0000000000173980

AUTHOR

Zhao-min Wang

showing 6 related works from this author

In-flight performance of the DAMPE silicon tracker

2018

Abstract DAMPE (DArk Matter Particle Explorer) is a spaceborne high-energy cosmic ray and gamma-ray detector , successfully launched in December 2015. It is designed to probe astroparticle physics in the broad energy range from few GeV to 100 TeV. The scientific goals of DAMPE include the identification of possible signatures of Dark Matter annihilation or decay, the study of the origin and propagation mechanisms of cosmic-ray particles, and gamma-ray astronomy . DAMPE consists of four sub-detectors: a plastic scintillator strip detector, a Silicon–Tungsten tracKer–converter (STK), a BGO calorimeter and a neutron detector . The STK is composed of six double layers of single-sided silicon mi…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGamma rayDark matterFOS: Physical sciencesCosmic rayScintillator01 natural sciences7. Clean energyOptics0103 physical sciencesDark matterNeutron detection010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysInstrumentationNuclear and High Energy PhysicAstroparticle physicsPhysicsCalorimeter (particle physics)010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleDetectorGamma raysGamma rayInstrumentation and Detectors (physics.ins-det)Cosmic raySpaceborne experimentSilicon trackerHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for AstrophysicsbusinessCosmic rays; Dark matter; Gamma rays; Silicon tracker; Spaceborne experiment; Nuclear and High Energy Physics; Instrumentation
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The on-orbit calibration of DArk Matter Particle Explorer

2019

Abstract The DArk Matter Particle Explorer (DAMPE), a satellite-based cosmic ray and gamma-ray detector, was launched on December 17, 2015, and began its on-orbit operation on December 24, 2015. In this work we document the on-orbit calibration procedures used by DAMPE and report the calibration results of the Plastic Scintillator strip Detector (PSD), the Silicon-Tungsten tracKer-converter (STK), the BGO imaging calorimeter (BGO), and the Neutron Detector (NUD). The results are obtained using Galactic cosmic rays, bright known GeV gamma-ray sources, and charge injection into the front-end electronics of each sub-detector. The determination of the boundary of the South Atlantic Anomaly (SAA…

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayScintillator01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesNeutron detectionDark MatterInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCalorimeter (particle physics)010308 nuclear & particles physicsDetectorSettore FIS/01 - Fisica SperimentaleGamma rayAstronomyAstronomy and AstrophysicsCosmic RaysSouth Atlantic AnomalyHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Internal alignment and position resolution of the silicon tracker of DAMPE determined with orbit data

2017

Abstract The DArk Matter Particle Explorer (DAMPE) is a space-borne particle detector designed to probe electrons and gamma-rays in the few GeV to 10 TeV energy range, as well as cosmic-ray proton and nuclei components between 10 GeV and 100 TeV. The silicon–tungsten tracker–converter is a crucial component of DAMPE. It allows the direction of incoming photons converting into electron–positron pairs to be estimated, and the trajectory and charge (Z) of cosmic-ray particles to be identified. It consists of 768 silicon micro-strip sensors assembled in 6 double layers with a total active area of 6.6 m 2 . Silicon planes are interleaved with three layers of tungsten plates, resulting in about o…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhotonSiliconProtonPhysics::Instrumentation and DetectorsAlignment; Cosmic-ray detectors; Gamma-ray telescopes; Silicon-strip detectors; Nuclear and High Energy Physics; InstrumentationGamma-ray telescopesAstrophysics::High Energy Astrophysical PhenomenaCosmic-ray detectorsFOS: Physical scienceschemistry.chemical_elementElectron01 natural sciencesSilicon-strip detectorRadiation lengthParticle detectorOptics0103 physical sciences010303 astronomy & astrophysicsInstrumentationImage resolutionNuclear and High Energy PhysicAlignmentPhysicsRange (particle radiation)010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleInstrumentation and Detectors (physics.ins-det)Cosmic-ray detectorSilicon-strip detectorschemistryGamma-ray telescopeHigh Energy Physics::ExperimentbusinessNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

2019

DAMPE satellite has directly measured the cosmic ray proton spectrum from 40 GeV to 100 TeV and revealed a new feature at about 13.6 TeV.

dark matter cosmic rays spaceProtonMilky WayAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsKinetic energy01 natural sciences0103 physical sciences010306 general physicsNuclear ExperimentResearch ArticlesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral indexMultidisciplinary010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologySettore FIS/01 - Fisica SperimentaleSciAdv r-articlesPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaResearch Article
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Measurement of the Cosmic Ray Helium Energy Spectrum from 70 GeV to 80 TeV with the DAMPE Space Mission

2021

The measurement of the energy spectrum of cosmic ray helium nuclei from 70 GeV to 80 TeV using 4.5 years of data recorded by the DArk Matter Particle Explorer (DAMPE) is reported in this work. A hardening of the spectrum is observed at an energy of about 1.3 TeV, similar to previous observations. In addition, a spectral softening at about 34 TeV is revealed for the first time with large statistics and well controlled systematic uncertainties, with an overall significance of $4.3\sigma$. The DAMPE spectral measurements of both cosmic protons and helium nuclei suggest a particle charge dependent softening energy, although with current uncertainties a dependence on the number of nucleons canno…

Astrophysics::High Energy Astrophysical PhenomenaDark matterGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesCosmic raySpace (mathematics)01 natural sciences7. Clean energyCosmic ray heliumHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesEnergy spectrumcosmic rays dark matter spacecrystals010306 general physicsHeliumPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)COSMIC cancer databasedetectorSettore FIS/01 - Fisica SperimentalecalibrationchemistryParticleAstrophysics - High Energy Astrophysical PhenomenaNucleonperformance
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The DArk Matter Particle Explorer mission

2017

The DArk Matter Particle Explorer (DAMPE), one of the four scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Sciences, is a general purpose high energy cosmic-ray and gamma-ray observatory, which was successfully launched on December 17th, 2015 from the Jiuquan Satellite Launch Center. The DAMPE scientific objectives include the study of galactic cosmic rays up to $\sim 10$ TeV and hundreds of TeV for electrons/gammas and nuclei respectively, and the search for dark matter signatures in their spectra. In this paper we illustrate the layout of the DAMPE instrument, and discuss the results of beam tests and calib…

Physics - Instrumentation and DetectorsSatellite launchesGamma ray observatoriesAstrophysicsGalactic cosmic rays01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ObservatoryDetectors and Experimental TechniquesCosmic rays dark matter space experiments010303 astronomy & astrophysicsphysics.ins-detSpace science missionsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)CosmologyCosmology Galaxies Gamma rays Tellurium compounds Chinese Academy of Sciences Dark matter particles Explorer missions Galactic cosmic rays Gamma ray observatories Satellite launches Scientific objectives Space science missions Cosmic raysSpace ScienceAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaParticle Physics - ExperimentAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic raydark matterTellurium compounds0103 physical sciencesCosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)010308 nuclear & particles physicshep-exGamma raysAstronomyAstronomy and AstrophysicsGalaxiesChinese academy of sciencesGalaxyScientific objectivesDark matter particlesChinese Academy of SciencesSatellitespace experimentsExplorer missionsastro-ph.IM
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