Search results for " DETECTOR"

showing 10 items of 2719 documents

Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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Response of AGATA segmented HPGe detectors to gamma rays up to 15.1MeV

2013

WOS: 000314826000009

AGATA; Gamma-ray spectroscopy; Gamma-ray tracking; HPGe detectors; Pulse-shape and gamma-ray tracking algorithms; Semiconductor detector performance and simulationsNuclear and High Energy PhysicsPulse-shape and gamma-ray tracking algorithmsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSemiconductor detector performance and simulationsTracking (particle physics)01 natural sciencesNuclear physicsGamma-ray tracking0103 physical sciencesGamma spectroscopyddc:530Gamma-ray spectroscopyNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationNuclear ExperimentDetectors de radiacióPhysicsSpectrometer010308 nuclear & particles physicsDetectorHPGe detectorsGamma ray81V35Semiconductor detectorAGATAFísica nuclearHpge detectorAGATA
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Production of 4He and 4He_ in Pb–Pb collisions at √sNN = 2.76 TeV at the LHC

2018

Results on the production of 4He and 4He nuclei in Pb–Pb collisions at √sNN = 2.76 TeV in the rapidity range | y |< 1, using the ALICE detector, are presented in this paper. The rapidity densities corresponding to 0–10% central events are found to be dN/dy4He = (0.8 ± 0.4 (stat) ± 0.3 (syst)) × 10−6 and dN/dy4He = (1.1 ± 0.4 (stat) ± 0.2 (syst)) × 10−6, respectively. This is in agreement with the statistical thermal model expectation assuming the same chemical freeze-out temperature (Tchem = 156 MeV) as for light hadrons. The measured ratio of 4He/4He is 1.4 ± 0.8 (stat) ± 0.5 (syst). peerReviewed

ALICE detectorPb–Pb collisionsAnti-nucleiLHC
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Heavy flavour decay muon production at forward rapidity in proton--proton collisions at sqrt(s) = 7 TeV

2012

The production of muons from heavy flavour decays is measured at forward rapidity in proton-proton collisions at $\sqrt{s} = 7$ TeV collected with the ALICE experiment at the LHC. The analysis is carried out on a data sample corresponding to an integrated luminosity $L_{\rm int} = 16.5$ nb$^{-1}$. The transverse momentum and rapidity differential production cross sections of muons from heavy flavour decays are measured in the rapidity range 2.5 &lt; y &lt; 4, over the transverse momentum range 2 &lt; $p_{\rm T}$ &lt; 12 GeV/$c$. The results are compared to predictions based on perturbative QCD calculations.

ALICE experiment; P-P collisions; Heavy flavour muon decayProtonAlicePhysics::Instrumentation and DetectorsHeavy flavour muon decayheavy flavour01 natural sciencesPp CollisionsSingle MuonsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEHeavy Flavour Production[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentAlice ExperimentALICE experiment; Heavy flavour production; LHC; Pp collisions; Single muons; Nuclear and High Energy PhysicsP-P collisionsQuantum chromodynamicsPhysicsLarge Hadron ColliderLuminosity (scattering theory)PhysicsProduction Cross-SectionPerturbative QCDP-P collisionP(P)Over-Bar CollisionsLHC ALICE experiment pp collisions Single muons Heavy flavour productionLHCLhcpp collisionsParticle Physics - ExperimentHeavy flavour productionParticle physicsNuclear and High Energy PhysicsLHC; ALICE; heavy flavourFOS: Physical sciencesalice experiment; pp collisions; heavy flavour production; single muons; lhcNuclear physicsmuon0103 physical sciencesALICE; heavy flavour; muonRapidity010306 general physicsHadron-CollisionsMuonta114Bottom-Quark Production010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyALICE; LHC; CERN; strange particle; pp; 7 TeV; Heavy flavour production; Single muonsALICE experimentSingle muonsJ/Psi ProductionHigh Energy Physics::ExperimentLepton
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On the selection of AGN neutrino source candidates for a source stacking analysis with neutrino telescopes

2006

The sensitivity of a search for sources of TeV neutrinos can be improved by grouping potential sources together into generic classes in a procedure that is known as source stacking. In this paper, we define catalogs of Active Galactic Nuclei (AGN) and use them to perform a source stacking analysis. The grouping of AGN into classes is done in two steps: first, AGN classes are defined, then, sources to be stacked are selected assuming that a potential neutrino flux is linearly correlated with the photon luminosity in a certain energy band (radio, IR, optical, keV, GeV, TeV). Lacking any secure detailed knowledge on neutrino production in AGN, this correlation is motivated by hadronic AGN mode…

AMANDAActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsIceCubeLuminosityAGNNeutrinosBlazarAstrophysics::Galaxy AstrophysicsAGN; AMANDA; IceCube; Neutrinos; Point sources; Source stackingAstroparticle physicsPhysicsAstrophysics (astro-ph)Point sourcesAstronomyAstronomy and AstrophysicsQuasarSource stackingNeutrino detectorAstronomiaHigh Energy Physics::ExperimentNeutrino
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The IceCube data acquisition system: Signal capture, digitization, and timestamping

2008

IceCube is a km-scale neutrino observatory under construction at the South Pole with sensors both in the deep ice (InIce) and on the surface (IceTop). The sensors, called Digital Optical Modules (DOMs), detect, digitize and timestamp the signals from optical Cherenkov-radiation photons. The DOM Main Board (MB) data acquisition subsystem is connected to the central DAQ in the IceCube Laboratory (ICL) by a single twisted copper wire-pair and transmits packetized data on demand. Time calibration is maintained throughout the array by regular transmission to the DOMs of precisely timed analog signals, synchronized to a central GPS-disciplined clock. The design goals and consequent features, func…

AMANDANuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesAstrophysicsNeutrino telescopeSignalHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryNuclear physicsHigh Energy Physics - Experiment (hep-ex)IcecubeData acquisitionSignal digitizationddc:530Nuclear Experiment (nucl-ex)Nuclear ExperimentInstrumentationPhysicsbusiness.industryAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAMANDA; Icecube; Neutrino telescope; Signal digitizationTimestampingInstrumentation and Detectors (physics.ins-det)Analog signalTransmission (telecommunications)Systems designTimestampbusinessComputer hardware
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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Acoustic characterization of Silica aerogel clamped plates for perfect absorption purpose

2017

International audience; Silica aerogel has been widely studied as bulk material for its extremely low density and thermal conductivity. Plates or membranes made of this extremely soft materials exhibits interesting properties for sound absorption. A novel signal processing method for the characterization of an acoustic metamaterial made of silica aerogel clamped plates is presented. The acoustic impedance of a silica aerogel clamped plate is derived from the elastic theory for the flexural waves, while the transfer matrix method is used to model reflection and transmission coefficients of a single plate. Experimental results are obtained by using an acoustic impedance tube. The difference b…

Absorption (acoustics)Materials scienceAcoustics and UltrasonicsPhysics::Instrumentation and DetectorsTransfer-matrix method (optics)Physics::Optics01 natural sciencesCondensed Matter::Disordered Systems and Neural Networks03 medical and health sciences0302 clinical medicineThermal conductivityArts and Humanities (miscellaneous)0103 physical sciencesReflection coefficientComposite material030223 otorhinolaryngology010301 acousticsComputingMilieux_MISCELLANEOUSMetamaterialAerogel[PHYS.MECA]Physics [physics]/Mechanics [physics][PHYS.MECA.ACOU]Physics [physics]/Mechanics [physics]/Acoustics [physics.class-ph]Condensed Matter::Soft Condensed MatterReflection (mathematics)[PHYS.MECA] Physics [physics]/Mechanics [physics]Acoustic impedance[PHYS.MECA.ACOU] Physics [physics]/Mechanics [physics]/Acoustics [physics.class-ph]
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Design study for a 500 MeV positron beam at the Mainz Microtron MAMI

2022

A design study has been performed for a positron beam with an energy of 500 MeV to be realized at the applied physics area of the Mainz Microtron MAMI. Positrons will be created after pair conversion of bremsstrahlung, produced by the 855 MeV electron beam af MAMI in a tungsten converter target. From the two conceivable geometries (i) pair conversion in the bremsstrahlung converter target itself, and (ii) bremsstrahlung pair conversion in a separated lead foil, the former was considered in detail. Positrons will be energy selected within an outside open electron beam-line bending magnet, and bent back by an additional sector magnet. Magnetic focusing elements in between are designed to prep…

Accelerator Physics (physics.acc-ph)530 PhysicsPhysics::Instrumentation and DetectorsPhysics::Accelerator PhysicsFOS: Physical sciencesPhysics - Accelerator Physics530 PhysikNuclear ExperimentAtomic and Molecular Physics and Optics
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Fast photon detection for particle identification with COMPASS RICH-1

2006

Particle identification at high rates is an important challenge for many current and future high-energy physics experiments. The upgrade of the COMPASS RICH-1 detector requires a new technique for Cherenkov photon detection at count rates of several $10^6$ per channel in the central detector region, and a read-out system allowing for trigger rates of up to 100 kHz. To cope with these requirements, the photon detectors in the central region have been replaced with the detection system described in this paper. In the peripheral regions, the existing multi-wire proportional chambers with CsI photocathode are now read out via a new system employing APV pre-amplifiers and flash ADC chips. The ne…

Accelerator Physics (physics.acc-ph)Nuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsCherenkov detectorOther Fields of PhysicsFOS: Physical sciencesCOMPASS; RICH; Multi-anode PMT; Particle identificationCOMPASSParticle identificationPhotocathodelaw.inventionParticle identificationNuclear physicsOpticsMulti-anode PMTlawCompassCOMPASS; RICHInstrumentationRICHCherenkov radiationPhysicsbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)UpgradePhysics - Accelerator PhysicsHigh Energy Physics::Experimentbusiness
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