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CERN Document Server Sök i 145 journaler efter:  1 - 10nästaslut  gå till journal: Sökningen tog 0.60 sekunder. 
1.
Development of a technique for the determination of the spatial position of sparks in a spark chamber without taking pictures / Charpak, G ; Favier, J ; Massonnet, L
1963. - 7 p.
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2.
The Alpha Magnetic Spectrometer (AMS) on the International Space Station. I: Results from the test flight on the space shuttle / AMS Collaboration
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km . A search for antihelium nuclei in the rigidity range 1– 140 GV was performed. [...]
2002 - 75 p. - Published in : Phys. Rep. 366 (2002) 331-405
- Published in : Phys. Rep. 380 (2003) 97-98
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3.
Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam / OPERA Collaboration
OPERA is a long-baseline experiment designed to search for $\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode. It was based at the INFN Gran Sasso laboratory (LNGS) and took data from 2008 to 2012 with the CNGS neutrino beam from CERN. [...]
arXiv:1811.00095.- 2019-02-20 - 7 p. - Published in : SciPost Phys. Proc. 1 (2019) 028 Fulltext: PDF;
In : The 15th International Workshop on Tau Lepton Physics, Amsterdam, Netherlands, 24 - 28 Sep 2018, pp.028
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4.
Four-layer aerogel Cherenkov counter / Arisaka, K (UCLA, Los Angeles (main)) ; Borsato, E (U. Padua (main) ; INFN, Padua) ; Boutigny, D (Annecy, LAPP) ; Buzykaev, A R (Novosibirsk, IYF) ; Dal Corso, F (U. Padua (main) ; INFN, Padua) ; De Bonis, I (Annecy, LAPP) ; Favier, J (Annecy, LAPP) ; Ferroni, F (U. Rome La Sapienza (main) ; INFN, Rome) ; Foucher, M (Maryland U., College Park) ; Ganzhur, S F (Novosibirsk, IYF) et al.
A 4-layer design of aerogel threshold counters using two refractive indices was suggested for the particle identification in the forward region of the BaBar detector. Three prototypes filled with the high quality aerogel produced in Novosibirsk were tested at T10 beam at CERN. [...]
1998 - 6 p. - Published in : J. Noncryst. Solids 225 (1998) 375-380
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5.
Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam / OPERA Collaboration
The OPERA experiment was designed to study $\nu_\mu\to\nu_\tau$ oscillations in appearance mode in the CNGS neutrino beam. In this letter we report the final analysis of the full data sample collected between 2008 and 2012, corresponding to $17.97\cdot 10^{19}$ protons on target. [...]
arXiv:1804.04912.- 2018-05-23 - 7 p. Article from SCOAP3: PDF; Fulltext: PDF; External links: Physics Synopsis; Interactions.org article
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6.
Final results of the search for $\nu_{\mu} \to \nu_{e}$ oscillations with the OPERA detector in the CNGS beam / OPERA Collaboration
The OPERA experiment has discovered the tau neutrino appearance in the CNGS muon neutrino beam, in agreement with the 3 neutrino flavour oscillation hypothesis. The OPERA neutrino interaction target, made of Emulsion Cloud Chamber, was particularly efficient in the reconstruction of electromagnetic showers. [...]
arXiv:1803.11400.- 2018-06-27 - 15 p. - Published in : JHEP 06 (2018) 151 Article from SCOAP3: PDF; Fulltext: PDF;
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7.
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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8.
New results on $\nu_\mu \to \nu_\tau$ appearance with the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the $\nu_\mu \to \nu_\tau$ channel, via the detection of the $\tau$-leptons created in charged current $\nu_\tau$ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. [...]
arXiv:1308.2553.- 2013 - 32 p.
Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
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9.
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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10.
Isotopic Composition of Light Nuclei in Cosmic Rays: Results from AMS-01 / AMS-01 Collaboration
The variety of isotopes in cosmic rays allows us to study different aspects of the processes that cosmic rays undergo between the time they are produced and the time of their arrival in the heliosphere. In this paper, we present measurements of the isotopic ratios $^2$H/$^4$He, $^3$He/$^4$He, $^6$Li/$7$Li, $7$Be/($^9$Be+$^{10}$Be), and $^{10}$B/$^{11}$B in the range 0.2-1.4 GeV of kinetic energy per nucleon. [...]
arXiv:1106.2269.- 2011 - 12 p. - Published in : Astrophys. J. 736 (2011) 105 Fulltext: PDF; External link: Preprint
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12 Favier, J
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