Search results for " Detectors"

showing 10 items of 2027 documents

Improvement in fast particle track reconstruction with robust statistics

2014

The IceCube project has transformed one cubic kilometer of deep natural Antarctic ice into a Cherenkov detector. Muon neutrinos are detected and their direction inferred by mapping the light produced by the secondary muon track inside the volume instrumented with photomultipliers. Reconstructing the muon track from the observed light is challenging due to noise, light scattering in the ice medium, and the possibility of simultaneously having multiple muons inside the detector, resulting from the large flux of cosmic ray muons. This manuscript describes work on two problems: (1) the track reconstruction problem, in which, given a set of observations, the goal is to recover the track of a muo…

Nuclear and High Energy PhysicsParticle physicsCherenkov detectorPhysics::Instrumentation and DetectorsFOS: Physical sciencesddc:500.2Neutrino telescopeTrack reconstructionlaw.inventionIceCubelawCoincidentAngular resolutionddc:530InstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)Remote sensingIce CubePhysicsMuonTrack (disk drive)DetectorIceCube; Neutrino astrophysics; Neutrino telescope; Robust statistics; Track reconstructionRobust statisticsNeutrino astrophysicsNeutrino detectorHigh Energy Physics::ExperimentNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Measurement of $ZZ$ production in $pp$ collisions at $\sqrt{s}=7$ TeV and limits on anomalous $ZZZ$ and $ZZ\gamma$ couplings with the ATLAS detector

2013

Journal of High Energy Physics 2013.3 (2013): 128 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)

Nuclear and High Energy PhysicsParticle physicsCiências Naturais::Ciências FísicasPhysics::Instrumentation and Detectors:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2Hadron-hadron scattering01 natural sciences7. Clean energy530High Energy Physics - ExperimentStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530High Energy Physics010306 general physicsQCCiencias ExactasBosonPhysicsQuantum chromodynamicsGauge bosonMuonLarge Hadron ColliderScience & TechnologyHadron-Hadron ScatteringATLAS detector010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleATLAS experimentHigh Energy Physics::PhenomenologyFísicaNEW PHYSICSATLASZZ productionsZ BOSONHADRON-HADRON COLLISIONSPhysics::Accelerator Physicsproton-proton collisionsHigh Energy Physics::ExperimentLHCNeutrinoParticle Physics - Experiment
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The Hunt for New Physics at the Large Hadron Collider

2010

233 páginas.-- AHEP Group: et al..-- El Pdf del artículo es la versión pre-print: arXiv.1001.2693v1.-- Trabajo presentado al "The International Workshop on Beyond the Standard Model Physics and LHC Signatures (BSM-LHC) celebrado en Boston (USA) del 2 al 4 de junio de 2009.

Nuclear and High Energy PhysicsParticle physicsCold dark matterPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciencesRANDALL-SUNDRUM MODEL01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)R-PARITY BREAKING0103 physical sciencesHigh Energy PhysicsANOMALOUS MAGNETIC-MOMENT010306 general physicsParticle Physics - PhenomenologyPhysicsEXPLICIT CP VIOLATIONDARK-MATTER DETECTIONLarge Hadron Collider010308 nuclear & particles physicsPhysicsElectroweak interactionHigh Energy Physics::PhenomenologyFísicaRENORMALIZATION-GROUP EQUATIONSHierarchy problemSupersymmetryAtomic and Molecular Physics and OpticsGRAND UNIFIED THEORIESSUPERSYMMETRIC STANDARD MODELHidden sectorExtra dimensionsHigh Energy Physics - PhenomenologyMINIMAL FLAVOR VIOLATION[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentHIGGS-BOSON PRODUCTION
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Implementation and performance of the third level muon trigger of the ATLAS experiment at LHC

2006

The trigger system of the ATLAS experiment at the LHC aims at a high selectivity in order to keep the full physics potential while reducing the 40 MHz initial event rate imposed by the LHC bunch crossing down to /spl sim/100 Hz, as required by the data acquisition system. Algorithms working in the final stage of the trigger environment (Event Filter) are implemented to run both in a "wrapped" mode (reconstructing tracks in the entire Muon Spectrometer) and in a "seeded" mode (according to a dedicated strategy that performs pattern recognition only in regions of the detector where trigger hypotheses have been produced at earlier stages). The working principles of the offline muon reconstruct…

Nuclear and High Energy PhysicsParticle physicsHLTPhysics::Instrumentation and DetectorsMuonReal-time computingevent filter01 natural sciencesData acquisitionAtlas (anatomy)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]medicineElectrical and Electronic EngineeringDiscrete event simulationDetectors and Experimental TechniquesPhysicsMuonsLarge Hadron Collider010308 nuclear & particles physicsEvent (computing)DetectorATLAS experimentMuons.ATLASTriggermedicine.anatomical_structureNuclear Energy and EngineeringFilter (video)Event Filter
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Flavour in heavy neutrino searches at the LHC

2012

Heavy neutrinos at the TeV scale have been searched for at the LHC in the context of left-right models, under the assumption that they couple to the electron, the muon, or both. We show that current searches are also sensitive to heavy neutrinos coupling predominantly to the tau lepton, and present limits can significantly constrain the parameter space of general flavour mixing.

Nuclear and High Energy PhysicsParticle physicsLHC (Large Hadron Collider)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHeavy neutrinoFOS: Physical sciencesContext (language use)ElectronParameter space01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsMixing (physics)PhysicsMuonLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoLepton
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The neutron background of the XENON100 dark matter search experiment

2013

TheXENON100 experiment, installed underground at the LaboratoriNazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering off xenon nuclei. This paper presents a study on the nuclear recoil background of the experiment, taking into account neutron backgrounds from (alpha, n) reactions and spontaneous fission due to natural radioactivity in the detector and shield materials, as well as muon-induced neutrons. Based on MonteCarlo simulations and using measured radioactive contaminations of all detector components, we predict the nuclear recoil backgrounds for the WIMP search results published by theXENO…

Nuclear and High Energy PhysicsParticle physicsLarge Underground Xenon experimentPhysics::Instrumentation and DetectorsDark matterGeant4Astrophysics::Cosmology and Extragalactic AstrophysicsWIMP Argon Programme01 natural sciencesNuclear physicsWIMPNuclear and High Energy Physics Neutron Background Dark Matter Search XENON TPC0103 physical sciencesNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSSpontaneous fissionPhysicsElastic scatteringFluxMuons010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsWeakly interacting massive particlesHigh Energy Physics::ExperimentSimulation
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Detecting the long-distance structure of the X(3872)

2014

We study the X(3872)-->D^0 \bar D^0 \pi^0 decay within a D \bar D^* molecular picture for the X(3872) state. This decay mode is more sensitive to the long-distance structure of the X(3872) resonance than its J/\psi\pi\pi and J/\psi3\pi decays, which are mainly controlled by the details of the X(3872) wave function at short distances. We show that the D^0 \bar D^0 final state interaction can be important, and that a precise measurement of this partial decay width can provide valuable information on the interaction strength between the D^{(*)} \bar D^{(*)} charm mesons.

Nuclear and High Energy PhysicsParticle physicsMeson[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th][SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Structure (category theory)FOS: Physical sciencesInteraction strength01 natural sciencesHigh Energy Physics - Experiment[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsWave functionComputer Science::DatabasesPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyResonanceFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentBar (unit)X(3872)
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Search for massive long-lived highly ionising particles with the ATLAS detector at the LHC

2011

A search is made for massive highly ionising particles with lifetimes in excess of 100 ns, with the ATLAS experiment at the Large Hadron Collider, using 3.1 pb-1 of pp collision data taken at √s = 7TeV. The signature of energy loss in the ATLAS inner detector and electromagnetic calorimeter is used. No such particles are found and limits on the production cross section for electric charges 6e ≤ |q| ≤ 17e and masses 200 GeV ≤ m ≤ 1000 GeV are set in the range 1–12 pb for different hypotheses on the production mechanism.

Nuclear and High Energy PhysicsParticle physicsNew PhysicsCiências Naturais::Ciências FísicasPhysics::Instrumentation and DetectorsPhysics beyond the Standard Model:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesHigh-energy collider experiment; Long-lived particle; Highly ionising; New physicsHigh-energy collider experimentddc:500.253001 natural sciencesHigh Energy Physics - ExperimentNuclear physicslong-lived particle; high-energy collider experiment; new physics; highly ionisingHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)0103 physical sciencesMASSIVE CHARGED PARTICLESmedicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530High Energy PhysicsHighly ionisingNew physics010306 general physicsNuclear ExperimentPhysicsRange (particle radiation)Large Hadron ColliderScience & Technology010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorATLAS experimentDrell–Yan processFísicaATLASLong-lived particleTransition radiation detectormedicine.anatomical_structureExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentLHCParticle Physics - Experiment
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Solar Neutrinos Before and After Neutrino 2004

2004

We compare, using a three neutrino analysis, the allowed neutrino oscillation parameters and solar neutrino fluxes determined by the experimental data available Before and After Neutrino 2004. New data available after Neutrino2004 include refined KamLAND and gallium measurements. We use six different approaches to analyzing the KamLAND data. We present detailed results using all the available neutrino and anti-neutrino data for Delta m^2_{12}, tan^2 theta_{12}, sin^2 theta_{13}, and sin^2 eta (sterile fraction). Using the same complete data sets, we also present Before and After determinations of all the solar neutrino fluxes, which are treated as free parameters, an upper limit to the lumi…

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyLuminosityNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentPhysicsStandard solar model010308 nuclear & particles physicsScatteringOscillationAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSigmaHigh Energy Physics - Phenomenology13. Climate actionHigh Energy Physics::ExperimentNeutrino
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Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II

2009

The AMANDA-II detector, operating since 2000 in the deep ice at the geographic South Pole, has accumulated a large sample of atmospheric muon neutrinos in the 100 GeV to 10 TeV energy range. The zenith angle and energy distribution of these events can be used to search for various phenomenological signatures of quantum gravity in the neutrino sector, such as violation of Lorentz invariance (VLI) or quantum decoherence (QD). Analyzing a set of 5511 candidate neutrino events collected during 1387 days of livetime from 2000 to 2006, we find no evidence for such effects and set upper limits on VLI and QD parameters using a maximum likelihood method. Given the absence of evidence for new flavor-…

Nuclear and High Energy PhysicsParticle physicsOscillationsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaConfidence-IntervalsGravityFOS: Physical sciencesGeneratorLorentz covariance01 natural sciences7. Clean energyHigh Energy Physics - ExperimentScatteringHigh Energy Physics - Experiment (hep-ex)SensitivityQuantum Decoherence0103 physical sciencesddc:530Muon neutrino010306 general physicsNeutrino oscillationTelescopeAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSmall SignalsLorentz Invariance Violation
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