Search results for "Argo"

showing 10 items of 424 documents

Gamma ray sources observation with the ARGO-YBJ detector

2011

In this paper we report on the observations of TeV gamma ray sources performed by the air shower de- tector ARGO-YBJ. The objects studied in this work are the blazar Markarian 421 and the extended galactic source MGROJ1908+06, monitored during 2 years of operation. Mrk421 has been detected by ARGO-YBJ with a statisti- cal significance of 11 standard deviations. The observed TeV emission was highly variable, showing large enhance- ments of the flux during active periods. The study of the spectral behaviour during flares revealed a positive correla- tion of the hardness with the flux, as already reported in the past by the Whipple telescope, suggesting that this is a long term property of the…

PhysicsNuclear and High Energy PhysicsGamma AstronomyPhysics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaDetectorGamma rayFluxAstronomyExtensive Air ShowerAstronomy and AstrophysicsAstrophysicsGamma-ray astronomyArray DetectorGamma-RayArgo-YbjGamma Astronomy Array DetectorCrab NebulaAir showerPulsarMilagroBlazarInstrumentationArgoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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The ARGO-YBJ experiment in Tibet

2008

The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet, P.R. China) has been completed during the last spring (2007). It consists of a central carpet made of 130 identical sub-units of 12 RPCs each (a "cluster"), covering a surface of about 5800 m2 with 93% active area, and a guard ring of 24 further clusters of the same type surrounding the central carpet with a lower sampling density. Signals are picked up by external electrodes of small size, thus allowing the sampling of EAS with high space-time granularity. Shower events are detected at a trigger rate of about 4 kHz. Events with a few particles detected by a single cluster are counted in scale…

PhysicsNuclear and High Energy PhysicsGamma ray burstSingle clusterTrigger rateDetectorgamma ray bursts gamma rays cosmic rays extended air showersAstronomySampling (statistics)Cosmic rayExtended air showers Cosmic rays Gamma ray sources Gamma ray burstsGamma ray sourcesGeodesyCosmic rayGuard ringExtended air showerSampling densityInstrumentationArgoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Direct mass measurements of unstable rare earth isotopes with the ISOLTRAP mass spectrometer

1996

Abstract Direct mass measurements of neutron deficient rare earth isotopes in the vicinity of 146 Gd were performed for the first time with the Penning trap mass spectrometer ISOLTRAP at ISOLDE/CERN. Since ISOL-facilities deliver these isotopes with a large amount of isobaric contamination, these measurements became possible only after the installation of a new cooler trap which acts as an isobar separator. To date more than 40 isotopes of the elements Pr, Nd, Pm, Sm, Eu, Dy, and Ho have been measured with a typical accuracy of δm ≈ 14 keV. Some of these isotopes provide an important anchor for many other isotopes linked by known Q-values.

PhysicsNuclear and High Energy PhysicsIsotope010308 nuclear & particles physicsIsotopes of argon[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Mass spectrometryPenning trap01 natural sciences7. Clean energyISOLTRAPIsotopes of oxygenIsotopes of nitrogenNuclear physics13. Climate action0103 physical sciencesNeutronAtomic physics010306 general physicsNuclear Physics A
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Liquid argon calorimeter performance at high rates

2012

Abstract We project the performance of the ATLAS liquid argon endcap and forward calorimeters at the planned high luminosity LHC option HL-LHC by exposing small calorimeter modules of the electromagnetic, hadronic, and forward calorimeters to high intensity beams at IHEP/Protvino. The beam intensity extends well beyond the maximum expected for these calorimeters at HL-LHC. The signal reconstruction and calorimeter performance have been studied in full detail.

PhysicsNuclear and High Energy PhysicsLarge Hadron ColliderArgonLuminosity (scattering theory)Physics::Instrumentation and Detectorschemistry.chemical_elementCryogenicsCalorimeterNuclear physicsmedicine.anatomical_structurechemistryAtlas (anatomy)medicineMeasuring instrumentPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentInstrumentationBeam (structure)Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Nuclear moments and charge radii of argon isotopes between the neutron-shell closures and

2008

We report the measurement of optical isotope shifts for 40−44 Ar relative to 38 Ar from which changes in the mean square nuclear charge radii across the 1f7/2 neutron shell are deduced. In addition, the hyperfine structure of 41 Ar and 43 Ar yields the spins, magnetic dipole and electric quadrupole moments, in particular the spin I = 5/2 for 43 Ar. The investigations were carried out by fast-beam collinear laser spectroscopy using highly sensitive detection based on optical pumping and state-selective collisional ionization. Mean square charge radii are now known from 32 Ar to 46 Ar, covering sd-shell as well as f7/2-shell nuclei. They are discussed in the framework of spherical SGII Skyrme…

PhysicsNuclear and High Energy PhysicsNuclear TheoryIsotopes of argonEffective nuclear chargeIonizationPhysics::Space PhysicsQuadrupoleAstrophysics::Solar and Stellar AstrophysicsNeutronAtomic physicsSpectroscopyMagnetic dipoleHyperfine structureNuclear Physics A
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Gamow-Teller transitions in theA=40isoquintet of relevance for neutrino captures inAr40

2014

Background: The Gamow-Teller response of $^{40}\mathrm{Ar}$ is important for the use of liquid argon as a medium for neutrino detection. An ambiguity about the Gamow-Teller strength for the excitation of ${1}^{+}$ states at 2290 and 2730 keV in $^{40}\mathrm{K}$ results in a significant uncertainty for neutrino capture rates. This ambiguity is caused by the large discrepancy observed between strengths extracted from $^{40}\mathrm{Ar}$($p$, $n$) charge-exchange data and the transition strengths for the analog transitions studied in the $\ensuremath{\beta}$ decay of $^{40}\mathrm{Ti}$.Purpose: This study was aimed at resolving the ambiguity between the results from the $^{40}\mathrm{Ar}$($p$,…

PhysicsNuclear and High Energy PhysicsParticle physicsAmplitudeSHELL modelLiquid argonNeutrinoBorn approximationEnergy (signal processing)ExcitationNeutrino scatteringPhysical Review C
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Theoretical uncertainties on quasielastic charged-current neutrino–nucleus cross sections

2006

We estimate the theoretical uncertainties of the model developed in Phys. Rev. C70 055503 for inclusive quasielastic charged-current neutrino-nucleus reactions at intermediate energies. Besides we quantify the deviations of the predictions of this many body framework from those obtained within a simple Fermi gas model. An special attention has been paid to the ratio \sigma(\mu)/\sigma(e) of interest for experiments on atmospheric neutrinos. We show that uncertainties affecting this ratio are likely smaller than 5%

PhysicsNuclear and High Energy PhysicsParticle physicsArgonNuclear TheoryMany-body theorychemistry.chemical_elementFísicaFOS: Physical sciencesMany bodyNeutrino scatteringNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenologymedicine.anatomical_structureHigh Energy Physics - Phenomenology (hep-ph)chemistrymedicineNeutrinoFermi gasNucleusCharged currentPhysics Letters B
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Nachweis der Mehrfachemission von Sekund�relektronen mittels Proportionalz�hlrohr

1965

A proportional counter is used as analyser for electron energies (in the range 10 to 20 keV). The resolving power for 20 keV is 21%. The multiple emission of secondary electrons is investigated with this counter.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)ArgonAstrophysics::High Energy Astrophysical PhenomenaElectron multiplierAnalyserchemistry.chemical_elementProportional counterElectronSecondary electronschemistrySecondary emissionAtomic physicsZeitschrift f�r Physik
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Laser driven X-ray parametric amplification in neutral gases—a new brilliant light source in the XUV

2011

Abstract In this paper we present the experimental setup and results showing a new type of strong-field parametric amplification of high-order harmonic radiation. With a simple semi-classical model, we can identify the most important experimental parameters, the spectral range and the small signal gain in gases. Using a single stage amplifier, a small signal gain of 8000 has been obtained in argon for the spectral range of 40–50 eV, using 350 fs, 7 mJ pulses at 1.05 μm. An outlook for an experiment employing a double stage gas system will be given.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Argonbusiness.industryAmplifierX-raychemistry.chemical_elementLaserOptical parametric amplifierlaw.inventionOpticschemistrylawExtreme ultravioletbusinessInstrumentationParametric statisticsNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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A purity monitoring system for liquid argon calorimeters

2005

Abstract For liquid argon calorimeters electronegative impurities dissolved in the medium degrade the detector response and deteriorate the energy resolution, especially at high energies. A concept for a purity monitoring system for liquid argon calorimeters has been developed and is presented here. Special combined monitors of 241 Am- and 207 Bi-cells are used to monitor the concentration of impurities. The working principle as well as results from test measurements are discussed.

PhysicsNuclear and High Energy PhysicsResolution (mass spectrometry)Physics::Instrumentation and DetectorsImpurityDetectorElectron attachmentAnalytical chemistryLiquid argonHigh Energy Physics::ExperimentMonitoring systemPhysics::Chemical PhysicsInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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