Search results for "QC770"

showing 10 items of 270 documents

The liquid-argon scintillation pulseshape in DEAP-3600

2020

AbstractDEAP-3600 is a liquid-argon scintillation detector looking for dark matter. Scintillation events in the liquid argon (LAr) are registered by 255 photomultiplier tubes (PMTs), and pulseshape discrimination (PSD) is used to suppress electromagnetic background events. The excellent PSD performance of LAr makes it a viable target for dark matter searches, and the LAr scintillation pulseshape discussed here is the basis of PSD. The observed pulseshape is a combination of LAr scintillation physics with detector effects. We present a model for the pulseshape of electromagnetic background events in the energy region of interest for dark matter searches. The model is composed of (a) LAr scin…

PhotomultiplierPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterFOS: Physical scienceslcsh:AstrophysicsScintillatorWavelength shifter01 natural sciencesParticle detectorDEAPOptics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)PhysicsScintillation010308 nuclear & particles physicsbusiness.industryInstrumentation and Detectors (physics.ins-det)Scintillation counterlcsh:QC770-798businessEuropean Physical Journal C: Particles and Fields
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First operation of the KATRIN experiment with tritium

2020

AbstractThe determination of the neutrino mass is one of the major challenges in astroparticle physics today. Direct neutrino mass experiments, based solely on the kinematics of $$\upbeta $$β-decay, provide a largely model-independent probe to the neutrino mass scale. The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to directly measure the effective electron antineutrino mass with a sensitivity of $$0.2\hbox { eV}$$0.2eV ($$90\%$$90% CL). In this work we report on the first operation of KATRIN with tritium which took place in 2018. During this commissioning phase of the tritium circulation system, excellent agreement of the theoretical prediction with the recorded spectra was …

Physics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsFOS: Physical scienceslcsh:Astrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]TritiumKATRIN01 natural sciencesantineutrino/e: massHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)lcsh:QB460-4660103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]lcsh:Nuclear and particle physics. Atomic energy. RadioactivityMass scaleddc:530Electron Capture[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsEngineering (miscellaneous)Nuclear ExperimentAstroparticle physicsPhysics010308 nuclear & particles physicstritiumPhysicsQuímicaInstrumentation and Detectors (physics.ins-det)sensitivityddc:lcsh:QC770-798TritiumHigh Energy Physics::ExperimentNeutrinoPräzisionsexperimente - Abteilung BlaumNeutrino Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Electron neutrinoperformanceKATRINAstrophysics - Cosmology and Nongalactic Astrophysicsexperimental results
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Material radioassay and selection for the XENON1T dark matter experiment

2017

The XENON1T dark matter experiment aims to detect weakly interacting massive particles (WIMPs) through low-energy interactions with xenon atoms. To detect such a rare event necessitates the use of radiopure materials to minimize the number of background events within the expected WIMP signal region. In this paper we report the results of an extensive material radioassay campaign for the XENON1T experiment. Using gamma-ray spectroscopy and mass spectrometry techniques, systematic measurements of trace radioactive impurities in over one hundred samples within a wide range of materials were performed. The measured activities allowed for stringent selection and placement of materials during the…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsDark matterMonte Carlo methodmeasurement methodsFOS: Physical scienceschemistry.chemical_elementRadiopuritylcsh:AstrophysicsWIMP: detectorSciences de l'ingénieur01 natural sciencesgamma ray: energy spectrumNuclear physicsmass spectrumXENONXenonWIMPlcsh:QB460-4660103 physical sciencesDark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSpectroscopy[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Engineering (miscellaneous)background: radioactivityPhysicsRange (particle radiation)Physique010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)AstronomiesensitivitychemistryWeakly interacting massive particleslcsh:QC770-798TPCnumerical calculations: Monte Carlo
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Cosmic-ray muon flux at Canfranc Underground Laboratory

2019

Residual flux and angular distribution of high-energy cosmic muons have been measured in two underground locations at the Canfranc Underground Laboratory (LSC) using a dedicated Muon Monitor. The instrument consists of three layers of fast scintillation detector modules operating as 352 independent pixels. The monitor has flux-defining area of 1 m${}^{2}$, covers all azimuth angles, and zenith angles up to $80^\circ$. The measured integrated muon flux is $(5.26 \pm 0.21) \times 10^{-3}$ m${}^{-2}$s${}^{-1}$ in the Hall A of the LAB2400 and $(4.29 \pm 0.17) \times 10^{-3}$ m${}^{-2}$s${}^{-1}$ in LAB2500. The angular dependence is consistent with the known profile and rock density of the sur…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsFOS: Physical sciencesFluxlcsh:AstrophysicsCosmic rayApplied Physics (physics.app-ph)hiukkasfysiikkaScintillator01 natural sciencesNuclear physicslcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010303 astronomy & astrophysicsEngineering (miscellaneous)ZenithPhysicsMuon010308 nuclear & particles physicsCanfranc Underground LaboratoryPhysics - Applied PhysicsInstrumentation and Detectors (physics.ins-det)Azimuthilmaisimethigh-energy cosmic muonsMuon fluxlcsh:QC770-798High Energy Physics::Experimentkosminen säteily
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Theia: an advanced optical neutrino detector

2020

The European physical journal. C, Particles and fields 80(5), 416 (2020). doi:10.1140/epjc/s10052-020-7977-8

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)neutrino detectors liquid scintillators cherenkovPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaexperimental physicstutkimuslaitteetFOS: Physical scienceslcsh:Astrophysicshiukkasfysiikkanucl-ex01 natural sciencesAtomic530High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle and Plasma PhysicsDouble beta decay0103 physical scienceslcsh:QB460-466Deep Underground Neutrino Experimentlcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclearddc:530Nuclear Experiment (nucl-ex)010306 general physicsEngineering (miscellaneous)physics.ins-detNuclear ExperimentCherenkov radiationPhysicsScintillationQuantum Physics010308 nuclear & particles physicshep-exDetectorneutriinotMolecularInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsNeutrino detectorilmaisimetlcsh:QC770-798High Energy Physics::ExperimentNeutrino
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Minimal coupling in presence of non-metricity and torsion

2020

We deal with the question of what it means to define a minimal coupling prescription in presence of torsion and/or non-metricity, carefully explaining while the naive substitution $\partial\to\na$ introduces extra couplings between the matter fields and the connection that can be regarded as non-minimal in presence of torsion and/or non-metricity. We will also investigate whether minimal coupling prescriptions at the level of the action (MCPL) or at the level of field equations (MCPF) lead to different dynamics. To that end, we will first write the Euler-Lagrange equations for matter fields in terms of the covariant derivatives of a general non-Riemannian space, and derivate the form of the…

Physics and Astronomy (miscellaneous)FOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Space (mathematics)Computer Science::Digital Libraries01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakelcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityCovariant transformation010306 general physicsEngineering (miscellaneous)Mathematical PhysicsSpin-½Mathematical physicsMinimal couplingPhysics010308 nuclear & particles physicsCharge (physics)Mathematical Physics (math-ph)Action (physics)Connection (mathematics)Computer Science::Mathematical Softwaresymbolslcsh:QC770-798Noether's theorem
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Averages of $b$-hadron, $c$-hadron, and $\tau$-lepton properties as of summer 2016

2017

This article reports world averages of measurements of $b$-hadron, $c$-hadron, and $\tau$-lepton properties obtained by the Heavy Flavor Averaging Group using results available through summer 2016. For the averaging, common input parameters used in the various analyses are adjusted (rescaled) to common values, and known correlations are taken into account. The averages include branching fractions, lifetimes, neutral meson mixing parameters, \CP~violation parameters, parameters of semileptonic decays and CKM matrix elements.

Physics and Astronomy (miscellaneous)HadronKOBAYASHI-MASKAWA MATRIX01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - Experiment[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCPhysicsCabibbo–Kobayashi–Maskawa matrixPhysicsSettore FIS/01 - Fisica SperimentaleBEAUTYhep-phNuclear & Particles PhysicsHigh Energy Physics - PhenomenologyPhysical SciencesCP violationParticle Physics - ExperimentEXCITED CHARM MESONSTRIPLE-PRODUCT CORRELATIONSParticle physicsMesonHEAVY FLAVOURSlcsh:AstrophysicsCHARM0202 Atomic Molecular Nuclear Particle And Plasma PhysicsQUARK FRAGMENTATION FRACTIONS0103 physical scienceslcsh:QB460-466RELATIVE BRANCHING FRACTIONSB-D(0)-(B)OVER-BAR(D)(0) OSCILLATION FREQUENCYlcsh:Nuclear and particle physics. Atomic energy. RadioactivityEXCLUSIVE SEMILEPTONIC HEAVY010306 general physicsQED RADIATIVE-CORRECTIONS0206 Quantum PhysicsEngineering (miscellaneous)DECAY-WIDTH DIFFERENCETAU LEPTONSParticle Physics - PhenomenologyScience & Technologyhep-ex010308 nuclear & particles physicsHigh Energy Physics::Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]FORM-FACTOR RATIOSlcsh:QC770-798High Energy Physics::ExperimentLepton
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Dispersion relation formalism for the two-photon exchange correction to elastic muon-proton scattering: elastic intermediate state

2018

We evaluate the two-photon exchange correction to the unpolarized cross section in the elastic muon-proton scattering within dispersion relations. One of the six independent invariant amplitudes requires a subtraction. We fix the subtraction function to the model estimate of the full two-photon exchange at one of three MUSE beam energies and make a prediction for the two other energies. Additionally, we present single and double polarization observables accounting for the lepton mass.

Physics and Astronomy (miscellaneous)Nuclear TheoryFOS: Physical scienceslcsh:Astrophysics01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Two-photon excitation microscopyDispersion relation0103 physical scienceslcsh:QB460-466Intermediate statelcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment (nucl-ex)010306 general physicsEngineering (miscellaneous)Nuclear ExperimentPhysicsMuon010308 nuclear & particles physicsScatteringSubtractionHigh Energy Physics - PhenomenologyAmplitudeQuantum electrodynamicslcsh:QC770-798Lepton
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$\texttt{HEPfit}$: a Code for the Combination of Indirect and Direct Constraints on High Energy Physics Models

2020

The European physical journal / C Particles and fields C80(5), 456 (2020). doi:10.1140/epjc/s10052-020-7904-z

Physics and Astronomy (miscellaneous)Physics beyond the Standard ModelMonte Carlo methoddoublet: 2 [Higgs particle]Parameter space01 natural sciencesMonte Carlo: Markov chainHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)effective field theoryHigh Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Statistical physicsStandard model (cryptography)Physicsnew physicsHiggs particle: doublet: 2statistical analysis: BayesianObservablehep-phHigh Energy Physics - PhenomenologysymbolsParticle Physics - Experimentcorrection: obliqueBayesian probabilityFOS: Physical scienceslcsh:AstrophysicsMarkov chain [Monte Carlo]Bayesian [statistical analysis]530programmingSet (abstract data type)oblique [correction]symbols.namesake0103 physical scienceslcsh:QB460-466operator: dimension: 6ddc:530lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsnumerical calculationsEngineering (miscellaneous)Particle Physics - Phenomenology010308 nuclear & particles physicshep-exMarkov chain Monte Carlomanual[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798dimension: 6 [operator]
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Cutoff dependence of the thrust peak position in the dipole shower

2020

We analyse the dependence of the peak position of the thrust distribution on the cutoff value in the Nagy-Soper dipole shower. We compare the outcome of the parton shower simulations to a relation of the dependence from an analytic computation, derived within soft-collinear effective theory. We show that the result of the parton shower simulations and the analytic computation are in good agreement.

Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsComputationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical scienceslcsh:AstrophysicsThrust01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Position (vector)lcsh:QB460-4660103 physical sciencesEffective field theoryCutofflcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsParton showerEngineering (miscellaneous)Physics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsComputational physicsDipoleHigh Energy Physics - PhenomenologyDistribution (mathematics)lcsh:QC770-798High Energy Physics::Experiment
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