Search results for "53"

showing 10 items of 2908 documents

First moments of the nucleon generalized parton distributions from lattice QCD

2012

We report on our lattice calculations of the nucleon's generalized parton distributions (GPDs), concentrating on their first moments for the case of N_f=2. Due to recent progress on the numerical side we are able to present results for the generalized form factors at pion masses as low as 260 MeV. We perform a fit to one-loop covariant baryon chiral perturbation theory with encouraging results.

010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyNuclear TheoryFOS: Physical sciencesDESYPartonLattice QCD01 natural sciencesNuclear physicsHigh Energy Physics - LatticeResearch centre0103 physical sciencesddc:530Nuclear Experiment010306 general physicsNucleon
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Effective characterization of the phase and intensity profiles of asymmetrically distorted light pulses in optical fiber systems

2009

International audience; We address the problem of characterization of light pulses that propagate in long-haul high-bit-rate optical communication systems under strongly perturbed conditions. We show that the conventional technique for characterization of the phase and intensity profile of such pulses becomes qualitatively inconsistent when the pulse's profile is asymmetrically distorted with respect to its center of mass. We resolve these inconsistencies by partially reformulating the conventional technique by means of appropriate pulse parameters, which we call upgraded parameters, that allow a fair characterization of the intensity and phase of all types of light pulses, including those …

010309 optics[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[CHIM.THEO] Chemical Sciences/Theoretical and/or physical chemistry020210 optoelectronics & photonics0103 physical sciences[ CHIM.THEO ] Chemical Sciences/Theoretical and/or physical chemistry0202 electrical engineering electronic engineering information engineeringStatistical and Nonlinear Physics02 engineering and technology190.5530 060.5530 060.2330 060.2360 060.451001 natural sciencesAtomic and Molecular Physics and Optics
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The 1430s: a cold period of extraordinary internal climate variability during the early Spörer Minimum with social and economic impacts in north-west…

2016

Changes in climate affected human societies throughout the last millennium. While European cold periods in the 17th and 18th century have been assessed in detail, earlier cold periods received much less attention due to sparse information available. New evidence from proxy archives, historical documentary sources and climate model simulations permit us to provide an interdisciplinary, systematic assessment of an exceptionally cold period in the 15th century. Our assessment includes the role of internal, unforced climate variability and external forcing in shaping extreme climatic conditions and the impacts on and responses of the medieval society in north-western and central Europe. Climate…

010504 meteorology & atmospheric sciences530 PhysicsStratigraphyFood prices010502 geochemistry & geophysics01 natural sciencesProxy (climate)medicineEconomic impact analysis910 Geography & travel550 Earth sciences & geology0105 earth and related environmental sciencesGlobal and Planetary Change300 Social sciences sociology & anthropologyPaleontologySubsistence agriculture15. Life on landSeasonalitymedicine.disease13. Climate actionClimatologyFamine570 Life sciences; biologyClimate modelGlobal and Planetary Change900 History
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Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A 3-Year Sample of Almost 1,600 Elves Recorded Above South America by the Pierre Auger Cosmic-Ray Observatory

2020

The time and location of the 1,598 verified and reconstructed elves, used for the analysis showcased in this paper, are publicly available on the website of the Pierre Auger Observatory (https://www.auger.org/ index.php/science/data). We wish to thank the World Wide Lightning Location Network (http://wwlln.net), a collaboration among over 50 universities and institutions, for providing the lightning location data used in this paper. We acknowledge Robert Marshall for providing one of the most advanced elve simulations to the public, a key tool in understanding the elves observed by the Pierre Auger Observatory. The successful installation, commissioning, and operation of the Pierre Auger Ob…

010504 meteorology & atmospheric sciencesAstronomyField of view010502 geochemistry & geophysics01 natural sciences7. Clean energyAugerlcsh:QB1-991ObservatoryultravioletStormddc:550UHE Cosmic Raystime resolutionCosmic-ray observatoryPhysicslcsh:QE1-996.5astro-ph.GeologyAugerwidth [beam]IonosphereField of viewGeologylcsh:AstronomyUHE [cosmic radiation]Environmental Science (miscellaneous)horizonLightningddc:530High Energy PhysicsIonosphereCosmic-ray observatory0105 earth and related environmental sciencesfluorescence [detector]backgroundFísicaAstronomyStormsensitivityLightningopticslcsh:GeologyElves UV fluorescence detectorsThunderstorm13. Climate actionExperimental High Energy PhysicsnetworkThunderstormGeneral Earth and Planetary SciencesElvesObservatory
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A giant exoplanet orbiting a very-low-mass star challenges planet formation models

2019

Surveys have shown that super-Earth and Neptune-mass exoplanets are more frequent than gas giants around low-mass stars, as predicted by the core accretion theory of planet formation. We report the discovery of a giant planet around the very-low-mass star GJ 3512, as determined by optical and near-infrared radial-velocity observations. The planet has a minimum mass of 0.46 Jupiter masses, very high for such a small host star, and an eccentric 204-day orbit. Dynamical models show that the high eccentricity is most likely due to planet-planet interactions. We use simulations to demonstrate that the GJ 3512 planetary system challenges generally accepted formation theories, and that it puts con…

010504 meteorology & atmospheric sciencesGas giant530 PhysicsFOS: Physical sciencesMinimum massAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSettore FIS/05 - Astronomia e AstrofisicaPlanet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsMultidisciplinary520 AstronomyGiant planetAstronomyPlanetary system620 EngineeringAccretion (astrophysics)ExoplanetOrbitAstrophysics - Solar and Stellar Astrophysics13. Climate actionAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Earth and Planetary AstrophysicsScience
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Microbiology and atmospheric processes: biological, physical and chemical characterization of aerosol particles

2008

Abstract. The interest in bioaerosols has traditionally been linked to health hazards for humans, animals and plants. However, several components of bioaerosols exhibit physical properties of great significance for cloud processes, such as ice nucleation and cloud condensation. To gain a better understanding of their influence on climate, it is therefore important to determine the composition, concentration, seasonal fluctuation, regional diversity and evolution of bioaerosols. In this paper, we will review briefly the existing techniques for detection, quantification, physical and chemical analysis of biological particles, attempting to bridge physical, chemical and biological methods for …

010504 meteorology & atmospheric sciencesIndoor bioaerosollcsh:LifeBiological particles[SDU.STU]Sciences of the Universe [physics]/Earth SciencesNanotechnology[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]03 medical and health scienceslcsh:QH540-549.5[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentEcology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface Processes[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere0303 health sciences[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.OCEAN] Sciences of the Universe [physics]/Ocean Atmosphere030306 microbiologyChemistrylcsh:QE1-996.5[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentAerosolCharacterization (materials science)lcsh:Geologylcsh:QH501-531[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]13. Climate action[SDU.STU] Sciences of the Universe [physics]/Earth SciencesIce nucleuslcsh:EcologyBiochemical engineeringAerosol sampling
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2016

Gianluca Tramontana was supported by the GEOCARBON EU FP7 project (GA 283080). Dario Papale, Martin Jung and Markus Reichstein acknowledge funding from the EU FP7 project GEOCARBON (grant agreement no. 283080) and the EU H2020 BACI project (grant agreement no. 640176). Gustau Camps-Valls wants to acknowledge the support by an ERC Consolidator Grant with grant agreement 647423 (SEDAL). Kazuhito Ichii was supported by Environment Research and Technology Development Funds (2-1401) from the Ministry of the Environment of Japan and the JAXA Global Change Observation Mission (GCOM) project (no. 115). Christopher R. Schwalm was supported by National Aeronautics and Space Administration (NASA) gran…

010504 meteorology & atmospheric sciencesMeteorologyFLUXNET0208 environmental biotechnology0207 environmental engineeringlcsh:Life02 engineering and technologySensible heatAtmospheric sciences7. Clean energy01 natural sciencesFlux (metallurgy)FluxNetMachine learning; Carbon fluxes; Energy fluxes; FLUXNET; Remote sensing; FLUXCOMlcsh:QH540-549.5Latent heatMachine learningCarbon fluxes020701 environmental engineeringEcology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface ProcessesFLUXCOMMultivariate adaptive regression splineslcsh:QE1-996.5Empirical modellingPrimary production15. Life on landRemote sensingEnergy fluxes020801 environmental engineeringlcsh:Geologylcsh:QH501-531Kernel method13. Climate actionEnvironmental sciencelcsh:EcologyBiogeosciences
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Assessing optimal water quality monitoring network in road construction using integrated information-theoretic techniques

2020

Author´s accepted manuscript. The environmental impacts of road construction on the aquatic environment necessitate the monitoring of receiving water quality. The main contribution of the paper is developing a feasible methodology for spatial optimization of the water quality monitoring network (WQMN) in surface water during road construction using the field data. First, using the Canadian Council of Ministers of the Environment (CCME) method, the water quality index (WQI) was computed in each potential monitoring station during construction. Then, the integrated form of the information-theoretic techniques consists of the transinformation entropy (TE), and the value of information (VOI) we…

010504 meteorology & atmospheric sciencesRoad constructionOperations researchComputer science0207 environmental engineeringAnalytic hierarchy processTOPSIS02 engineering and technologyIdeal solutionMutual informationVDP::Teknologi: 500::Bygningsfag: 530::Konstruksjonsteknologi: 53301 natural sciencesValue of informationEntropy (information theory)Water quality020701 environmental engineering0105 earth and related environmental sciencesWater Science and TechnologyJournal of Hydrology
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Observation of classically 'forbidden' electromagnetic wave propagation and implications for neutrino detection.

2018

Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled wi…

010504 meteorology & atmospheric sciencesWave propagationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesElectromagnetic radiationAtomicIce shelfParticle and Plasma Physics0103 physical sciencesddc:530NuclearInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)geographygeography.geographical_feature_categoryultra high energy photons and neutrinos010308 nuclear & particles physicsMolecularAstronomy and AstrophysicsNuclear & Particles PhysicsComputational physicsRay tracing (physics)Radio propagationNeutrino detectorcosmic ray experimentsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesRadio wave
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