Search results for " Detectors"

showing 10 items of 2027 documents

Proposal to Detect Dark Matter using Axionic Topological Antiferromagnets

2019

Antiferromagnetically doped topological insulators (A-TI) are among the candidates to host dynamical axion fields and axion-polaritons; weakly interacting quasiparticles that are analogous to the dark axion, a long sought after candidate dark matter particle. Here we demonstrate that using the axion quasiparticle antiferromagnetic resonance in A-TI's in conjunction with low-noise methods of detecting THz photons presents a viable route to detect axion dark matter with mass 0.7 to 3.5 meV, a range currently inaccessible to other dark matter detection experiments and proposals. The benefits of this method at high frequency are the tunability of the resonance with applied magnetic field, and t…

Particle physicsPhotonPhysics - Instrumentation and DetectorsDark matterGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesResonance (particle physics)530High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Condensed Matter - Strongly Correlated ElectronsHigh Energy Physics - Phenomenology (hep-ph)Detect Dark Matter; Antiferromagnets0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Polariton010306 general physicsAxionPhysicsStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - Mesoscale and Nanoscale PhysicsInstrumentation and Detectors (physics.ins-det)Magnetic fieldHigh Energy Physics - PhenomenologyTopological insulatorQuasiparticleCondensed Matter::Strongly Correlated Electrons
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A test of electric charge conservation with Borexino

2015

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio-purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single mono-energetic photon was obtained. This new bound, tau > 6.6 10**28 yr at 90 % C.L., is two orders of magnitude better than the previous limit.

Particle physicsPhysics - Instrumentation and DetectorsOrders of magnitude (temperature)Physics::Instrumentation and DetectorsGeneral Physics and AstronomyFOS: Physical sciencesElectronScintillatorElectric chargeHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ddc:550Nuclear ExperimentBorexinoComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]Liquid scintillation countingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The beam and detector of the NA62 experiment at CERN

2017

NA62 is a fixed-target experiment at the CERN SPS dedicated to measurements of rare kaon decays. Such measurements, like the branching fraction of the $K^{+} \rightarrow \pi^{+} \nu \bar\nu$ decay, have the potential to bring significant insights into new physics processes when comparison is made with precise theoretical predictions. For this purpose, innovative techniques have been developed, in particular, in the domain of low-mass tracking devices. Detector construction spanned several years from 2009 to 2014. The collaboration started detector commissioning in 2014 and will collect data until the end of 2018. The beam line and detector components are described together with their early …

Particle physicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical scienceslarge detector systems for particle and astroparticle physicsCalorimeters; Cherenkov detectors; Large detector systems for particle and astroparticle physics; Particle tracking detectors; Instrumentation; Mathematical PhysicsNA62 experimentTracking (particle physics)7. Clean energy01 natural sciencesParticle detectorHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareNONuclear physicsmathematical physicsHigh Energy Physics - Experiment (hep-ex)Calorimeters0103 physical sciencesparticle tracking detectorsDetectors and Experimental Techniques010306 general physicsParticle Physicsphysics.ins-detCalorimeters; Cherenkov detectors; large detector systems for particle and astroparticle physics; particle tracking detectors; instrumentation; mathematical physicsPhysicsinstrumentationCalorimeterLarge Hadron Collider010308 nuclear & particles physicsBranching fractionhep-exDetectorCherenkov detectorsInstrumentation and Detectors (physics.ins-det)Particle tracking detectorBeamlineLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentBeam (structure)Particle Physics - ExperimentCherenkov detector
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Axion search with BabyIAXO in view of IAXO

2020

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to backgro…

Particle physicsPhysics - Instrumentation and Detectorssolar axion[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]experimental methodsDark matterFOS: Physical sciences7. Clean energyString (physics)Standard Modelaxion helioscopedesign [detector]International Axion Observatory (IAXO)ObservatoryPeccei-Quinn mechanismDark Matterdetector design[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesAxionsun-tracking systemsphysics.ins-detactivity reportdetector: designPhysicsinstrumentationHelioscopeLarge Hadron Colliderdetectorsolar [axion]DESYInstrumentation and Detectors (physics.ins-det)[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]IAXOmagnetopticsaxion: solar
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Improved luminosity determination in pp collisions at root s=7 TeV using the ATLAS detector at the LHC

2013

The luminosity calibration for the ATLAS detector at the LHC during pp collisions at sqrt(s) = 7 TeV in 2010 and 2011 is presented. Evaluation of the luminosity scale is performed using several luminosity-sensitive detectors, and comparisons are made of the long-term stability and accuracy of this calibration applied to the pp collisions at sqrt(s) = 7 TeV. A luminosity uncertainty of Delta L/L = +/- 3.5% is obtained for the 47 pb-1 of data delivered to ATLAS in 2010, and an uncertainty of Delta L/L = +/- 1.8% is obtained for the 5.5 fb-1 delivered in 2011.

Particle physicsPhysics and Astronomy (miscellaneous)530 PhysicsAtlas detectorPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsInteraction-Point01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)0103 physical sciencesmedicineCalibration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fysikddc:530High Energy Physics010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Engineering (miscellaneous)PhysicsLarge Hadron ColliderLuminosity (scattering theory)Sensors010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorFísicaBeamATLASmedicine.anatomical_structureExperimental High Energy PhysicsPhysical SciencesHigh Energy Physics::ExperimentLHCParticle Physics - Experiment
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Search for Dark Matter Annihilations in the Sun with the 79-String IceCube Detector

2012

We have performed a search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first time, the DeepCore sub-array is included in the analysis, lowering the energy threshold and extending the search to the austral summer. The 317 days of data collected between June 2010 and May 2011 are consistent with the expected background from atmospheric muons and neutrinos. Upper limits are therefore set on the dark matter annihilation rate, with conversions to limits on spin-dependent and spin-independent WIMP-proton cross-sections for WIMP masses in the range 20 - 5000 GeV. These are the most stringent s…

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesGeneral Physics and AstronomyCosmic rayddc:500.2MASSIVE PARTICLESAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)LIMITSWIMP0103 physical sciencesddc:550010306 general physicsLight dark matterCANDIDATESHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsCONSTRAINTSCAPTURENEUTRINOSPhysics and AstronomyNeutrino detector13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentCryogenic Dark Matter SearchNeutrinoAstrophysics - High Energy Astrophysical PhenomenaPhysical Review Letters
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Measurement of the Inclusive Electron Neutrino Charged Current Cross Section on Carbon with the T2K Near Detector

2014

The T2K off-axis near detector, ND280, is used to make the first differential cross-section measurements of electron neutrino charged current interactions at energies ~1 GeV as a function of electron momentum, electron scattering angle and four-momentum transfer of the interaction. The total flux-averaged $\nu_e$ charged current cross-section on carbon is measured to be $1.11\pm0.09~(stat)\pm0.18~(syst)\times10^{-38} cm^2/nucleon$. The differential and total cross-section measurements agree with the predictions of two leading neutrino interaction generators, NEUT and GENIE. The NEUT prediction is $1.23\times10^{-38} cm^2/nucleon$ and the GENIE prediction is $1.08\times10^{-38} cm^2/nucleon$…

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesParticle detectorsElectronCarbon Electron scattering Electrons Neutrons Testbed7. Clean energyHigh Energy Physics - ExperimentNuclear physicsCross section (physics)Physics and Astronomy (all)High Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentCharged currentPhysicsCharged current Differential cross section Electron momentum Electron neutrino Neutrino interactions Off-axis Total cross section Total fluxFísicaGargamelleHigh Energy Physics::ExperimentNeutrinoNucleonElectron neutrinoElectron scatteringPhysical Review Letters
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Evidence for Muon Neutrino Oscillation in an Accelerator-Based Experiment

2005

We present results for muon neutrino oscillation in the KEK to Kamioka (K2K) long-baseline neutrino oscillation experiment. K2K uses an accelerator-produced muon neutrino beam with a mean energy of 1.3 GeV directed at the Super-Kamiokande detector. We observed the energy dependent disappearance of muon neutrino, which we presume have oscillated to tau neutrino. The probability that we would observe these results if there is no neutrino oscillation is 0.0050% (4.0 sigma).

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesMuon neutrino010306 general physicsNeutrino oscillationPhysicsTamura Norio010308 nuclear & particles physicsOscillationDetectorHigh Energy Physics::PhenomenologySigmaFísicaSolar neutrino problemK2K experimentPhysics::Accelerator Physics田村 詔生High Energy Physics::ExperimentBeam (structure)
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Testing charged current quasi-elastic and multinucleon interaction models in the NEUT neutrino interaction generator with published datasets from the…

2016

There has been a great deal of theoretical work on sophisticated charged current quasi-elastic (CCQE) neutrino interaction models in recent years, prompted by a number of experimental results that measured unexpectedly large CCQE cross sections on nuclear targets. As the dominant interaction mode at T2K energies, and the signal process in oscillation analyses, it is important for the T2K experiment to include realistic CCQE cross section uncertainties in T2K analyses. To this end, T2K’s Neutrino Interaction Working Group has implemented a number of recent models in NEUT, T2K’s primary neutrino interaction event generator. In this paper, we give an overview of the models implemented and pres…

Particle physicsPhysics::Instrumentation and DetectorsC-12Astronomy & AstrophysicsMASS7. Clean energy01 natural sciencesPhysics Particles & FieldsMiniBooNENuclear physics0103 physical sciencesMINERνAMuon neutrino010306 general physicsNeutrino oscillationEvent generatorPhysicsScience & TechnologyMuonDELTA010308 nuclear & particles physicsPhysicsT2K experimentNUCLEUS SCATTERINGPhysical SciencesSIMULATIONHigh Energy Physics::ExperimentNeutrino
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LeptonInjector and LeptonWeighter: A neutrino event generator and weighter for neutrino observatories

2021

We present a high-energy neutrino event generator, called LeptonInjector, alongside an event weighter, called LeptonWeighter. Both are designed for large-volume Cherenkov neutrino telescopes such as IceCube. The neutrino event generator allows for quick and flexible simulation of neutrino events within and around the detector volume, and implements the leading Standard Model neutrino interaction processes relevant for neutrino observatories: neutrino-nucleon deep-inelastic scattering and neutrino-electron annihilation. In this paper, we discuss the event generation algorithm, the weighting algorithm, and the main functions of the publicly available code, with examples.

Particle physicsPhysics::Instrumentation and DetectorsComputer scienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyCHERENKOV LIGHT YIELDWeighting01 natural sciencesHigh Energy Physics - Experiment010305 fluids & plasmasStandard ModelHigh Energy Physics - Experiment (hep-ex)Neutrino interactionHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsCherenkov radiationEvent generatorEvent generator; Neutrino generator; Neutrino interaction; Neutrino simulation; WeightingGenerator (computer programming)hep-exEvent (computing)ICEHigh Energy Physics::PhenomenologyDetectorhep-phComputational Physics (physics.comp-ph)Quantitative Biology::GenomicsHigh Energy Physics - Phenomenologyphysics.comp-phHardware and ArchitectureHigh Energy Physics::ExperimentNeutrino simulationNeutrino generatorEvent generatorNeutrinoPhysics - Computational PhysicsLeptonComputer Physics Communications
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