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CERN Document Server 找到 317 笔记录  1 - 10下一个最後  跳到记录: 检索需时 0.69 秒. 
1.
Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method / OPERA Collaboration
This paper describes a new $\nu_e$ identification method specifically designed to improve the low-energy ($< 30\,\mathrm{GeV}$) $\nu_e$ identification efficiency attained by enlarging the emulsion film scanning volume with the next generation emulsion readout system. A relative increase of 25-70% in the $\nu_e$ low-energy region is expected, leading to improvements in the OPERA sensitivity to neutrino oscillations in the framework of the 3 + 1 model. [...]
arXiv:2211.04636.- 2023-03-09 - 13 p. - Published in : PTEP 2023 (2023) 033C01 Fulltext: document - PDF; 2211.04636 - PDF;
2.
OPERA public note 190 : Background reduction and systematic uncertainty of the ESD method in the OPERA experiment / Hayakawa, Tomohiro (Nagoya University)
This is a supplementary material for the paper "Updated constraints on sterile neutrino mixing in the OPERA experiment using a new nu_e identication method"
CERN-OPEN-2022-016.
- 2022. - 7 p.
Preprint
3.
OPERA tau neutrino charged current interactions / OPERA Collaboration
The OPERA experiment was designed to discover the v$_\tau$ appearance in a v$_\mu$ beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. [...]
2021 - 18 p. - Published in : Sci. Data 8 (2021) 218 Fulltext: PDF;
4.
First observation of a tau neutrino charged current interaction with charm production in the Opera experiment / OPERA Collaboration
An event topology with two secondary vertices compatible with the decay of short-lived particles was found in the analysis of neutrino interactions in the Opera target. The observed topology is compatible with tau neutrino charged current (CC) interactions with charm production and neutrino neutral current (NC) interactions with $c\overline{c}$ pair production. [...]
arXiv:1912.11012.- 2020-08-04 - 10 p. - Published in : Eur. Phys. J. C 80 (2020) 699 Article from SCOAP3: PDF; Fulltext: PDF;
5.
Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA experiment has conclusively observed the appearance of tau neutrinos in the muon neutrino CNGS beam. Exploiting the OPERA detector capabilities, it was possible to isolate high purity samples of $\nu_{e}$, $\nu_{\mu}$ and $\nu_{\tau}$ charged current weak neutrino interactions, as well as neutral current weak interactions. [...]
arXiv:1904.05686.- 2019-09-07 - 8 p. - Published in : Phys. Rev. D 100 (2019) 051301 Article from SCOAP3: PDF; Fulltext: PDF;
6.
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
7.
Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector / OPERA Collaboration
The OPERA experiment discovered muon neutrino into tau neutrino oscillations in appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus was also endowed with electronic detectors with tracking capability, such as scintillator strips and resistive plate chambers. [...]
arXiv:1810.10783.- 2019-10-01 - 15 p. - Published in : JCAP 1910 (2019) 003 Fulltext: PDF;
8.
The Hi-GAL compact source catalogue – I. The physical properties of the clumps in the inner Galaxy (−71$_{.}^{\circ}$0 < ℓ < 67$_{.}^{\circ}$0) / Elia, Davide (INAF, Rome) ; Molinari, S. (INAF, Rome) ; Schisano, E. (INAF, Rome) ; Pestalozzi, M. (INAF, Rome) ; Pezzuto, S. (INAF, Rome) ; Merello, M. (INAF, Rome) ; Noriega-Crespo, A. (Baltimore, Space Telescope Sci.) ; Moore, T.J. T. (Liverpool John Moores U., ARI) ; Russeil, D. (Marseille, Lab. Astrophys.) ; Mottram, J.C. (Heidelberg, Max Planck Inst. Astron.) et al.
Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $\mu$m. We present a band-merged catalogue of spatially matched sources and their properties derived from fits to the spectral energy distributions (SEDs) and heliocentric distances, based on the photometric catalogs presented in Molinari et al. [...]
arXiv:1706.01046.- 2017 - 44 p. - Published in : Mon. Not. R. Astron. Soc. 471 (2017) 100-143 Fulltext: PDF;
9.
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
10.
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;

CERN Document Server : 找到 317 笔记录   1 - 10下一个最後  跳到记录:
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248 Hayakawa, Takashi
3 Hayakawa, Takehito
1 Hayakawa, Takesi
3 Hayakawa, Taku
1 Hayakawa, Tomohiro
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