Gran Sasso Underground Laboratory, is presented. The experiment looked for the appearance of \nue in the CNGS neutrino beam using the data collected in 2008 and 2009. [...]
arXiv:1303.3953.- 2013 - 3 p. Fulltext: PDF; External link: Preprint
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10.
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data / OPERA Collaboration
In spring 2012 CERN provided two weeks of a short bunch proton beam dedicated to the neutrino velocity measurement over a distance of 730 km. The OPERA neutrino experiment at the underground Gran Sasso Laboratory used an upgraded setup compared to the 2011 measurements, improving the measurement time accuracy. [...]
arXiv:1212.1276.- 2013 - 14 p. - Published in : JHEP 01 (2013) 153 Fulltext: PDF; Springer Open Access article: PDF; External link: Preprint
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1 Chernyavsky, M
83 Chernyavsky, M M
2 Chernyavsky, M.M.
1 Chernyavsky, MM
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