Search results for "Astroparticle physics"

showing 10 items of 101 documents

Probing neutrino non-standard interactions with atmospheric neutrino data

2001

We have reconsidered the atmospheric neutrino anomaly in light of the laetst data from Super-Kamiokande contained events and from Super-Kamiokande and MACRO up-going muons. We have reanalysed the proposed solution to the atmospheric neutrino anomaly in terms of non-standard neutrino-matter interactions (NSI) as well as the standard nu_mu -> nu_tau oscillations (OSC). Our statistical analysis shows that a pure NSI mechanism is now ruled out at 99%, while the standard nu_mu -> nu_tau OSC mechanism provides a quite remarkably good description of the anomaly. We therefore study an extended mechanism of neutrino propagation which combines both oscillation and non-standard neutrino-matter i…

PhysicsNuclear and High Energy PhysicsParticle physicsMuonVacuum stateHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)FísicaOrder (ring theory)FOS: Physical sciencesAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)Astroparticle PhysicsHigh Energy Physics - Phenomenology (hep-ph)Statistical analysisHigh Energy Physics::ExperimentAnomaly (physics)NeutrinoAtmospheric neutrinoNeutrino oscillation
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

2020

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers.

Physics::Instrumentation and DetectorsAstronomyprimary [cosmic radiation]01 natural sciences030218 nuclear medicine & medical imagingAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinesurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Data Processing; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of High Energy Physics DetectorsInstrumentationMathematical PhysicsData Processing; Large detector systems for particle and astroparticle physics; Largedetector-systems performance; Performance of High Energy Physics DetectorsLarge detector-systems performanceHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEInstrumentation et méthodes en physiqueData ProcessingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugercascadeobservatoryCascadeLargedetector-systems performanceddc:620Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airAstrophysics::High Energy Astrophysical PhenomenawaterFOS: Physical sciencesCosmic rayAtmosphere03 medical and health sciencesOptics0103 physical sciencesHigh Energy Physics14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithEngineering & allied operationsPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryhep-exdetector: surfaceLarge detector systems for particle and astroparticle physicsAutres mathématiquescosmic radiation: primaryCherenkov counterExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentPerformance of High Energy Physics Detectorsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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Combined performance studies for electrons at the 2004 ATLAS combined test-beam

2010

In 2004 at the ATLAS (A Toroidal LHC ApparatuS) combined test beam, one slice of the ATLAS barrel detector (including an Inner Detector set-up and the Liquid Argon calorimeter) was exposed to particles from the H8 SPS beam line at CERN. It was the first occasion to test the combined electron performance of ATLAS. This paper presents results obtained for the momentum measurement p with the Inner Detector and for the performance of the electron measurement with the LAr calorimeter (energy E linearity and resolution) in the presence of a magnetic field in the Inner Detector for momenta ranging from 20 GeV/c to 100 GeV/c. Furthermore the particle identification capabilities of the Transition Ra…

Physics::Instrumentation and DetectorsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]Transition radiation detectorsElectronsddc:500.201 natural sciencesParticle identificationNuclear physicsCalorimetersAtlas (anatomy)Particle tracking detectors0103 physical sciencesmedicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationDetectors de radiacióMathematical PhysicsPhysicsLarge Hadron ColliderScience & Technology010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsDetectorCalorimetermedicine.anatomical_structureTransition radiationBeamlineHigh Energy Physics::ExperimentBeam (structure)
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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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Search for point-like sources of ultra-high energy neutrinos at the pierre auger observatory and improved limit on the diffuse flux of tau neutrinos

2012

The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy Eν between 1017 eV and 1020 eV from point-like sources across the sky south of +55º and north of −65º declinations. A search has been performed for highly inclined extensive air showers produced by the interaction of neutrinos of all flavors in the atmosphere (downward-going neutrinos), and by the decay of tau leptons originating from tau neutrino interactions in Earth’s crust (Earth-skimming neutrinos). No candidate neutrinos have been found in data up to 2010 May 31. This corresponds to an equivalent exposure of ∼3.5 years of a full surface detector array for the Earth-skimming channel and ∼2 years…

Physics::Instrumentation and DetectorsSolar neutrinoAstronomyAstrophysics01 natural sciences7. Clean energyneutrinoTelescopiosTau neutrinoastroparticle physics; cosmic rays; neutrinos; telescopes010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)cosmic rayPhysics[PHYS]Physics [physics]High Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]neutrinosCOSMIC-RAYSCosmic neutrino backgroundastroparticle physicsMeasurements of neutrino speedFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstrophysics::High Energy Astrophysical PhenomenaTELESCÓPIOSFOS: Physical sciencesAstroparticle physiccosmic rays0103 physical sciencesDETECTORCiencias ExactasPierre Auger Observatory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and AstrophysicstelescopesSolar neutrino problem13. Climate actionSpace and Planetary ScienceExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
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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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First results on ProtoDUNE-SP liquid argon time projection chamber performance from a beam test at the CERN Neutrino Platform

2020

The ProtoDUNE-SP detector is a single-phase liquid argon time projection chamber with an active volume of 7.2× 6.1× 7.0 m3. It is installed at the CERN Neutrino Platform in a specially-constructed beam that delivers charged pions, kaons, protons, muons and electrons with momenta in the range 0.3 GeV/c to 7 GeV/c. Beam line instrumentation provides accurate momentum measurements and particle identification. The ProtoDUNE-SP detector is a prototype for the first far detector module of the Deep Underground Neutrino Experiment, and it incorporates full-size components as designed for that module. This paper describes the beam line, the time projection chamber, the photon detectors, the cosmic-r…

Physics::Instrumentation and Detectorsilmaisimettutkimuslaitteetneutriinotlarge detector systems for particle and astroparticle physicsHigh Energy Physics::Experimenttime projection chambers (TPC)noble liquid detectors (scintillation ionization double-phase)hiukkasfysiikka
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Performance study of a 3×1×1 m3 dual phase liquid Argon Time Projection Chamber exposed to cosmic rays

2021

We report the results of the analyses of the cosmic ray data collected with a 4 tonne (3×1×1 m3) active mass (volume) Liquid Argon Time-Projection Chamber (TPC) operated in a dual-phase mode. We present a detailed study of the TPC's response, its main detector parameters and performance. The results are important for the understanding and further developments of the dual-phase technology, thanks to the verification of key aspects, such as the extraction of electrons from liquid to gas and their amplification through the entire one square metre readout plain, gain stability, purity and charge sharing between readout views. peerReviewed

Physics::Instrumentation and Detectorsilmaisimettutkimuslaitteetparticle tracking detectorstime projection chambersneutriinotlarge detector systems for particle and astroparticle physicshiukkasfysiikkakosminen säteilyneutrino detectors
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Measurement of visible cross sections in proton-lead collisions at √sNN= 5.02 TeV in van der Meer scans with the ALICE detector

2014

In 2013, the Large Hadron Collider provided proton-lead and lead-proton collisions at the center-of-mass energy per nucleon pair $\sqrt{s_{\rm{NN}}}=5.02$ TeV. Van der Meer scans were performed for both configurations of colliding beams, and the cross section was measured for two reference processes, based on particle detection by the T0 and V0 detectors, with pseudo-rapidity coverage $4.6<\eta< 4.9$, $-3.3<\eta<-3.0$ and $2.8<\eta< 5.1$, $-3.7<\eta<-1.7$, respectively. Given the asymmetric detector acceptance, the cross section was measured separately for the two configurations. The measured visible cross sections are used to calculate the integrated luminosity of the proton-lead and lead-…

ProtonNuclear Theorylarge detector systems for particle and astroparticle physicsLarge detector systems for particle and astroparticle physics; Particle tracking detec- tors; Heavy-ion detectors01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Particle tracking detectorsparticle tracking detectors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron detectionNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentInstrumentationMathematical PhysicsPhysicsLarge Hadron ColliderLuminosity (scattering theory)PhysicsDetectorLuminosity measurement3. Good healthPRIRODNE ZNANOSTI. Fizika.Large detector systems for particle and astroparticle physics Particle tracking detec- torNucleonParticle Physics - ExperimentLarge detector systems for particle and astroparticle physics ; Particle tracking detectors ; Heavy-ion detectorsParticle physicsParticle tracking detec- torsInstrumentationHeavy-ion detectorsFOS: Physical sciencesLarge detector systems for particle and astroparticle physics; Particle tracking detectors; Heavy-ion detectors[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear physicsCross section (physics)p-Pb collisions at the LHC0103 physical sciencesNuclear Physics - Experiment010306 general physics010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsALICE experimentLarge detector systems for particle and astroparticle physics Particle tracking detec- tors; Heavy-ion detectorsNATURAL SCIENCES. Physics.heavy-ion detectorsInstrumentation; Mathematical PhysicsPhysics::Accelerator PhysicsHigh Energy Physics::Experiment
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The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)

2015

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 13th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2013; Asilomar Conference Grounds Monterey Peninsula; United States; 8 September 2013 through 13 September 2013. The International Axion Observatory (IAXO) is a proposed 4th-generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 - 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling gaγ down to a few ×10-12 GeV-1 for a wide range of axion masses up to ∼ 0.25 eV. This is an improvement over the currently best …

QCD axionParticle physicsPhysics::Instrumentation and DetectorsDark matterPhysics and Astronomy(all)01 natural sciences7. Clean energymagnetic helioscopeHigh Energy Physics::TheoryQCD axionsAstroparticle PhysicsAxionObservatory0103 physical sciencesDark matterQCD axions; magnetic helioscope; dark matterDark Matterddc:530Detectors and Experimental Techniques010306 general physicsAxionAstroparticle physicsPhysicsHelioscope010308 nuclear & particles physicsAxion Dark Matter ExperimentHigh Energy Physics::PhenomenologyStrong CP problemIAXOStrong CP ProblemALPStrong CP problemAstroparticle physicsCERN Axion Solar TelescopeParticle Physics - ExperimentHelioscopesPhysics Procedia
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