0000000000118617

AUTHOR

Wang B

showing 7 related works from this author

First Measurement of the Absolute Branching Fraction of Λ→pμ−ν¯μ

2021

The absolute branching fraction of Λ→pμ−ν¯μ is reported for the first time based on an e+e− annihilation sample of 10×109 J/ψ events collected with the BESIII detector at s=3.097 GeV. The branching fraction is determined to be B(Λ→pμ−ν¯μ)=[1.48±0.21(stat)±0.08(syst)]×10−4, which is improved by about 30% in precision over the previous indirect measurements. Combining this result with the world average of B(Λ→pe−ν¯e), we obtain the ratio {[Γ(Λ→pμ−ν¯μ)]/[Γ(Λ→pe−ν¯e)]} to be 0.178±0.028, which agrees with the standard model prediction assuming lepton flavor universality. The asymmetry of the branching fractions of Λ→pμ−ν¯μ and Λ¯→p¯μ+νμ is also determined, and no evidence for CP violation is fo…

PhysicsMeasurementAnnihilationBranching010308 nuclear & particles physicsBranching fractionmedia_common.quotation_subjectGeneral Physics and AstronomyAbsoluteTime based01 natural sciencesAsymmetryNOStandard ModelSubatomär fysikSubatomic Physics0103 physical sciencesCP violationAtomic physics010306 general physicsLeptonmedia_commonPhysical Review Letters
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Complete Measurement of the Λ Electromagnetic Form Factors.

2019

The exclusive process e+e−→ΛΛ¯, with Λ→pπ− and Λ¯→p¯π+, has been studied at s=2.396 GeV for measurement of the timelike Λ electric and magnetic form factors, GE and GM. A data sample, corresponding to an integrated luminosity of 66.9 pb−1, was collected with the BESIII detector for this purpose. A multidimensional analysis with a complete decomposition of the spin structure of the reaction enables a determination of the modulus of the ratio R=|GE/GM| and, for the first time for any baryon, the relative phase ΔΦ=ΦE−ΦM. The resulting values are R=0.96±0.14(stat)±0.02(syst) and ΔΦ=37°±12°(stat)±6°(syst), respectively. These are obtained using the recently established and most precise value of …

Multi-dimensional analysisElectron–positron annihilationRelative phaseHadronAnalytical chemistryGeneral Physics and AstronomyHadronsOBSERVABLESLambdaBaryon01 natural sciencesArticleNOHigh Energy Physics - ExperimentSubatomär fysikGermanium compoundsElectromagnetic form factorsSubatomic Physics0103 physical sciencesMagnetic form factorTwo-photon exchangePiddc:530010306 general physicsAsymmetry parameterProton Scattering; Nucleons; HydrogenPhysicsIntegrated luminosityDecompositionPhysicsHigh Energy Physics::PhenomenologyApproximation theoryPhysics multidisciplinaryPhotonHigh Energy Physics - Experiment; High Energy Physics - ExperimentBaryonLuminanceSpin structuresHigh Energy Physics::ExperimentMagnetic form factorMulti dimensional analysisBar (unit)Physical review letters
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The ARGO-YBJ Experiment Progresses and Future Extension

2010

Gamma ray source detection above 30 TeV is an encouraging approach for finding galactic cosmic ray origins. All sky survey for gamma ray sources using wide field of view detector is essential for population accumulation for various types of sources above 100 GeV. To target the goals, the ARGO-YBJ experiment has been established. Significant progresses have been made in the experiment. A large air shower detector array in an area of 1 km2 is proposed to boost the sensitivity. Hybrid detections with multi-techniques will allow a good discrimination between different types of primary particles, including photons and protons, thus enable an energy spectrum measurement for individual species. F…

PhotonGamma ray source cosmic ray origin detector arraymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPopulationDetector arrayFOS: Physical sciencesCosmic rayAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)detector arrayUltra-high-energy cosmic rayeducationMathematical Physicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_studyDetectorGamma ray sourceAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicscosmic ray originCosmic ray originAir showerSpace and Planetary ScienceSkyAstrophysics - High Energy Astrophysical Phenomena
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Background radioactivity in the scaler mode technique of the Argo-YBJ detector

2011

""ARGO-YBJ is an extensive air shower detector located at the Yangbajing Cosmic Ray Laboratory (4300 ma.s.l., 606 g cm^−2 atmospheric depth, Tibet, China).. It is made by a single layer of Resistive Plate Chambers. (RPCs, total surface ~ 6700 m^2) grouped into 153 units. called “clusters”. The low energy threshold of the experiment is obtained using the ”scaler operation mode”, counting all the particles hitting the detector without reconstruction of the shower size and arrival direction. For each cluster the signals generated by these particles are put in coincidence in a narrow time window (150 ns) and read by four independent. scaler channels, giving the counting rates of channel. >= 1, …

PhysicsResistive touchscreenPhysics and Astronomy (miscellaneous)Atmospheric pressureSettore FIS/01 - Fisica SperimentaleDetectorScaler ModeAstronomy and AstrophysicsCosmic rayRadioactivity Array Detector Scaler ModeArray DetectorCoincidenceComputational physicsRadioactivityAir showerCoincidentArgo
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Gamma ray sources observation with the ARGO-YBJ detector

2011

In this paper we report on the observations of TeV gamma ray sources performed by the air shower de- tector ARGO-YBJ. The objects studied in this work are the blazar Markarian 421 and the extended galactic source MGROJ1908+06, monitored during 2 years of operation. Mrk421 has been detected by ARGO-YBJ with a statisti- cal significance of 11 standard deviations. The observed TeV emission was highly variable, showing large enhance- ments of the flux during active periods. The study of the spectral behaviour during flares revealed a positive correla- tion of the hardness with the flux, as already reported in the past by the Whipple telescope, suggesting that this is a long term property of the…

PhysicsNuclear and High Energy PhysicsGamma AstronomyPhysics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaDetectorGamma rayFluxAstronomyExtensive Air ShowerAstronomy and AstrophysicsAstrophysicsGamma-ray astronomyArray DetectorGamma-RayArgo-YbjGamma Astronomy Array DetectorCrab NebulaAir showerPulsarMilagroBlazarInstrumentationArgoNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Distance decay 2.0 – a global synthesis of taxonomic and functional turnover in ecological communities

2021

AbstractUnderstanding the variation in community composition and species abundances, i.e., β-diversity, is at the heart of community ecology. A common approach to examine β-diversity is to evaluate directional turnover in community composition by measuring the decay in the similarity among pairs of communities along spatial or environmental distances. We provide the first global synthesis of taxonomic and functional distance decay along spatial and environmental distance by analysing 149 datasets comprising different types of organisms and environments. We modelled an exponential distance decay for each dataset using generalized linear models and extracted r2 and slope to analyse the streng…

0106 biological sciencesGeneralized linear modelDistance decayCommunity010604 marine biology & hydrobiology15. Life on land010603 evolutionary biology01 natural sciencesLatitudeExponential functionSimilarity (network science)Environmental scienceMarine ecosystem14. Life underwaterPhysical geographySpatial extent
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Evidence for the direct two-photon transition from ψ(3686) to J/ψ.

2012

The two-photon transition ψ(3686)→γγJ/ψ is studied in a sample of 1.06×10(8) ψ(3686) decays collected by the BESIII detector. The branching fraction is measured to be (3.1±0.6(stat)(-1.0)(+0.8)(syst))×10(-4) using J/ψ→e(+)e(-) and J/ψ→μ(+)μ(-) decays, and its upper limit is estimated to be 4.5×10(-4) at the 90% confidence level. This work represents the first measurement of a two-photon transition among charmonium states. The orientation of the ψ(3686) decay plane and the J/ψ polarization in this decay are also studied. In addition, the product branching fractions of sequential E1 transitions ψ(3686)→γχ(cJ) and χ(cJ)→γJ/ψ(J=0,1,2) are reported.

PhysicsParticle physicsBranching fractionElectron–positron annihilationGeneral Physics and AstronomyPhysical review letters
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