Search results for "Dynamic"

showing 10 items of 12329 documents

Application of optimized artificial intelligence algorithm to evaluate the heating energy demand of non-residential buildings at European level

2019

Abstract A reliable preliminary forecast of heating energy demand of a building by using a detailed dynamic simulation software typically requires an in-depth knowledge of the thermal balance, several input data and a very skilled user. The authors will describe how to use Artificial Neural Networks to predict the demand for thermal energy linked to the winter climatization of non-residential buildings. To train the neural network it was necessary to develop an accurate energy database that represents the basis of the training of a specific Artificial Neural Networks. Data came from detailed dynamic simulations performed in the TRNSYS environment. The models were built according to the stan…

Artificial neural networkDecision support toolComputer science020209 energyReliability (computer networking)02 engineering and technologyTRNSYSStandard deviationIndustrial and Manufacturing EngineeringBuilding simulationSoftware020401 chemical engineering0202 electrical engineering electronic engineering information engineering0204 chemical engineeringElectrical and Electronic EngineeringLearning algorithmThermal balanceCivil and Structural EngineeringSettore ING-IND/11 - Fisica Tecnica AmbientaleArtificial neural networkbusiness.industryMechanical EngineeringBuilding and ConstructionIndustrial engineeringPollutionDynamic simulationGeneral EnergyHigh energy performancebusinessEnergy (signal processing)Thermal energy
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Estimation of Granger causality through Artificial Neural Networks: applications to physiological systems and chaotic electronic oscillators

2021

One of the most challenging problems in the study of complex dynamical systems is to find the statistical interdependencies among the system components. Granger causality (GC) represents one of the most employed approaches, based on modeling the system dynamics with a linear vector autoregressive (VAR) model and on evaluating the information flow between two processes in terms of prediction error variances. In its most advanced setting, GC analysis is performed through a state-space (SS) representation of the VAR model that allows to compute both conditional and unconditional forms of GC by solving only one regression problem. While this problem is typically solved through Ordinary Least Sq…

Artificial neural networks; Chaotic oscillators; Granger causality; Multivariate time series analysis; Network physiology; Penalized regression techniques; Remote synchronization; State-space models; Stochastic gradient descent L1; Vector autoregressive modelGeneral Computer ScienceDynamical systems theoryComputer science02 engineering and technologyChaotic oscillatorsPenalized regression techniquesNetwork topologySettore ING-INF/01 - ElettronicaMultivariate time series analysisVector autoregression03 medical and health sciences0302 clinical medicineScientific Computing and Simulation0202 electrical engineering electronic engineering information engineeringRepresentation (mathematics)Optimization Theory and ComputationNetwork physiologyState-space modelsArtificial neural networkArtificial neural networksData ScienceTheory and Formal MethodsQA75.5-76.95Stochastic gradient descent L1Granger causality State-space models Vector autoregressive model Artificial neural networks Stochastic gradient descent L1 Multivariate time series analysis Network physiology Remote synchronization Chaotic oscillators Penalized regression techniquesRemote synchronizationStochastic gradient descentAutoregressive modelAlgorithms and Analysis of AlgorithmsVector autoregressive modelElectronic computers. Computer scienceSettore ING-INF/06 - Bioingegneria Elettronica E InformaticaGranger causality020201 artificial intelligence & image processingGradient descentAlgorithm030217 neurology & neurosurgeryPeerJ Computer Science
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Dynamic computed tomography: a novel technique to study lung aeration and atelectasis formation during experimental CPR

2002

Objective: To develop an image based technique to study the effect of different ventilatory strategies on lung ventilation and alveolar recruitment during cardiopulmonary resuscitation (CPR). Design: (1) Technical development of the following components: (a) construction of an external chest compression device, which does not interfere with CT imaging, and (b) development of a software tool to detect lung parenchyma automatically and to calculate radiological density parameters. (2) Feasibility studies: three strategies of CPR ventilation were performed and imaged in one animal each (pigs, 25 kg): volume-constant ventilation (VCV), no ventilation, or continuous airway pressure (CPAP). One m…

Artificial ventilationPulmonary AtelectasisSwinemedicine.medical_treatmentAtelectasisEmergency NursingIntensive careAnimalsMedicineCardiopulmonary resuscitationMechanical ventilationLungbusiness.industryHemodynamicsmedicine.diseaseCardiopulmonary ResuscitationHeart Arrestmedicine.anatomical_structureAnesthesiaEmergency MedicineBreathingFeasibility StudiesArterial bloodPulmonary VentilationTomography X-Ray ComputedCardiology and Cardiovascular MedicinebusinessResuscitation
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Understanding social behavior evolutions through agent-based modeling

2012

Agent-based social simulation as a computational approach to social simulation has been largely used to explore social phenomena. The purpose of this paper is to describe a theoretical model of transmission and evolution of social behaviors in a network of artificial societies (artificial world) using agent-based modeling technology. In this model, each agent (society) is subdivided into social behaviors where individual and social learning occur. The agent-agent interactions are carried out by their social behaviors; otherwise the agent-environment interactions through consumption of ecological resources by its social behaviors in repression and satisfaction. We distinguish social behavior…

Artificial worldSocial dynamicsGlobalizationManagement scienceComputer sciencebusiness.industryMulti-agent systemArtificial intelligencebusinessSocial learningSocial heuristicsSocial behaviorSocial simulation2012 International Conference on Multimedia Computing and Systems
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Dark coupling and gauge invariance

2010

We study a coupled dark energy–dark matter model in which the energymomentum exchange is proportional to the Hubble expansion rate. The inclusion of its perturbation is required by gauge invariance. We derive the linear perturbation equations for the gauge invariant energy density contrast and velocity of the coupled fluids, and we determine the initial conditions. The latter turn out to be adiabatic for dark energy, when assuming adiabatic initial conditions for all the standard fluids. We perform a full Monte Carlo Markov Chain likelihood analysis of the model, using WMAP 7-year data.

AstrofísicaAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Monte Carlo methodFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCosmological perturbation theoryGauge theoryAdiabatic process010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsMarkov chain Monte CarloHigh Energy Physics - PhenomenologyQuantum electrodynamicssymbolsDark energyHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Future CMB cosmological constraints in a dark coupled universe

2010

Cosmic microwave background satellite missions as the ongoing Planck experiment are expected to provide the strongest constraints on a wide set of cosmological parameters. Those constraints, however, could be weakened when the assumption of a cosmological constant as the dark energy component is removed. Here we show that it will indeed be the case when there exists a coupling among the dark energy and the dark matter fluids. In particular, the expected errors on key parameters as the cold dark matter density and the angular diameter distance at decoupling are significantly larger when a dark coupling is introduced. We show that it will be the case also for future satellite missions as EPIC…

AstrofísicaAstrophysics and AstronomyNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cold dark matterDark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyThermodynamics of the universeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsHot dark matterAstronomyHigh Energy Physics - PhenomenologyDark energyDark fluidAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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MOJAVE. XII. ACCELERATION AND COLLIMATION OF BLAZAR JETS ON PARSEC SCALES

2014

We report on the acceleration properties of 329 features in 95 blazar jets from the MOJAVE VLBA program. Nearly half the features and three-quarters of the jets show significant changes in speed and/or direction. In general, apparent speed changes are distinctly larger than changes in direction, indicating that changes in the Lorentz factors of jet features dominate the observed speed changes rather than bends along the line of sight. Observed accelerations tend to increase the speed of features near the jet base, $\lesssim 10-20$ parsecs projected, and decrease their speed at longer distances. The range of apparent speeds at fixed distance in an individual jet can span a factor of a few, i…

AstrofísicaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencessymbols.namesakeAcceleration0103 physical sciencesBlazar010303 astronomy & astrophysicsVery Long Baseline ArrayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Line-of-sightShock (fluid dynamics)010308 nuclear & particles physicsAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxyLorentz factorSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)AstronomiasymbolsAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

2019

We present the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1$\mathrm{M}_\odot$ during the first and second observing runs of the Advanced gravitational-wave detector network. During the first observing run (O1), from September $12^\mathrm{th}$, 2015 to January $19^\mathrm{th}$, 2016, gravitational waves from three binary black hole mergers were detected. The second observing run (O2), which ran from November $30^\mathrm{th}$, 2016 to August $25^\mathrm{th}$, 2017, saw the first detection of gravitational waves from a binary neutron star inspiral, in addition to the observation of gravitational waves from a total of seven binary …

AstrofísicaDYNAMICSGravitacióneutron star: binaryAstronomyGeneral Physics and AstronomyBinary numberAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology010305 fluids & plasmasgravitational waves black holesAstrophysicSIGNALSPopulation DistributionsLIGOQCQBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HESettore FIS/01gravitational radiation detector: networkPROGENITORSPhysicsgravitational wavesPhysical Sciencesastro-ph.CO[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaMETALLICITYAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)QC1-999gr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsMASSAstrophysics; GravitationGeneral Relativity and Quantum CosmologyBinary black holebinary: coalescenceSYSTEMS0103 physical sciences010306 general physicsSTFCScience & TechnologyGravitational wavegravitational radiationRCUKGravitational Wave Physicsbinary: compactLIGOEVOLUTIONBlack holeNeutron starVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionBLACK-HOLERADIATIONINFERENCE[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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X-ray emission from stellar jets by collision against high-density molecular clouds: an application to HH 248

2015

We investigate the plausibility of detecting X-ray emission from a stellar jet that impacts against a dense molecular cloud. This scenario may be usual for classical T Tauri stars with jets in dense star-forming complexes. We first model the impact of a jet against a dense cloud by 2D axisymmetric hydrodynamic simulations, exploring different configurations of the ambient environment. Then, we compare our results with XMM-Newton observations of the Herbig-Haro object HH 248, where extended X-ray emission aligned with the optical knots is detected at the edge of the nearby IC 434 cloud. Our simulations show that a jet can produce plasma with temperatures up to 10 MK, consistent with producti…

AstrofísicaHERBIGHARO OBJECTSJETS AND OUTFLOWS [ISM]Astrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesCloud computingAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsISM [X-RAYS]Space (mathematics)LuminosityHYDRODYNAMICS//purl.org/becyt/ford/1 [https]INDIVIDUAL OBJECTS (HH 248) [ISM]hydrodynamics Herbig-Haro objects ISM: individual objects: HH 248 ISM: jets and outflows X-rays: ISMAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsJet (fluid)business.industryMolecular cloudAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]PlasmaAstronomíaT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHerbig–Haro objectsbusiness
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Evaporation of Near-Extremal Reissner-Nordström Black Holes

2000

The formation of near-extremal Reissner-Nordstrom black holes in the S-wave approximation can be described, near the event horizon, by an effective solvable model. The corresponding one-loop quantum theory remains solvable and allows to follow analytically the evaporation process which is shown to require an infinite amount of time.

AstrofísicaHigh Energy Physics - TheoryPhysicsEvent horizonMembrane paradigmAstronomyAstronomical PhenomenaEvaporationFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Models TheoreticalFuzzballGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Theory (hep-th)Nonsingular black hole modelsAstronomiaCamps Teoria quàntica deBlack hole thermodynamicsMathematical physicsPhysical Review Letters
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