Search results for "high [electromagnetic field]"

showing 10 items of 20620 documents

IMI Prevention of Myopia and Its Progression

2021

The prevalence of myopia has markedly increased in East and Southeast Asia, and pathologic consequences of myopia, including myopic maculopathy and high myopia-associated optic neuropathy, are now some of the most common causes of irreversible blindness. Hence, strategies are warranted to reduce the prevalence of myopia and the progression to high myopia because this is the main modifiable risk factor for pathologic myopia. On the basis of published population-based and interventional studies, an important strategy to reduce the development of myopia is encouraging schoolchildren to spend more time outdoors. As compared with other measures, spending more time outdoors is the safest strategy…

ulkoilugenetic structuresContact Lensesmedicine.medical_treatmenttaittovirheetehkäisyatropinePopulationVisual impairmentlikinäköisyysorthokeratologyGlobal HealthRefraction Ocularmyopia-associated optic neuropathyOptic neuropathy03 medical and health sciences0302 clinical medicineMyopiaPrevalencemedicineHumansRisk factorhigh myopiaeducationeducation.field_of_studySpecial Issuebusiness.industrypathologic myopiamyopic macular degenerationOrthokeratologyAccommodation Ocularpiilolasitmedicine.diseaseeye diseasesAmplitude of accommodationEyeglassesDisease Progression030221 ophthalmology & optometryOptometryMaculopathysense organsmedicine.symptombusinessAccommodation030217 neurology & neurosurgeryInvestigative Opthalmology & Visual Science
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Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

2017

A search for ultra-high energy photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation mode. An unprecedented separation power between photon and hadron primaries is achieved by combining measurements of the longitudinal air-shower development with the particle content at ground measured by the fluorescence and surface detectors, respectively. Only three photon candidates at energies 1-2 EeV are found, which is compatible with the expected hadron-induced background. Upper limits on the integral flux of ultra-high energy photons of 0.027, 0.009, 0.008, 0.008 and 0.007 km-2 sr-1 yr-1 are derived at 95% C.L. for ener…

ultra high energy cosmic rays cosmic ray experimentsPhoton[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyHadronFluxultra high energy cosmic rays; cosmic ray experiments7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)energy: thresholdCosmic ray experiments[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsphoton: productionconstraint: energyCOSMIC-RAYSAugerobservatoryContent (measure theory)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenalongitudinalAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayultra high energy cosmic raysdark matterUltra high energy cosmic rays Cosmic ray experiments Astronomy and Astrophysics.Nuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesultra high energy cosmic rays; cosmic ray experiments; Astronomy and Astrophysicscosmic radiation: UHEHigh Energy PhysicsCiencias ExactasPierre Auger ObservatorySPECTRUMhybridbackgrounddetector: surface010308 nuclear & particles physicsFísicaUltra high energy cosmic raysAstronomy and AstrophysicsASTROFÍSICAULTRA-HIGH ENERGYfluxExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experimentshadron[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Ultra-High Energy Neutrinos at the Pierre Auger Observatory

2013

The observation of ultrahigh energy neutrinos (UHE nu s) has become a priority in experimental astroparticle physics. UHE nu s can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going nu) or in the Earth crust (Earth-skimming nu), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and …

ultra high energy neutrino[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsCiencias FísicasAstronomyFluxAstrophysics7. Clean energy01 natural sciencesAltas energíasAuger//purl.org/becyt/ford/1 [https]surface [detector]ObservatoryneutriniCosmic-rayscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCascada atmosférica extensaOBSERVATÓRIOS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsneutrino; Augerlcsh:QC1-999AugercascadeUHE [neutrino]observatoryPhysics::Space PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearultra high energy neutrinosNeutrinoAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASsignatureTAU-NEUTRINOSatmosphere [showers]FLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Article SubjectairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayFísica de Partículas y CamposLIMITPartícules (Física nuclear)Ultra high energy cosmic rayAtmosphere[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Air-showersSEARCHNeutrino0103 physical sciencesddc:530010306 general physicsAstrophysiqueCiencias ExactasPierre Auger ObservatoryAstroparticle physicsSPECTRUM010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaUltra high energy cosmic raystelescopes//purl.org/becyt/ford/1.3 [https]Ultrahigh Energyflux13. Climate actionenergy [neutrino]Pierre AugerExperimental High Energy PhysicsARRAYHigh Energy Physics::ExperimentAstroparticle physicslcsh:Physics
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Ultra-high temperature metamorphism recorded in Fe-rich olivine-bearing migmatite from the Khondalite Belt, North China Craton

2018

International audience; We document the first occurrence of Fe‐rich olivine‐bearing migmatitic metapelite in the Khondalite Belt, North China Craton. Petrological analyses revealed two exotic assemblages of orthopyroxene+spinel+olivine and orthopyroxene+spinel+cordierite. Phase relation modelling suggests that these assemblages are diagnostic of ultra‐high temperature (UHT) metamorphism in the Fe‐rich system, with temperatures from 1,000 to 1,050°C at 0.6 GPa. U–Th–Pb SIMS analyses on zircon reveal a similar age of c. 1.92 Ga for the olivine‐bearing migmatite and an adjacent gabbronoritic intrusion that is therefore identified as the heat source for the UHT metamorphism. These results, coup…

ultra-high temperature metamorphism010504 meteorology & atmospheric sciencesGeochemistry[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/PetrographyMetamorphismengineering.material010502 geochemistry & geophysics01 natural sciencesNorth China CratonKhondalite BeltGeochemistry and PetrologymigmatitesPetrology0105 earth and related environmental sciences[ SDU.STU.PE ] Sciences of the Universe [physics]/Earth Sciences/Petrographygeographygeography.geographical_feature_categoryOlivineUltra-high-temperature metamorphismGeologymetamorphic olivineMigmatiteGranuliteCraton13. Climate actionengineeringKhondaliteMaficGeology
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"Table 2" of "Measurement of azimuthal anisotropy of muons from charm and bottom hadrons in $pp$ collisions at $\sqrt{s}=13$ TeV with the ATLAS detec…

2020

Summary of results for inclusive muon v2 as a function of pT. Uncertainties are statistical and systematic, respectively.

v213000.0Physics::Instrumentation and DetectorsP P --> HF muon + XPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentHF muonProton-Proton Collision
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"Table 1" of "Measurement of azimuthal anisotropy of muons from charm and bottom hadrons in $pp$ collisions at $\sqrt{s}=13$ TeV with the ATLAS detec…

2020

Summary of results for inclusive muon v2 as a function of multiplicity. Uncertainties are statistical and systematic, respectively.

v213000.0Physics::Instrumentation and DetectorsP P --> HF muon + XPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentHF muonProton-Proton Collision
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"Table 20" of "Investigations of anisotropic flow using multi-particle azimuthal correlations in pp, p-Pb, Xe-Xe, and Pb-Pb collisions at the LHC"

2019

$v_2\{2\}$ with $|\Delta \eta| > 1.4$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

v22Gap14Xe Xe --> CHARGED XHigh Energy Physics::Experiment5440.0Nuclear Experiment
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"Table 22" of "Investigations of anisotropic flow using multi-particle azimuthal correlations in pp, p-Pb, Xe-Xe, and Pb-Pb collisions at the LHC"

2019

$v_4\{2\}$ with $|\Delta \eta| > 1.0$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

v42Gap10Xe Xe --> CHARGED XHigh Energy Physics::Experiment5440.0Nuclear Experiment
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"Table 22" of "Combination of the searches for pair-produced vector-like partners of the third-generation quarks at $\sqrt{s} =$ 13 TeV with the ATLA…

2018

Expected and observed 95% upper limits on the vector-like bottom quark pair-production signal strength (i.e. the ratio sigma_exclusion/sigma_VLQ) as a function of the branching ratio for a vector-like quark mass of 1400 GeV, asumming that the vector-like quarks exclusively decay to SM particles (and third generation quarks). If interpreting these results in models with decays to non-Standard-Model particles, one must check that the additional decays will not end up in any control regions of the relevant analyses.

vector-like quarkspair-productionHigh Energy Physics::LatticeP P --> T THigh Energy Physics::PhenomenologyHigh Energy Physics::Experiment13000upper cross-section limit
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"Table 20" of "Combination of the searches for pair-produced vector-like partners of the third-generation quarks at $\sqrt{s} =$ 13 TeV with the ATLA…

2018

Expected and observed 95% upper limits on the vector-like bottom quark pair-production signal strength (i.e. the ratio sigma_exclusion/sigma_VLQ) as a function of the branching ratio for a vector-like quark mass of 1200 GeV, asumming that the vector-like quarks exclusively decay to SM particles (and third generation quarks). If interpreting these results in models with decays to non-Standard-Model particles, one must check that the additional decays will not end up in any control regions of the relevant analyses.

vector-like quarkspair-productionHigh Energy Physics::LatticeP P --> T THigh Energy Physics::PhenomenologyHigh Energy Physics::Experiment13000upper cross-section limit
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