Search results for "Argo"

showing 10 items of 424 documents

Layout and performance of RPC used in the Argo-YBJ experiment

2006

The layout of the RPCs, used in the Argo-YBJ experiment to image with a high space-time granularity the atmospheric shower, is described in this paper. The detector has been assembled to provide both digital and analog informations in order to cover a wide particle density range with a time accuracy of 1 ns. The experimental results obtained operating the chambers in streamer mode at sea level with a standard gas mixture are presented. (c) 2006 Elsevier B.V. All rights reserved.

PhysicsNuclear and High Energy PhysicsRivelatori a gaPhysics::Instrumentation and DetectorsCosmic rays detectorAstrophysics::High Energy Astrophysical PhenomenaDetectorSettore FIS/01 - Fisica SperimentaleResistive Plate Chambers Cosmic Rays Extended Air ShowersCamere a piani resistiviRivelatori di raggi cosmiciSettore AGR/03 - Arboricoltura Generale E Coltivazioni ArboreeGas detectorRange (statistics)RPCGranularityParticle densityInstrumentationArgoRemote sensing
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Neutrino mass ordering at DUNE: An extra ν bonus

2019

We study the possibility of extracting the neutrino mass ordering at the future Deep Underground Neutrino Experiment using atmospheric neutrinos, which will be available before the muon neutrino beam starts being perational. The large statistics of the atmospheric muon neutrino and antineutrino samples at the far detector, together with the baselines of thousands of kilometers that these atmospheric (anti)neutrinos travel, provide the ideal ingredients to extract the neutrino mass ordering via matter effects in the neutrino propagation through the Earth. Crucially, muon capture by Argon provides excellent charge-tagging, allowing to disentangle the neutrino and antineutrino signature. This …

PhysicsParticle physicsArgonTime projection chamber010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorHigh Energy Physics::Phenomenologychemistry.chemical_element01 natural sciences7. Clean energyHigh Energy Physics - ExperimentMuon captureHigh Energy Physics - Phenomenologychemistry13. Climate action0103 physical sciencesDeep Underground Neutrino ExperimentMuon neutrinoHigh Energy Physics::ExperimentNeutrino010306 general physicsBeam (structure)Physical Review D
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Large underground, liquid based detectors for astro-particle physics in Europe: scientific case and prospects

2007

This document reports on a series of experimental and theoretical studies conducted to assess the astro-particle physics potential of three future large-scale particle detectors proposed in Europe as next generation underground observatories. The proposed apparatus employ three different and, to some extent, complementary detection techniques: GLACIER (liquid Argon TPC), LENA (liquid scintillator) and MEMPHYS (\WC), based on the use of large mass of liquids as active detection media. The results of these studies are presented along with a critical discussion of the performance attainable by the three proposed approaches coupled to existing or planned underground laboratories, in relation to…

PhysicsParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsDetectorActive detectionFOS: Physical sciencesAstronomy and AstrophysicsScintillator01 natural sciencesCritical discussionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesLiquid argonLiquid basedHigh Energy Physics::Experiment[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrino010306 general physicsParticle Physics - PhenomenologyJournal of Cosmology and Astroparticle Physics
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Software Timing Calibration of the ARGO-YBJ Detector

2009

The ARGO-YBJ experiment is mainly devoted to search for astronomical gamma sources. The arrival direction of air showers is reconstructed thanks to the times measured by the pixels of the detector. Therefore, the timing calibration of the detector pixels is crucial in order to get the best angular resolution and pointing accuracy. Because of the large number of pixels a hardware timing calibration is practically impossible. Therefore an off-line software calibration has been adopted. Here, the details of the procedure and the results are presented. (C) 2008 Elsevier B.V. All rights reserved.

PhysicsPixelCalibration (statistics)business.industryPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorSettore FIS/01 - Fisica SperimentaleComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsAstronomia gammaGamma Astronomy Timing Calibration Extensive Air ShowersSciami estesiCalibrazione temporaleOpticsSoftwareRaggi cosmiciSettore FIS/05 - Astronomia e AstrofisicaAngular resolutionbusinessArgoRemote sensing
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Argon-broadened line parameters in the nu3 band of 12CH4

1997

International audience; Prompted by improved measurements of collisional line shapes in the nu3 band P, Q and R branches of 12CH4, we have performed semi-classical line broadening calculations for methane perturbed by argon. We have used the theoretical approach developed by Robert and Bonamy as an extension of the well-known Anderson-Tsao-Curnutte theory. The semi-classical theory as reformulated here is shown to fully account for the tetrahedral symmetry of methane type molecules. The variation of argon-broadened linewidth coefficients in the nu3 band of 12CH4 with the branch, J, symmetry and energy level fine structure is discussed.

PhysicsRadiationArgon010304 chemical physicschemistry.chemical_elementTetrahedral symmetry01 natural sciencesAtomic and Molecular Physics and OpticsSymmetry (physics)Methane010309 opticschemistry.chemical_compoundLaser linewidthchemistry0103 physical sciencesMoleculeAtomic physicsPhysics::Chemical PhysicsSpectroscopyLine (formation)
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Background radioactivity in the scaler mode technique of the Argo-YBJ detector

2011

""ARGO-YBJ is an extensive air shower detector located at the Yangbajing Cosmic Ray Laboratory (4300 ma.s.l., 606 g cm^−2 atmospheric depth, Tibet, China).. It is made by a single layer of Resistive Plate Chambers. (RPCs, total surface ~ 6700 m^2) grouped into 153 units. called “clusters”. The low energy threshold of the experiment is obtained using the ”scaler operation mode”, counting all the particles hitting the detector without reconstruction of the shower size and arrival direction. For each cluster the signals generated by these particles are put in coincidence in a narrow time window (150 ns) and read by four independent. scaler channels, giving the counting rates of channel. >= 1, …

PhysicsResistive touchscreenPhysics and Astronomy (miscellaneous)Atmospheric pressureSettore FIS/01 - Fisica SperimentaleDetectorScaler ModeAstronomy and AstrophysicsCosmic rayRadioactivity Array Detector Scaler ModeArray DetectorCoincidenceComputational physicsRadioactivityAir showerCoincidentArgo
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Laboratory astrophysics survey of key x-ray diagnostic lines using a microcalorimeter on an electron beam ion trap

2000

Cosmic plasma conditions created in an electron beam ion trap (EBIT) make it possible to simulate the dependencies of key diagnostic X-ray lines on density, temperature, and excitation conditions that exist in astrophysical sources. We used a microcalorimeter for such laboratory astrophysics studies because it has a resolving power ≈1000, quantum efficiency approaching 100%, and a bandwidth that spans the X-ray energies from 0.2 keV to 10 keV. Our microcalorimeter, coupled with an X-ray optic to increase the effective solid angle, provides a significant new capability for laboratory astrophysics measurements. Broadband spectra obtained from the National Institute of Standards and Technology…

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementFizikai tudományokAstrophysicsSpectral lineNeonTermészettudományokAtomic processeIonizationPhysics::Atomic PhysicsAtomic dataNuclear and High Energy PhysicPhysicsArgonKryptonAstronomy and AstrophysicsLine: IdentificationPlasmaX-rays: GeneralchemistrySpace and Planetary ScienceAstrophysical plasmaMethods: Laboratory plasmaAtomic physicsElectron beam ion trap
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Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays

2021

This work would not have been possible without the support of the Swiss National Science Foundation, Switzerland; CEA and CNRS/IN2P3, France; KEK and the JSPS program, Japan; Ministerio de Ciencia e Innovacion in Spain under grants FPA2016-77347-C2, SEV-2016-0588 and MdM-2015-0509, Comunidad de Madrid, the CERCA program of the Generalitat de Catalunya and the fellowship (LCF/BQ/DI18/11660043) from "La Caixa" Foundation (ID 100010434); the Programme PNCDI III, CERN-RO, under Contract 2/2020, Romania; the U.S. Department of Energy under Grant No. DE-SC0011686. This project has received funding from the European Union's Horizon 2020 Research and Innovation program under Grant Agreement no. 654…

Physics::Instrumentation and DetectorsLibrary scienceargon: gas01 natural sciences7. Clean energyNeutrino detectorArgon gasPolitical scienceParticle tracking detectors0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]media_common.cataloged_instanceNeutrino detectors[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]European union010306 general physicsInstrumentationMathematical Physicsmedia_common010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsTime projection Chambers (TPC)time projection chamber: liquid argonParticle tracking detectorTime projection chambercosmic radiationLarge detector systems for particle and astroparticle physicyield: stabilityLiquid argonperformance
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The mass-hierarchy and CP-violation discovery reach of the LBNO long-baseline neutrino experiment.

2014

The next generation neutrino observatory proposed by the LBNO collaboration will address fundamental questions in particle and astroparticle physics. The experiment consists of a far detector, in its first stage a 20 kt LAr double phase TPC and a magnetised iron calorimeter, situated at 2300 km from CERN and a near detector based on a high-pressure argon gas TPC. The long baseline provides a unique opportunity to study neutrino flavour oscillations over their 1st and 2nd oscillation maxima exploring the $L/E$ behaviour, and distinguishing effects arising from $\delta_{CP}$ and matter. In this paper we have reevaluated the physics potential of this setup for determining the mass hierarchy (M…

Physics::Instrumentation and Detectorsfar detectorkaukoputket ja teleskoopit7. Clean energyviolation [CP]CP violation; Neutrino Detectors and Telescopes; Oscillation; Nuclear and High Energy PhysicsHigh Energy Physics - Phenomenology (hep-ph)Observatorymass: hierarchy [neutrino]detector [neutrino]QCPhysicsTime projection chamberLarge Hadron ColliderOscillationmagnetization [iron]oscillation [neutrino]High Energy Physics - PhenomenologyCP violationliquid argon [time projection chamber]CP violationNeutrinoParticle physicsNuclear and High Energy PhysicsCERN Lab530 PhysicseducationFOS: Physical sciencesddc:500.2oscillation [flavor]114 Physical sciencesNuclear physicsphase spacenear detectorstatistical analysisiron [calorimeter]Particle Physics - PhenomenologyAstroparticle physicsNeutrino Detectors and Telescopesta114Físicaflavor [neutrino]CP [phase]CERN SPSMODELproposed [observatory]Oscillation13. Climate actionPhase space[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]gas [argon]beam [neutrino]High Energy Physics::ExperimentMATTERneutrino detectorsCP violation.
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Szukając wolności: Sprawa kapitana m/s "Batory" Jana Ćwiklińskiego

2014

After WWII the Polish ocean liner “Batory” operated on the route Gdynia–New York, and from 1951 to India. The captain of the ship was Jan Ćwikliński. The Ministry for Public Security accused him of having a hostile attitude towards the People’s Republic of Poland and insisted on him being removed from his position as Batory captain. In the spring of 1953 the ship underwent a technical check-up at a shipyard in Great Britain. In the mean-time it was rumoured that the captain was to be arrested upon his return to Poland on suspicion of espionage. When the renovation works were about to be completed, Ćwikliński decided to escape and left his ship for good. The captain was given political asylu…

Polskie Linie Oceanicznethe Pulaski Transort Linethe Ministry for Public Securitythe Polish Ocean Linesstatek towarowy „Wolna Polska”Ministerstwo Bezpieczeństwa Publiczneg oPolish ocean linerspolska emigracja polityczna po drugiej wojnie świa- towejfugitives from the People’s Republic of Polandthe cargo ship “Wolna Polska” [Eng. “Free Po- land”]polskie transatlantykiPulaski Transport LinePolish political emigration aft er WWIIthe Stalin perioduciekinierzy z PRLepoka stalinowskaZapiski Historyczne (main title). Poświęcone historii Pomorza i krajów bałtyckich (subtitle)
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