Search results for "Fluid Dynamic"

showing 10 items of 1034 documents

Monoclinic model shear zones

1998

Abstract Although many ductile shear zones are supposed to have developed by approximately simple shear flow, some must have formed under different conditions. A few types of such ‘non-simple shear zones’ have been proposed in the literature such as transpression-, transtension- and stretching-shear zones. This paper presents a full three-dimensional kinematic model of shear zones with monoclinic flow geometry. Monoclinic shear zone types can be classified according to flow parameters, and according to the geometry and orientation of accumulating finite strain. Modelling of finite strain accumulation shows that a number of unusual and potentially problematic structural features may develop …

GeologyGeometryCondensed Matter::Soft Condensed MatterPhysics::Fluid DynamicsShear modulusSimple shearShear rateCondensed Matter::Materials ScienceShear (geology)Critical resolved shear stressShear stressGeotechnical engineeringAstrophysics::Earth and Planetary AstrophysicsShear velocityShear zoneGeologyJournal of Structural Geology
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The formation of large quartz veins by rapid ascent of fluids in mobile hydrofractures

2001

Abstract This paper aims to resolve two main problems related to the formation of quartz veins: (1) the predominance of quartz veins at shallow crustal levels and not deeper in the crust, close to the source of metamorphic fluids where the temperature sensitivity of quartz solubility is much higher than at lower, upper-crustal temperatures and (2) the formation of very large 100–1000 m scale quartz veins that would require huge amounts of fluid flow in current models of vein formation. It is proposed here that these problems are resolved by the recognition of very fast (m/s) mobile hydrofracture ascent of batches of fluid. Mobile hydrofractures are fluid-filled fractures that propagate at t…

GeophysicsMetamorphic rockFracture (geology)Fluid dynamicsMineralogyCrustCurrent (fluid)Vein (geology)PetrologyQuartzGeologyEarth-Surface ProcessesWall rockTectonophysics
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Effect of pH on the mobility of the herbicide MCPA in a sand-goethite column: 1D and 2D reactive transport modeling

2018

Abstract Adsorption and transport of the herbicide 2-methyl-4-chlorophenoxyacetic acid (MCPA) in a homogeneous sand-goethite system were investigated as a function of pH. Interaction of MCPA with the solid surface was geochemically modeled according to the charge distribution multisite complexation (CD-MUSIC) approach. Based on this calibration, retardation of MCPA transport in column experiments was significantly underestimated by conventional 1D simulations. As a new approach, Positron Emission Tomography (PET) was employed to analyze the flow field, using 18F− as a radiotracer. The observed heterogeneity was reproduced in 2D simulations assuming increased permeability and porosity at the…

GoethiteFlow (psychology)ThermodynamicsCharge density010501 environmental sciences010502 geochemistry & geophysics01 natural sciencesPollutionMCPAPermeability (earth sciences)chemistry.chemical_compoundAdsorptionchemistryGeochemistry and Petrologyvisual_artvisual_art.visual_art_mediumFluid dynamicsEnvironmental ChemistryPorosity0105 earth and related environmental sciencesApplied Geochemistry
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Group analysis and similarity solutions of the compressible boundary layer equations

1989

In this paper the application of Lie's methods to the equations of the laminar boundary layer is discussed. The momentum and energy equations in Prandtl's form are considered for a steady, viscous, compressible laminar flow with non zero pressure gradient, variable viscosity and thermal conductivity. Group analysis yields similarity solutions for given pressure distributions and particular values of the invariance group parameters (group classification). Crocco's transformation is obtained for the infinite-dimensional group of the Lie's algebra admitted by the equations.

Group (mathematics)Mechanical EngineeringMathematical analysisPrandtl numberLie groupLaminar flowCondensed Matter PhysicsBoundary layer thicknessSimilarity solutionPhysics::Fluid Dynamicssymbols.namesakeBoundary layerMechanics of MaterialsBlasius boundary layersymbolsMathematicsMeccanica
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Numerical simulation of transcatheter mitral valve replacement: The dynamic implication of LVOT obstruction in the valve-in-ring case.

2022

Transcatheter mitral valve replacement (TMVR) has been used for “off-label” treatment when annuloplasty band ring for mitral repair fails. However, the complex anatomy and function of the mitral valve may lead to fatal complications as a result of the left ventricular outflow tract (LVOT) obstruction in TMVR. We report the structural and hemodynamic response of LVOT obstruction resulting from TMVR with the Edwards SAPIEN 3 Ultra (S3) device. We modified the original Living Heart Human Model (LHHM) to account for a failed mitral valve with an annuloplasty band ring and simulated the cardiac beating condition in the setting of S3 device implantation. Findings demonstrated a high dynamic behav…

Heart Valve Prosthesis ImplantationHeart Defects CongenitalHistoryCardiac CatheterizationPolymers and PlasticsRehabilitationBiomedical EngineeringBiophysicsMitral Valve InsufficiencyFinite Element (FE) analysisIndustrial and Manufacturing EngineeringVentricular Outflow ObstructionTreatment OutcomeRisk FactorsComputational Fluid Dynamic (CFD)Living heart human modelHeart Valve ProsthesisHumansMitral ValveOrthopedics and Sports MedicineBusiness and International ManagementTranscatheter mitral valve replacementJournal of biomechanics
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Constant circulation sequences of binary neutron stars and their spin characterization

2018

For isentropic fluids, dynamical evolution of a binary system conserves the baryonic mass and circulation; therefore, sequences of constant rest mass and constant circulation are of particular importance. In this work, we present the extension of our Compact Object CALculator (\cocal{}) code to compute such quasiequilibria and compare them with the well-known corotating and irrotational sequences, the latter being the simplest, zero-circulation case. The circulation as a measure of the spin for a neutron star in a binary system has the advantage of being exactly calculable since it is a local quantity. To assess the different measures of spin, such as the angular velocity of the star, the q…

High Energy Astrophysical Phenomena (astro-ph.HE)AstrofísicaPhysics010308 nuclear & particles physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Compact starConservative vector field01 natural sciencesGeneral Relativity and Quantum CosmologyNeutron starCirculation (fluid dynamics)0103 physical sciencesAstronomiaBinary systemConstant (mathematics)Astrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsMathematical physicsDimensionless quantitySpin-½
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Using evolutionary algorithms to model relativistic jets

2019

High-resolution Very-Long-Baseline Interferometry observations of NGC 1052 show a two sided jet with several regions of enhanced emission and a clear emission gap between the two jets.This gap shrinks with increasing frequency and vanishes around $\nu\sim43$ GHz. The observed structures are due to both the macroscopic fluid dynamics interacting with the surrounding ambient medium including an obscuring torus and the radiation microphysics. In this paper we investigate the possible physical conditions in relativistic jets of NGC 1052 by directly modelling the observed emission and spectra via state-of-the-art special-relativistic hydrodynamic (SRHD) simulations and radiative transfer calcula…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010504 meteorology & atmospheric sciencesMicrophysicsComputer Science::Information RetrievalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)TorusAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencesAstrophysical jetSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesVery-long-baseline interferometryRadiative transferFluid dynamicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics0105 earth and related environmental sciencesAstronomy & Astrophysics
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Dynamical efficiency of collisionless magnetized shocks in relativistic jets

2010

The so-called internal shock model aims to explain the light-curves and spectra produced by non-thermal processes originated in the flow of blazars and gamma-ray bursts. A long standing question is whether the tenuous collisionless shocks, driven inside a relativistic flow, are efficient enough to explain the amount of energy observed as compared with the expected kinetic power of the outflow. In this work we study the dynamic efficiency of conversion of kinetic-to- thermal/magnetic energy of internal shocks in relativistic magnetized outflows. We find that the collision between shells with a non-zero relative velocity can yield either two oppositely moving shocks (in the frame where the co…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsShock waveShock (fluid dynamics)Magnetic energyAstrophysics::High Energy Astrophysical PhenomenaRelative velocityFOS: Physical sciencesRarefaction020206 networking & telecommunications02 engineering and technologyKinetic energyComputational physicsAstrophysical jet0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingAstrophysics - High Energy Astrophysical PhenomenaBlazarAstrophysics::Galaxy AstrophysicsAIP Conference Proceedings
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Periodic massloss from viscous accretion flows around black holes

2014

We investigate the behaviour of low angular momentum viscous accretion flows around black holes using Smooth Particle Hydrodynamics (SPH) method. Earlier, it has been observed that in a significant part of the energy and angular momentum parameter space, rotating transonic accretion flow undergoes shock transition before entering in to the black hole and a part of the post-shock matter is ejected as bipolar outflows, which are supposed to be the precursor of relativistic jets. In this work, we simulate accretion flows having injection parameters from the inviscid shock parameter space, and study the response of viscosity on them. With the increase of viscosity, shock becomes time dependent …

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsAngular momentumShock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsMechanicsAccretion (astrophysics)Physics::Fluid DynamicsSmoothed-particle hydrodynamicsViscosityAstrophysical jetSpace and Planetary ScienceInviscid flowAstrophysics::Solar and Stellar AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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QUANTUM EFFECTS IN ACOUSTIC BLACK HOLES: THE BACKREACTION.

2004

We investigate the backreaction equations for an acoustic black hole formed in a Laval nozzle under the assumption that the motion of the fluid is one-dimensional. The solution in the near-horizon region shows that as phonons are (thermally) radiated the sonic horizon shrinks and the temperature decreases. This contrasts with the behaviour of Schwarzschild black holes, and is similar to what happens in the evaporation of (near-extremal) Reissner-Nordstrom black holes (i.e. infinite evaporation time). Finally, by appropriate boundary conditions the solution is extended in both the asymptotic regions of the nozzle.

High Energy Physics - TheoryNuclear and High Energy PhysicsSonic black holeEvent horizonWhite holeAstrophysics::High Energy Astrophysical PhenomenaHAWKINGFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black holeGeneral Relativity and Quantum CosmologyACOUSTICPhysics::Fluid DynamicsMicro black holeGeneral Relativity and Quantum CosmologyQuantum mechanicsPhysicsBLACK HOLEBACK REACTIONFLUIDCondensed Matter - Other Condensed MatterBlack holeHigh Energy Physics - Theory (hep-th)RADIATIONSchwarzschild radiusOther Condensed Matter (cond-mat.other)Hawking radiation
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