Search results for "Fluids"

showing 10 items of 1936 documents

A status report of the multipurpose superconducting electron cyclotron resonance ion source

2007

Intense heavy ion beam production with electron cyclotron resonance (ECR) ion sources is a common requirement for many of the accelerators under construction in Europe and elsewhere. An average increase of about one order of magnitude per decade in the performance of ECR ion sources was obtained up to now since the time of pioneering experiment of R. Geller at CEA, Grenoble, and this trend is not deemed to get the saturation at least in the next decade, according to the increased availability of powerful magnets and microwave generators. Electron density above 1013 cm(-3) and very high current of multiply charged ions are expected with the use of 28 GHz microwave heating and of an adequate …

PhysicsElectron density[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Cyclotron resonanceParticle accelerator01 natural sciences7. Clean energyIon sourceElectron cyclotron resonanceCharged particle010305 fluids & plasmaslaw.inventionIon29.25.NiIon sources: positive and negativelaw0103 physical sciencesAtomic physics010306 general physicsInstrumentationMicrowave
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Energy-loss straggling of 2-10 MeV/u Kr ions in gases

2013

Measurements have been performed on a time-of-flight setup at the Jyväskylä K130 cyclotron, aiming at energy-loss straggling of heavy ions in gases. Theoretical predictions based on recently developed theory as well as an empirical interpolation formula predict that straggling can be more than ten times higher than Bohr straggling in the MeV/u regime. Our measurements with up to 9.3 MeV/u Kr ions on He, N2, Ne and Kr targets confirm this feature. Our calculations show the relative contributions of linear straggling, bunching including packing, and charge exchange. Our results for stopping cross sections are compatible with values from the literature. Funding Agencies|EU||Academy of Finland …

PhysicsEnergy lossCyclotronPhysics::Medical Physics7. Clean energy01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmaslaw.inventionIonBohr modelNuclear physicssymbols.namesakelawAtomic and Molecular CollisionsTeknik och teknologier0103 physical sciencessymbolsEngineering and TechnologyAtomic physics010306 general physicsAtomien ja molekyylien törmäyksetCharge exchange
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Beyond the Vegard's law: solid mixing excess volume and thermodynamic potentials prediction, from end-members

2020

Abstract A method has been developed, herein presented, to model binary solid solutions' volume, enthalpy and Gibbs energy using the energy state functions, E ( V , S ) , of the end-members only. The E ( V , S ) s are expanded around an unknown mixing volume, V Mix , and the fundamental equilibrium equation − ( ∂ E / ∂ V ) S = P is used to determine V Mix . V Mix allows us to model enthalpy, straightforwardly. The same argument holds using Helmholtz energy, F ( V , T ) , in place of E ( V , S ) , and the equilibrium equation becomes − ( ∂ F / ∂ V ) T = P . One can readily determine the Gibbs free energy, too. The method presented remarkably simplifies computing of solid mixings' thermodynam…

PhysicsEnthalpyGeneral Physics and AstronomyThermodynamicsComputer simulation01 natural sciences010305 fluids & plasmasThermodynamic potentialGibbs free energysymbols.namesakeVolume (thermodynamics)Vegard's lawNitride materialHelmholtz free energy0103 physical sciencessymbols010306 general physicsMetals and alloyThermodynamic modelingMixing (physics)Solid solution
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Quantum Monte Carlo methods

2005

Introduction In most of the discussion presented so far in this book, the quantum character of atoms and electrons has been ignored. The Ising spin models have been an exception, but since the Ising Hamiltonian is diagonal (in the absence of a transverse magnetic field), all energy eigenvalues are known and the Monte Carlo sampling can be carried out just as in the case of classical statistical mechanics. Furthermore, the physical properties are in accord with the third law of thermodynamics for Ising-type Hamiltonians (e.g. entropy S and specific heat vanish for temperature T → 0, etc.) in contrast to the other truly classical models dealt with in previous chapters (e.g. classical Heisenbe…

PhysicsEntropy (statistical thermodynamics)Quantum Monte CarloMonte Carlo methodZero-point energyClassical fluidsStatistical mechanicsHybrid Monte Carlosymbols.namesakeQuantum mechanicsDynamic Monte Carlo methodsymbolsMonte Carlo method in statistical physicsIsing modelKinetic Monte CarloStatistical physicsQuasi-Monte Carlo methodHamiltonian (quantum mechanics)Monte Carlo molecular modelingSpin-½
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A density functional for liquid3He

1993

We present a density functional for the description of liquid3He properties at zero temperature in a mean field approximation. Its basic ingredients are a zero-range, particle- and spin-density dependent effective interaction of Skyrme type, and a long-range effective interaction of Lennard-Jones type supplemented with a weighted density approximation similar to the one used in the study of classical fluids, to phenomenologically account for short range correlations. After fixing the value of its parameters, the functional yields a good description of the equation of state and Landau parameters (spin symmetric and spin antisymmetric as well) from saturation to solidification densities. The …

PhysicsEquation of stateCondensed matter physicsMean field theoryAntisymmetric relationQuantum mechanicsDrop (liquid)PairingMomentum transferClassical fluidsZero soundAtomic and Molecular Physics and OpticsZeitschrift f�r Physik D: Atoms, Molecules and Clusters
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A generalization of the Carnahan–Starling approach with applications to four- and five-dimensional hard spheres

2018

Abstract Development of good equations of state for hard spheres is an important task in the study of real fluids. In a way consistent with other theoretical results, we generalize the famous Carnahan–Starling approach for arbitrary dimensions and apply it to four- and five-dimensional hard spheres. We obtain simple and integer representations for virial coefficients of lower orders and accurate equations of state. Since theoretically and practically validated, these results improve understanding of hard sphere fluids.

PhysicsEquation of stateGeneralizationGeneral Physics and AstronomyHard spheres01 natural sciences010305 fluids & plasmasVirial coefficientSimple (abstract algebra)0103 physical sciencesDevelopment (differential geometry)Statistical physics010306 general physicsInteger (computer science)Physics Letters A
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The screened cluster equation of state for hydrogen-helium mixtures: Atomic, molecular, and ionic contributions from first principles

2018

International audience

PhysicsEquation of stateHydrogenIonic bondingThermodynamicschemistry.chemical_elementCondensed Matter Physics01 natural sciences010305 fluids & plasmasVirial coefficientchemistry0103 physical sciencesBound stateCluster (physics)010306 general physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HeliumComputingMilieux_MISCELLANEOUS
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On the Measurements of Numerical Viscosity and Resistivity in Eulerian MHD Codes

2016

We propose a simple ansatz for estimating the value of the numerical resistivity and the numerical viscosity of any Eulerian MHD code. We test this ansatz with the help of simulations of the propagation of (magneto)sonic waves, Alfven waves, and the tearing mode instability using the MHD code Aenus. By comparing the simu- lation results with analytical solutions of the resistive-viscous MHD equations and an empirical ansatz for the growth rate of tearing modes we measure the numerical viscosity and resistivity of Aenus. The comparison shows that the fast-magnetosonic speed and wavelength are the characteristic velocity and length, respectively, of the aforementioned (relatively simple) syst…

PhysicsFOS: Physical sciencesAstronomy and AstrophysicsEulerian pathMechanicsCharacteristic velocity01 natural sciencesNumerical resistivityRiemann solver010305 fluids & plasmassymbols.namesakeViscosityAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetorotational instability0103 physical sciencessymbolsMagnetohydrodynamicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)AnsatzThe Astrophysical Journal Supplement Series
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Influence of electromagnetic boundary conditions onto the onset of dynamo action in laboratory experiments

2009

We study the onset of dynamo action of the Riga and Karlsruhe experiments with the addition of an external wall, the electro-magnetic properties of which being different from those of the fluid in motion. We consider a wall of different thickness, conductivity and permeability. We also consider the case of a ferro-fluid in motion.

PhysicsFerrofluid[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Mechanics of the fluids [physics.class-ph][SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]Fluid Dynamics (physics.flu-dyn)FOS: Physical sciences[PHYS.PHYS.PHYS-GEO-PH]Physics [physics]/Physics [physics]/Geophysics [physics.geo-ph]Physics - Fluid DynamicsConductivity01 natural sciences010305 fluids & plasmas[SPI.MECA.MEFL]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph]Physics::GeophysicsGeophysics (physics.geo-ph)Physics - GeophysicsPhysics::Fluid DynamicsClassical mechanicsPermeability (electromagnetism)0103 physical sciencesBoundary value problem[PHYS.MECA.MEFL]Physics [physics]/Mechanics [physics]/Fluid mechanics [physics.class-ph]010306 general physicsDynamo
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Modeling vibrating panels excited by a non-homogeneous turbulent boundary layer

2021

Abstract Predicting the vibration response of an elastic structure excited by a turbulent flow is of interest for the civil and military transportation sector. The models proposed in the literature are generally based on the assumption that the turbulent boundary layer (noted TBL in the following) exciting the structure is spatially homogeneous. However, this assumption is not always fulfilled in practice, in particular when the excited area is close to the starting point of the TBL or with curved structures. To overcome this issue, this work proposes to extend two approaches generally used for dealing with homogeneous TBL, namely the spatial and the wavenumber approaches. The extension of …

PhysicsField (physics)Basis (linear algebra)TurbulenceMechanical EngineeringComputationMathematical analysisFunction (mathematics)01 natural sciences[PHYS.MECA.ACOU]Physics [physics]/Mechanics [physics]/Acoustics [physics.class-ph]010305 fluids & plasmasWavelengthBoundary layer0103 physical sciencesWavenumber010301 acousticsComputingMilieux_MISCELLANEOUSJournal of Fluids and Structures
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