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CERN Document Server 33 notices trouvées  1 - 10suivantfin  aller vers la notice: La recherche a duré 0.57 secondes. 
1.
Implication on the core collapse supernova rate from 21 years of data of the Large Volume Detector / Agafonova, N.Y. (Moscow, INR) ; Aglietta, M. (INFN, Turin) ; Antonioli, P. (INFN, Bologna) ; Ashikhmin, V.V. (Moscow, INR) ; Badino, G. (INFN, Turin ; Turin U.) ; Bari, G. (INFN, Turin) ; Bertoni, R. ; Bressan, E. (Gran Sasso) ; Bruno, G. (Moscow, INR) ; Dadykin, V.L. (Moscow, INR) et al. /LVD
The Large Volume Detector (LVD) has been continuously taking data since 1992 at the INFN Gran Sasso National Laboratory. LVD is sensitive to neutrino bursts from gravitational stellar collapses with full detection probability over the Galaxy. [...]
arXiv:1411.1709.- 2015-03-20 - 9 p. - Published in : Astrophys. J. 802 (2015) 47 Fulltext: PDF; External link: Preprint
2.
Measurement of muon charge ratio with the Large Volume Detector / LVD Collaboration
The value of ${\mu^+/\mu^-}$ ratio for atmospheric muons has been measured with the Large Volume Detector, (LVD) at the INFN Gran Sasso National Laboratory, Italy (minimal depth is 3000 m w.e.). [...]
arXiv:1311.6995.
- 2013. - 14 p.
Preprint - Full text
3.
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam / OPERA Collaboration
The OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km with much higher accuracy than previous studies conducted with accelerator neutrinos. The measurement is based on high-statistics data taken by OPERA in the years 2009, 2010 and 2011. [...]
arXiv:1109.4897.- 2012 - 24 p. - Published in : JHEP 10 (2012) 093 Fulltext: PDF; Springer Open Access article: PDF; External links: Interactions.org article; Press Release; Nautilus article
4.
Search for $\nu_{\mu} \to \nu_{\tau}$ oscillation with the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA neutrino experiment in the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in direct appearance mode in the nu_mu to nu_tau channel, the nu_tau signature being the identification of the tau-lepton created in its charged current interaction. [...]
arXiv:1107.2594 ; CERN-PH-EP-2011-116.
- 2011. - 23 p.
CERN-PH-EP-2011-116 (2011-07-11) - Preprint - Full text
5.
Momentum measurement by the Multiple Coulomb Scattering method in the OPERA lead emulsion target / OPERA Collaboration
A new method of momentum measurement of charged particles through Multiple Coulomb Scattering (MCS) in the OPERA lead emulsion target is presented. It is based on precise measurements of track angular deviations performed thanks to the very high resolution of nuclear emulsions. [...]
arXiv:1106.6211.- 2012 - 15 p. - Published in : New J. Phys. 14 (2012) 013026 Fulltext: arXiv:1106.6211 - PDF; njp12_1_013026 - PDF; IOP Open Access article: PDF; External link: Preprint
6.
Study of neutrino interactions with the electronic detectors of the OPERA experiment / OPERA Collaboration
The OPERA experiment is based on a hybrid technology combining electronic detectors and nuclear emulsions. OPERA collected muon-neutrino interactions during the 2008 and 2009 physics runs of the CNGS neutrino beam, produced at CERN with an energy range of about 5-35 GeV. [...]
arXiv:1102.1882.- 2011 - 22 p. - Published in : New J. Phys. 13 (2011) 053051 Fulltext: arXiv:1102.1882 - PDF; njp11_5_053051 - PDF; External link: Preprint
7.
Observation of a first $\nu_\tau$ candidate event in the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrino oscillations in direct appearance mode through the study of the $\nu_\mu\rightarrow\nu_\tau$ channel. The hybrid apparatus consists of an emulsion/lead target complemented by electronic detectors and it is placed in the high energy long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. [...]
arXiv:1006.1623.- 2010 - 19 p. - Published in : Phys. Lett. B 691 (2010) 138-145 Fulltext: arXiv:1006.1623 - PDF; S0370269310007537 - XML; External link: Interactions.org article
8.
Measurement of the atmospheric muon charge ratio with the OPERA detector / OPERA Collaboration
The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run. [...]
arXiv:1003.1907.- 2010 - 14 p. - Published in : Eur. Phys. J. C 67 (2010) 25-37 Fulltext: arXiv:1003.1907 - PDF; 10052_2010_1284_OnlinePDF - PDF; External link: Preprint
9.
The OPERA experiment in the CERN to Gran Sasso neutrino beam / Acquafredda, R (INFN, Naples) ; Adam, T (Strasbourg, IPHC) ; Agafonova, N (Moscow, INR) ; Alvarez Sanchez, P (CERN) ; Ambrosio, M (INFN, Naples) ; Anokhina, A (SINP, Moscow) ; Aoki, S (Kobe U.) ; Ariga, A (Bern U., LHEP) ; Ariga, T (Nagoya U.) ; Arrabito, L (Lyon, IPN) et al.
2009 - Published in : JINST 4 (2009) P04018 SISSA/IOP Open Access article: PDF;
10.
The detection of neutrino interactions in the emulsion/lead target of the OPERA experiment / Agafonova, N. (Moscow, INR) ; Anokhina, A. (SINP, Moscow) ; Aoki, S. (Kobe U.) ; Ariga, A. (Bern U., LHEP) ; Ariga, T. (Bern U., LHEP) ; Arrabito, L. (Lyon, IPN) ; Autiero, D. (Lyon, IPN) ; Badertscher, A. (Zurich, ETH) ; Bagulya, A. (Lebedev Inst.) ; Bersani Greggio, F. (Frascati) et al.
The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in appearance mode through the study of $\nu_\mu\to\nu_\tau$ oscillations. The apparatus consists of an emulsion/lead target complemented by electronic detectors and it is placed in the high energy long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. [...]
arXiv:0903.2973.- 2009 - 17 p. - Published in : JINST 4 (2009) P06020 Fulltext: PDF; SISSA/IOP Open Access article : PDF; External link: Preprint

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Voir aussi: noms d'auteurs similaires
1 Enikeev, R
24 Enikeev, R I
2 Enikeev, R.I.
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