Search results for "ddc:5"

showing 10 items of 1717 documents

Shake-table testing of a stone masonry building aggregate: overview of blind prediction study

2023

Bulletin of earthquake engineering (2023). doi:10.1007/s10518-022-01582-x special issue: "Adjacent Interacting Masonry Structures"

Shake-table test550Incremental dynamic analysisincremental dynamic analysisheritagepushover analysismodelsddc:550masonry aggregatesBlind predictionHistorical masonry Masonry aggregates Incremental dynamic analysis Shake-table test Blind predictionCivil and Structural Engineeringhistorical masonryshake-table testwallsBuilding and ConstructionGeotechnical Engineering and Engineering GeologyBlind prediction; Historical masonry; Incremental dynamic analysis; Masonry aggregates; Shake-table testSettore ICAR/09 - Tecnica Delle CostruzioniGeophysicsseismic assessmentblind predictionHistorical masonryMasonry aggregatesstrengthperformance
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First Study on Nihonium (Nh, Element 113) Chemistry at TASCA

2021

Frontiers in Chemistry 9, 753738 (2021). doi:10.3389/fchem.2021.753738

Shell (structure)Analytical chemistrychemistry.chemical_elementSuperheavy Elementselement 113gas phase chromatographyAtomic orbitalatomifysiikkaTASCAReactivity (chemistry)QD1-999Original ResearchIsotopeGeneral Chemistry540superheavy elementkemialliset ominaisuudetChemistryFleroviumsuperheavy elementsUnpaired electronchemistrynihoniumddc:540physical preseparationVolatility (chemistry)
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Observation of a $\gamma$-decaying millisecond isomeric state in $^{128}$Cd$_{80}$

2017

A. Jungclaus et al. -- 6 pags., 5 figs., 2 tabs. -- Open Access funded by Creative Commons Atribution Licence 4.0

Shell model calculationNuclear and High Energy PhysicsFissionSHELL modelNuclear TheoryShell model calculationsTransition strengths[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energy0103 physical sciencesmedicineddc:530010306 general physicsNuclear ExperimentPhysicsMillisecondRadionuclideIsomeric decay010308 nuclear & particles physicsProjectileParity (physics)lcsh:QC1-999medicine.anatomical_structureIsomeric decaysPhysics::Accelerator PhysicsTransition strengthAtomic physicsNucleuslcsh:Physics
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Impact of red giant/AGB winds on active galactic nucleus jet propagation

2017

Astronomy and astrophysics 606, A40 (2017). doi:10.1051/0004-6361/201630117

Shock waveAstrofísicaActive galactic nucleusRed giantAstrophysics::High Energy Astrophysical PhenomenaContext (language use)AstrophysicsAstrophysics01 natural sciencesJets (Astrofísica)0103 physical sciencesAsymptotic giant branchAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsMixing (physics)Astrophysics::Galaxy AstrophysicsPhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and Astrophysics520Astrophysical jetsStars13. Climate actionSpace and Planetary ScienceGalàxies activesActive galaxiesddc:520
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Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment

2018

Monthly notices of the Royal Astronomical Society 479(3), 4253 - 4270 (2018). doi:10.1093/mnras/sty1750

Shock waveshock wave010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesISM: magnetic field0103 physical sciencesRadiative transferAdiabatic process010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicssupernova remnants [ISM]magnetic fields [ISM]Astronomy and Astrophysicsshock wavesAstronomy and Astrophysic520Magnetic fieldSupernovaSpace and Planetary Scienceddc:520Oblique shockMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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Arbitrary Phase Access for Stable Fiber Interferometers

2021

Well-controlled yet practical systems that give access to interference effects are critical for established and new functionalities in ultrafast signal processing, quantum photonics, optical coherence characterization, etc. Optical fiber systems constitute a central platform for such technologies. However, harnessing optical interference in a versatile and stable manner remains technologically costly and challenging. Here, degrees of freedom native to optical fibers, i.e., polarization and frequency, are used to demonstrate an easily deployable technique for the retrieval and stabilization of the relative phase in fiber interferometric systems. The scheme gives access (without intricate dev…

Signal processingPhase (waves)Physics::Opticsquantum photonics01 natural sciencesDegrees of freedom (mechanics)Quantum entanglement010309 opticsOpticsinterferometers0103 physical sciencesAstronomical interferometerddc:530Optical fibersFiber interferometersFiber010306 general physicsOptical reference signalsPhysicsPhotonsUltrafast signal processingInterference effectsbusiness.industryOptical fiber systemsReference signalsSettore ING-INF/02 - Campi ElettromagneticiCondensed Matter PhysicsParticle beamsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsSingle-photon detectorscoherent signal processingDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikinterferometers coherent signal processing quantum photonicsbusinessInterferometric systemLaser & Photonics Reviews
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Probing the radio emission from air showers with polarization measurements

2014

The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially wit…

SignalsAstronomy01 natural sciencesElectric fieldComputational physicsCosmic-raysComposition energy spectra and interactionscosmic rayRadio wavePhysicsEarth's magnetic fieldHigh Energy Astrophysical Phenomena (astro-ph.HE)Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsPolarization (waves)Polarization (waves)BolometersThunderstormsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCAMPO MAGNÉTICOradio emissionRadio waveNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerComposition energy spectra and interactions; Solar electromagnetic emission; BolometersAstrophysics::High Energy Astrophysical Phenomenainfrared submillimeter wave microwave and radiowave receivers and detectorsFieldFOS: Physical sciencesPierre Auger Observatory ; air shower ; radio emissionRadiationMonte-carlo SimulationsOpticsElectric field0103 physical sciencesddc:530Pierre auger observatory010306 general physicsPulsesInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industrySolar electromagnetic emissionFísicaOpticsDetectorComputational physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerEarth's magnetic fieldMagnetic fieldExperimental High Energy PhysicsbusinessCodalema
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Background studies for acoustic neutrino detection at the South Pole

2011

The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method to measure the tiny flux of cosmogenic neutrinos expected on Earth. The energy threshold for this process depends strongly on the absolute noise level in the target material. The South Pole Acoustic Test Setup (SPATS), deployed in the upper part of four boreholes of the IceCube Neutrino Observatory, has monitored the noise in Antarctic ice at the geographic South Pole for more than two years down to 500 m depth. The noise is very stable and Gaussian distributed. Lacking an in-situ calibration up to now, laboratory measurements have been used to estimate the absolute noise level in the 10 to …

SignalsTELESCOPEAbsolute noise levelAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstrophysics7. Clean energy01 natural sciencesIceCube Neutrino Observatorylaw.inventionIceCubeTelescopeAbsolute noise level; Acoustic neutrino detection; Neutrino flux limitNeutrino flux limitlawSIGNALS0103 physical sciencesWATERDetection theory010306 general physicsTelescopeInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsAcoustic neutrino detector010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsWaterAstronomy and AstrophysicsGeodesyAcoustic neutrino detectionNoiseNeutrino detectorPhysics and Astronomy13. Climate actionddc:540NeutrinoAstrophysics - Instrumentation and Methods for Astrophysics
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An Itô Formula for rough partial differential equations and some applications

2020

AbstractWe investigate existence, uniqueness and regularity for solutions of rough parabolic equations of the form $\partial _{t}u-A_{t}u-f=(\dot X_{t}(x) \cdot \nabla + \dot Y_{t}(x))u$ ∂ t u − A t u − f = ( X ̇ t ( x ) ⋅ ∇ + Y ̇ t ( x ) ) u on $[0,T]\times \mathbb {R}^{d}.$ [ 0 , T ] × ℝ d . To do so, we introduce a concept of “differential rough driver”, which comes with a counterpart of the usual controlled paths spaces in rough paths theory, built on the Sobolev spaces Wk,p. We also define a natural notion of geometricity in this context, and show how it relates to a product formula for controlled paths. In the case of transport noise (i.e. when Y = 0), we use this framework to prove a…

Sobolev spacePure mathematicsPartial differential equationMaximum principleProduct (mathematics)UniquenessChain ruleddc:510Parabolic partial differential equationVDP::Matematikk og Naturvitenskap: 400::Matematikk: 410AnalysisDomain (mathematical analysis)Mathematics
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Macro-regional Strategies, Cohesion Policy and Regional Cooperation in the European Union: Towards a Research Agenda

2018

Since 2009, the European Union has developed strategies for the Baltic Sea, Danube, Adriatic-Ionian and Alpine macro-regions. These macro-regional strategies represent a new tool of European Union governance that seeks to combine the community’s territorial cooperation and cohesion policy repertoire with intergovernmental ‘regional cooperation’ involving European Union member and partner countries. By establishing comprehensive governance architectures for cross-sectoral and trans-boundary policy coordination in areas such as transport infrastructure and environmental protection, macro-regional strategies seek to mobilise European Union member and non-member states alike in promoting and h…

Sociology and Political Science0211 other engineering and technologies02 engineering and technologyEuropean transnational cooperationRegional planning050602 political science & public administrationRegional scienceddc:550media_common.cataloged_instanceEuropean UnionEuropean unionMacro4407 Policy and AdministrationStock (geology)macro-regional strategiesmedia_common44 Human Society021110 strategic defence & security studiesCorporate governance05 social sciences4408 Political Science0506 political scienceregional cooperationBaltic seaPolitical Science and International RelationsTransport infrastructure
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