Search results for "Instrumentation and Detectors"

showing 3 items of 1873 documents

Excess electronic recoil events in XENON1T

2020

We report results from searches for new physics with low-energy electronic recoil data recorded with the XENON1T detector. With an exposure of 0.65 t-y and an unprecedentedly low background rate of $76\pm2$ events/(t y keV) between 1 and 30 keV, the data enables sensitive searches for solar axions, an enhanced neutrino magnetic moment, and bosonic dark matter. An excess over known backgrounds is observed at low energies and most prominent between 2 and 3 keV. The solar axion model has a 3.4$\sigma$ significance, and a 3D 90% confidence surface is reported for axion couplings to electrons, photons, and nucleons. This surface is inscribed in the cuboid defined by $g_{ae}<3.8 \times 10^{-12}$,…

xenon: targetaxionssolar axionmagnetic momentdimension: 3neutrino: solarPhysics beyond the Standard ModelSolar neutrinodark matter: direct detection01 natural sciences7. Clean energyHigh Energy Physics - ExperimentDark matter direct detection axionHigh Energy Physics - Experiment (hep-ex)neutrinoXENONHigh Energy Physics - Phenomenology (hep-ph)background: lowRecoilelectron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]beta-raysParticle Physics Experimentscoupling: (axion 2electron)multi-purpose particle detectornuclear instrumentationComputingMilieux_MISCELLANEOUSinstrumentationPhysicsxenon: liquidboson: dark matteraxion 2nucleontritiumnew physics: search forsemileptonic decayboson: vectortensionneutrino: magnetic momentHigh Energy Physics - Phenomenologyaxion 2photonlow backgroundbosonNeutrinoionizing radiationNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)dark matter detectorelectronic recoilElectron captureXENON1T detectorDark matterlow-energy electronic recoil dataFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]dark matterNONuclear physicsPE2_2PE2_1tritium: semileptonic decay0103 physical sciencessolar axion modelsurface[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]axion: couplingPE2_4010306 general physicspseudoscalarAxiondark matter: vectordark matter XENON1T detector electronic recoilsolar neutrinodetectorDark Matter Axions Beta Decay Liquid Xenon TPC010308 nuclear & particles physicsaxion 2electroncoupling: (axion 2nucleon)dark matter: detectormodel: axionGran Sassometrology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]axionstellar constraintscoupling: (axion 2photon)High Energy Physics::Experimentparticle dark matterdirect detectionbeta decayaxion: solar[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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Beam-induced and cosmic-ray backgrounds observed in the ATLAS detector during the LHC 2012 proton-proton running period

2016

This paper discusses various observations on beam-induced and cosmic-ray backgrounds in the ATLAS detector during the LHC 2012 proton-proton run. Building on published results based on 2011 data, the correlations between background and residual pressure of the beam vacuum are revisited. Ghost charge evolution over 2012 and its role for backgrounds are evaluated. New methods to monitor ghost charge with beam-gas rates are presented and observations of LHC abort gap population by ghost charge are discussed in detail. Fake jets from colliding bunches and from ghost charge are analysed with improved methods, showing that ghost charge in individual radio-frequency buckets of the LHC can be resol…

Большой адронный коллайдерbackground [beam]Physics::Instrumentation and DetectorsMonte Carlo methodPerformance of high energy physics detectorJet (particle physics)01 natural sciencesHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)pressureSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Instrumentationпротон-протонные столкновенияQCMathematical PhysicsPhysicseducation.field_of_studyPerformance of high energy physics detectorsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleBeam-intensity monitors; Beam-line instrumentation (beam position and profile monitors; Bunch length monitors); Data analysis; Performance of high energy physics detectors; Instrumentation; Mathematical PhysicsData analysiMonte Carlo [numerical calculations]ATLASbuildingsBunchesCERN LHC CollBeam-intensity monitorBeam-line instrumentation (beam position and profile monitorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGcolliding beams [p p]Particle Physics - ExperimentParticle physicsCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical PhenomenaPopulation:Ciências Físicas [Ciências Naturais]Beam-line instrumentation (beam position and profile monitorsData analysisFOS: Physical sciencesgapCosmic ray530Bunch length monitors)Nuclear physicsATLAS LHC High Energy Physics510 Mathematics0103 physical sciencesBeam-line instrumentation (beam position and profile monitors;; beam-intensity monitors; bunch length monitors); Data analysis;; Performance of High Energy Physics Detectors; LEPHigh Energy Physicsddc:610010306 general physicseducationMuonScience & Technologycosmic radiation [muon]010308 nuclear & particles physicsFísicaLEPBeam-intensity monitorsghostcorrelationExperimental High Energy PhysicsBeam-line instrumentation (beam position and profile monitors; beam-intensity monitors; bunch length monitors); Data analysis; Performance of High Energy Physics DetectorsBeam-line instrumentation (beam position and profile monitors; beam-intensity monitors; bunch length monitors)Physics::Accelerator PhysicsPerformance of High Energy Physics DetectorsATLAS детекторBeam (structure)experimental resultsbeam-line instrumentation
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Underground investigation of extensive air showers spectra at high energy range of cosmic rays and other research in the Pyhäsalmi mine

2020

Abstract High energy particles reaching the Earth’s atmosphere are known as cosmic rays. As a result of interactions with nuclei of air molecules, cosmic rays induce showers of secondary particles, which can be divided into 3 components: electromagnetic, hadronic and muonic components. The Experiment with Multi Muon Array (EMMA), located at the depth of 75 m in the Pyhäsalmi mine in Finland, investigates the muonic component of the Extensive Air Showers (EAS) to deduce the direction, energy, and the mass of the primary cosmic ray particles. In this paper we give a concise description and methodology used by EMMA followed by a brief review of the C14 experiment. Finally, we review the feasib…

ғарыш сәулелеріPhysics::Instrumentation and DetectorsastrofysiikkaAstrophysics::High Energy Astrophysical PhenomenaBoreholekneeOcean EngineeringCosmic rayhiukkasfysiikkaSpectral lineAtmosphereNuclear physicsnuclear and elementary particle physicscosmic rayshigh-energy muonжоғары энергиялы мюонPhysicsтізе аймағыtheoretical physicsRange (particle radiation)Muonastrophysicsкең ауқымды нөсер (КАН)Neutrino detectorilmaisimetExtensive Air Shower (EAS)EMMANeutrinokosminen säteily
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