Search results for "ddc:5"

showing 10 items of 1717 documents

Tevatron Run II combination of the effective leptonic electroweak mixing angle

2018

The Ministry of Science and Innovation and the Consolider-Ingenio 2010 Program and the European Union community Marie Curie Fellowship Contract No. 302103.

Drell-Yan processsemianalytical programsPhysics and Astronomy (miscellaneous)FERMION PAIR PRODUCTIONUPGRADETevatronhadron-colliders01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & Fieldselectron: pair productionHigh Energy Physics - Experiment (hep-ex)MONTE-CARLOUNIVERSAL MONTE-CARLOELECTROMAGNETIC CALORIMETERDZERO[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]HADRON COLLIDERSangular distributionBatavia TEVATRON CollMonte CarloPhysicsscattering [anti-p p]gauge bosonPhysicsElectroweak interactionDrell–Yan processWeinberg anglespontaneous symmetry breaking [electroweak interaction]muon: pair productionPhysical Sciencesmixing angle [electroweak interaction]bosonPHOTOSmass: measured [W]asymmetryParticle physicsFOS: Physical sciencesSEMIANALYTICAL PROGRAMddc:500.2Astronomy & Astrophysicselectroweak interaction: spontaneous symmetry breaking114 Physical sciences530programmingW: mass: measuredStandard Modelanti-p p: colliding beams[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]hadroproduction [Z0]0103 physical sciencesanti-p p: scatteringddc:530High Energy Physicspair production [electron]pair production [muon]CALORIMETER010306 general physicsQED RADIATIVE-CORRECTIONSQed radiative-corrections; fermion pair production; universal; Monte Carlo; parton distributions; hadron-colliders; electromagnetic; calorimeter;semianalytical programs; E(+)E(-) annihilation; boson; production; D0 detectorGauge bosonBOSON PRODUCTIONMuonScience & Technologyelectroweak interaction: mixing angleAnti-p p: scattering | anti-p p: colliding beams | Z0: hadroproduction | Z0: leptonic decay | electroweak interaction: spontaneous symmetry breaking | electroweak interaction: mixing angle | muon: pair production | W: mass: measured | Weinberg angle | Batavia TEVATRON Coll | angular distribution | electron: pair production | Drell-Yan process | gauge boson | programming | asymmetry | CDF | DZERO | experimental resultsIDENTIFICATION010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyuniversalWeinberg angleZ0: hadroproductionQED RADIATIVE-CORRECTIONS; FERMION PAIR PRODUCTION; UNIVERSAL; MONTE-CARLO; PARTON DISTRIBUTIONS; HADRON COLLIDERS; ELECTROMAGNETIC; CALORIMETER; SEMIANALYTICAL PROGRAM; E(+)E(-) ANNIHILATION; BOSON; PRODUCTION; D0 DETECTORleptonic decay [Z0]E(+)E(-) ANNIHILATIONelectromagneticPARTON DISTRIBUTIONSExperimental High Energy PhysicsZ0: leptonic decayD0 DETECTORCDFHigh Energy Physics::Experimentproductioncolliding beams [anti-p p]Leptonexperimental results
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Drift Time Measurement in the ATLAS Liquid Argon Electromagnetic Calorimeter using Cosmic Muons

2010

The ionization signals in the liquid argon of the ATLAS electromagnetic calorimeter are studied in detail using cosmic muons. In particular, the drift time of the ionization electrons is measured and used to assess the intrinsic uniformity of the calorimeter gaps and estimate its impact on the constant term of the energy resolution. The drift times of electrons in the cells of the second layer of the calorimeter are uniform at the level of 1.3% in the barrel and 2.8% in the endcaps. This leads to an estimated contribution to the constant term of (0.29-0.04+0.05)% in the barrel and (0.54-0.04+0.06)% in the endcaps. The same data are used to measure the drift velocity of ionization electrons …

Drift velocityPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsInstrumentationFOS: Physical sciencesddc:500.2ElectronAstrophysics::Cosmology and Extragalactic AstrophysicsElectromagnetic CalorimeterATLAS; Drift Time Measurement; Cosmic Muons5307. Clean energy01 natural sciencesPartícules (Física nuclear)High Energy Physics - Experiment010305 fluids & plasmasNuclear physicsHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)Ionization0103 physical sciencesmedicineFysikddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Cosmic MuonsDetectors and Experimental Techniques010306 general physicsEngineering (miscellaneous)Ciencias ExactasDetectors de radiacióPhysicsCalorimeter (particle physics)010308 nuclear & particles physicsAcceleradors de partículesResolution (electron density)Instrumentation and Detectors (physics.ins-det)ATLASliquid argonElectromagnetic calorimetermedicine.anatomical_structureExperimental High Energy PhysicsDrift Time MeasurementPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::ExperimentLHC
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Trace gas composition in the Asian summer monsoon anticyclone: a case study based on aircraft observations and model simulations

2017

We present in situ measurements of the trace gas composition of the upper tropospheric (UT) Asian summer monsoon anticyclone (ASMA) performed with the High Altitude and Long Range Research Aircraft (HALO) in the frame of the Earth System Model Validation (ESMVal) campaign. Air masses with enhanced O3 mixing ratios were encountered after entering the ASMA at its southern edge at about 150 hPa on 18 September 2012. This is in contrast to the presumption that the anticyclone's interior is dominated by recently uplifted air with low O3 in the monsoon season. We also observed enhanced CO and HCl in the ASMA, which are tracers for boundary layer pollution and tropopause layer (TL) air or stratosp…

ECHAMAtmospheric Science010504 meteorology & atmospheric sciences010502 geochemistry & geophysicsMonsoonAtmospheric scienceschemistry01 natural scienceslcsh:ChemistryTropospheretrace gasesErdsystem-Modellierungddc:550atmospheric modelling0105 earth and related environmental sciencesAtmosphereAsian summer monsoonAtmosphärische Spurenstoffelcsh:QC1-999Trace gasBoundary layerEarth scienceslcsh:QD1-999Anticyclone13. Climate actionClimatologyHYSPLITTropopauseaircraft measurementslcsh:PhysicsGeology
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Modeling the aerosol chemical composition of the tropopause over the Tibetan Plateau during the Asian summer monsoon

2019

Enhanced aerosol abundance in the upper troposphere and lower stratosphere (UTLS) associated with the Asian summer monsoon (ASM) is referred to as the Asian Tropopause Aerosol Layer (ATAL). The chemical composition, microphysical properties, and climate effects of aerosols in the ATAL have been the subject of discussion over the past decade. In this work, we use the ECHAM/MESSy Atmospheric Chemistry (EMAC) general circulation model at a relatively fine grid resolution (about 1.1×1.1∘) to numerically simulate the emissions, chemistry, and transport of aerosols and their precursors in the UTLS within the ASM anticyclone during the years 2010–2012. We find a pronounced maximum of aerosol extin…

ECHAMAtmospheric SciencegeographyPlateaugeography.geographical_feature_category010504 meteorology & atmospheric sciences010501 environmental sciencesMineral dustrespiratory systemAtmospheric sciences01 natural scienceslcsh:QC1-999Aerosollcsh:ChemistryTropospherelcsh:QD1-999Anticycloneddc:550TropopauseStratospherelcsh:Physics0105 earth and related environmental sciences
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The on-line coupled atmospheric chemistry model system MECO(n) – Part 5: Expanding the Multi-Model-Driver (MMD v2.0) for 2-way data exchange includin…

2018

Abstract. As part of the Modular Earth Submodel System (MESSy), the Multi-Model-Driver (MMD v1.0) was developed to couple online the regional Consortium for Small-scale Modeling (COSMO) model into a driving model, which can be either the regional COSMO model or the global European Centre Hamburg general circulation model (ECHAM) (see Part 2 of the model documentation). The coupled system is called MECO(n), i.e., MESSy-fied ECHAM and COSMO models nested n times. In this article, which is part of the model documentation of the MECO(n) system, the second generation of MMD is introduced. MMD comprises the message-passing infrastructure required for the parallel execution (multiple programme mul…

ECHAMatmospheric chemistryTheoretical computer science010504 meteorology & atmospheric sciencesComputer science0208 environmental biotechnology02 engineering and technology01 natural sciencesComputational scienceMESSyMECO(n)Erdsystem-Modellierungddc:550multi-scale modelling0105 earth and related environmental sciencesEMACtwo-way-nestinCOSMObusiness.industrylcsh:QE1-996.5grid transformationModular designGrid020801 environmental engineeringlcsh:GeologyEarth sciencesTransformation (function)Modular Earth Submodel SystemData exchangeLine (geometry)dustGRIDbusinessMulti-Model-DriverremappingInterpolationData transmissionGeoscientific Model Development
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Atomic Structures of Two Novel Immunoglobulin-like Domain Pairs in the Actin Cross-linking Protein Filamin

2009

Filamins are actin filament cross-linking proteins composed of an N-terminal actin-binding domain and 24 immunoglobulin-like domains (IgFLNs). Filamins interact with numerous proteins, including the cytoplasmic domains of plasma membrane signaling and cell adhesion receptors. Thereby filamins mechanically and functionally link the cell membrane to the cytoskeleton. Most of the interactions have been mapped to the C-terminal IgFLNs 16–24. Similarly, as with the previously known compact domain pair of IgFLNa20–21, the two-domain fragments IgFLNa16–17 and IgFLNa18–19 were more compact in small angle x-ray scattering analysis than would be expected for two independent domains. Solution state NM…

EGF-like domainFilaminsMolecular Sequence DataMolecular ConformationImmunoglobulinsmacromolecular substancesPlasma protein bindingBiologyFilaminModels BiologicalBiochemistryCell membraneHAMP domain03 medical and health sciencesContractile Proteins0302 clinical medicineddc:570Cell AdhesionmedicineHumansScattering RadiationAmino Acid SequenceCytoskeletonCell adhesionMolecular BiologyCytoskeletonActin030304 developmental biology0303 health sciencesMicrofilament ProteinsCell BiologyActinsRecombinant ProteinsProtein Structure Tertiary3. Good healthCell biologyCross-Linking Reagentsmedicine.anatomical_structureProtein Structure and Folding030217 neurology & neurosurgeryProtein BindingJournal of Biological Chemistry
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South Pole glacial climate reconstruction from multi-borehole laser particulate stratigraphy

2013

AbstractThe IceCube Neutrino Observatory and its prototype, AMANDA, were built in South Pole ice, using powerful hot-water drills to cleanly bore>100 holes to depths up to 2500 m. The construction of these particle physics detectors provided a unique opportunity to examine the deep ice sheet using a variety of novel techniques. We made high-resolution particulate profiles with a laser dust logger in eight of the boreholes during detector commissioning between 2004 and 2010. The South Pole laser logs are among the most clearly resolved measurements of Antarctic dust strata during the last glacial period and can be used to reconstruct paleoclimate records in exceptional detail. Here we use…

EPICA-DOME-C010504 meteorology & atmospheric sciencesDEEP ICEBoreholeAntarctic ice sheetDUSTddc:500.2ANTARCTIC ICE-SHEET01 natural sciencesIceCube Neutrino ObservatoryIceCubePaleontology0103 physical sciencesPaleoclimatologyddc:550COREGlacial period010303 astronomy & astrophysicsSIPLE DOME0105 earth and related environmental sciencesEarth-Surface Processesgeographygeography.geographical_feature_categoryEAST ANTARCTICAVOLCANIC WINTERVOSTOKOPTICAL-PROPERTIESStratigraphy13. Climate actionEarth and Environmental SciencesRadiometric datingIce sheetphysicsGeology
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Unveiling the strong interaction among hadrons at the LHC

2020

One of the key challenges for nuclear physics today is to understand from first principles the effective interaction between hadrons with different quark content. First successes have been achieved using techniques that solve the dynamics of quarks and gluons on discrete space-time lattices1,2. Experimentally, the dynamics of the strong interaction have been studied by scattering hadrons off each other. Such scattering experiments are difficult or impossible for unstable hadrons3–6 and so high-quality measurements exist only for hadrons containing up and down quarks7. Here we demonstrate that measuring correlations in the momentum space between hadron pairs8–12 produced in ultrarelativistic…

EXCHANGE-POTENTIAL APPROACHStrange quarkALICE CollaborationHadronNuclear TheoryStrong interaction; hadron collisionsPosition and momentum spacehiukkasfysiikkanucl-ex7. Clean energy01 natural sciencesVDP::Fysikk: 430High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Hadron-Hadron scattering (experiments)scattering [hadron]p p scattering[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]Nuclear Experiment (nucl-ex)Experimental nuclear physicsNUCLEONNuclear ExperimentNuclear ExperimentVDP::Physics: 430PhysicsMultidisciplinaryLarge Hadron ColliderPhysicsstrong interactionlattice [space-time]Publisher CorrectionPRIRODNE ZNANOSTI. Fizika.EXCHANGE-POTENTIAL APPROACH; BARYON-BARYON SCATTERING; NUCLEONCERN LHC CollLHCddc:500NucleonBARYON-BARYON SCATTERINGParticle Physics - Experimentdiscrete [space-time]QuarkParticle physicshadron collisionsCERN LabGeneral Science & TechnologyStrong interactionFOS: Physical sciencesshort-rangeHadron strong interaction LHC114 Physical sciences:Fysikk: 430 [VDP]Articlehadron scatteringquarkultrarelativistic proton–proton collisions LHC ALICE0103 physical sciencesNuclear Physics - ExperimentGeneral010306 general physics:Physics: 430 [VDP]interaction [hadron hadron]hep-ex010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyeffect [strong interaction]hadron-hadron interactionhadron scattering ; hadron-hadron interaction ; strong interaction: effect ; space-time: discrete ; space-time: lattice ; p p scattering ; quark ; correlation ; CERN LHC CollNATURAL SCIENCES. Physics.BaryoncorrelationHypernuclei; Neutron Stars; StrangenessPhysics::Accelerator PhysicsHigh Energy Physics::ExperimenthadronExperimental particle physicsNature
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Infrasonic, Acoustic and Seismic Waves Produced by the Axion Quark Nuggets

2022

We advocate an idea that the Axion Quark Nuggets (AQN) hitting the Earth can be detected by analysing the infrasound, acoustic and seismic waves which always accompany the AQN's passage in the atmosphere and underground. Our estimates for the infrasonic frequency $\nu\simeq 5$ ~Hz and overpressure $\delta p\sim 0.3 ~$Pa for relatively large size dark matter (DM) nuggets suggest that sensitivity of presently available instruments is already sufficient to detect very intense (but very rare) events today with existing technology. A study of much more frequent but less intense events requires a new type of instruments. We propose a detection strategy for a systematic study to search for such re…

Earth and Planetary Astrophysics (astro-ph.EP)570Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)General MathematicsFOS: Physical sciencesGeophysics (physics.geo-ph)Physics - GeophysicsHigh Energy Physics - PhenomenologyPhysics - Atmospheric and Oceanic PhysicsHigh Energy Physics - Phenomenology (hep-ph)Chemistry (miscellaneous)ddc:570Atmospheric and Oceanic Physics (physics.ao-ph)Computer Science (miscellaneous)dark matter; axion; quark nuggetsAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics - Earth and Planetary AstrophysicsSymmetry
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Polar motion prediction using the combination of SSA and Copula-based analysis

2018

The real-time estimation of polar motion (PM) is needed for the navigation of Earth satellite and interplanetary spacecraft. However, it is impossible to have real-time information due to the complexity of the measurement model and data processing. Various prediction methods have been developed. However, the accuracy of PM prediction is still not satisfactory even for a few days in the future. Therefore, new techniques or a combination of the existing methods need to be investigated for improving the accuracy of the predicted PM. There is a well-introduced method called Copula, and we want to combine it with singular spectrum analysis (SSA) method for PM prediction. In this study, first, we…

Earth satellite010504 meteorology & atmospheric scienceslcsh:GeodesyPolar motion010502 geochemistry & geophysics01 natural sciencesCopula (probability theory)Prediction methodsddc:550Applied mathematicsEOPSSASingular spectrum analysis0105 earth and related environmental sciencespolar motionData processinglcsh:QB275-343Full Paperlcsh:QE1-996.5lcsh:Geography. Anthropology. RecreationGeologyInternational Earth Rotation and Reference Systems ServiceMatemática Aplicadaprediction550 Geowissenschaftenlcsh:Geologylcsh:GCopulaSpace and Planetary SciencePolar motionPredictionHybrid modelEarth, Planets and Space
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