Search results for "Sound"

showing 10 items of 1845 documents

Longitudinal versus transverse spheroidal vibrational modes of an elastic sphere

2005

Analysis of the spheroidal modes of vibration of a free elastic sphere show that they can be qualitatively grouped into two categories: primarily longitudinal and primarily transverse. This is not a sharp distinction. However, there is a relatively stark contrast between the two kinds of modes. Primarily transverse modes have a small divergence and have frequencies that are almost functionally independent of the longitudinal speed of sound. Analysis of inelastic light scattering intensity from confined acoustic phonons in nanoparticles requires an understanding of this qualitative distinction between different spheroidal modes. In addition, some common misconceptions about spheroidal modes …

PhysicsCondensed Matter - Materials ScienceContinuum mechanicsPhonon[ PHYS.COND.CM-MS ] Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Materials Science (cond-mat.mtrl-sci)FOS: Physical sciences02 engineering and technologyInelastic scattering021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesLight scatteringElectronic Optical and Magnetic MaterialsTransverse planeClassical mechanicsNormal modeSpeed of soundMolecular vibration0103 physical sciences[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]010306 general physics0210 nano-technology
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Sound velocity and dimensional crossover in a superfluid Fermi gas in an optical lattice

2005

We study the sound velocity in cubic and non-cubic three-dimensional optical lattices. We show how the van Hove singularity of the free Fermi gas is smoothened by interactions and eventually vanishes when interactions are strong enough. For non-cubic lattices, we show that the speed of sound (Bogoliubov-Anderson phonon) shows clear signatures of dimensional crossover both in the 1D and 2D limits.

PhysicsCondensed Matter::Quantum GasesOptical latticeCondensed matter physicsPhononCondensed Matter - SuperconductivityCrossoverVan Hove singularityFOS: Physical sciences01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasSuperconductivity (cond-mat.supr-con)SuperfluiditySingularitySpeed of soundQuantum mechanicsCondensed Matter::Superconductivity0103 physical sciencesCondensed Matter::Strongly Correlated Electrons010306 general physicsFermi gas
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Second sound near lambda transition in presence of quantum vortices

2018

In this paper, temperature waves (also known as second sound) are consid- ered, with their respective coupling with waves in the order parameter describing the transition from normal phase to superfluid phase, and with waves in the vortex length density. We analyze the coupling between these three kinds of waves and explore its relevance in situations not far from the lambda transition. In particular, the expres- sions for the second sound speed and second sound attenuation are explicitly obtained within some approximations, showing the influence of the order parameter and the vortex length density, which is decisive close to the transition.

PhysicsCouplingApplied MathematicsGeneral MathematicsAttenuation010102 general mathematicsPhase (waves)Lambda transition01 natural sciences010305 fluids & plasmasVortexSuperfluidityQuantum electrodynamics0103 physical sciencesSecond sound0101 mathematicsQuantumSettore MAT/07 - Fisica MatematicaSecond sound Lambda phase transition Superfluid helium Quantum vortices
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Quasi-classical Physics Within Quantum Criticality in HF Compounds

2014

In this chapter, we explore how the fermion condensation paves the road for quasi-classical physics in HF compounds. This means simply that systems with FC admit partly the quasi-classical description of their thermodynamic and transport properties. This, in turn, simplifies a lot not only of their description but permits to gain more insights both in the puzzling NFL physics of HF compounds and of the physics of FC itself. The quasi-classical physics starts to be applicable near FCQPT, at which FC generates flat bands and quantum criticality, and makes the density of electron states in strongly correlated metals diverge. As we shall see, due to the formation of flat bands the strongly corr…

PhysicsCriticalityCondensed matter physicsChemical physicsQuantum critical pointFermi surfaceFermionElectronZero soundClassical physicsQuantum
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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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Coupling of heat flux and vortex polarization in superfluid helium

2020

We consider a macroscopic description of the mutual influence between heat flux and vortex polarization in superfluid helium, in which the vortices produce a lateral deviation of the heat flux, and the heat flux produces a lateral drift of vortices. This coupling is a consequence of a microscopic Magnus force and mutual friction force between the vortices and the flow of excitations carrying the heat. We keep track of these effects with simplified macroscopic equations, and we apply them to second sound propagation between rotating concentric cylinders and to spatial distribution of polarization across a rectangular channel with vortices polarized orthogonally to the channel in the presence…

PhysicsFriction force010102 general mathematicsStatistical and Nonlinear PhysicsMechanicsPolarization (waves)01 natural sciencesVortexPhysics::Fluid DynamicsHeat fluxCondensed Matter::Superconductivity0103 physical sciencesSecond soundConcentric cylinder010307 mathematical physicsMagnus effect0101 mathematicsMathematical PhysicsSuperfluid helium-4Journal of Mathematical Physics
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Anomalous dynamics triggered by a non-convex equation of state in relativistic flows

2017

The non-monotonicity of the local speed of sound in dense matter at baryon number densities much higher than the nuclear saturation density ($n_0 \approx 0.16\,$fm$^{-3}$) suggests the possible existence of a non-convex thermodynamics which will lead to a non-convex dynamics. Here, we explore the rich and complex dynamics that an equation of state (EoS) with non-convex regions in the pressure-density plane may develop as a result of genuinely relativistic effects, without a classical counterpart. To this end, we have introduced a phenomenological EoS, whose parameters can be restricted heeding to causality and thermodynamic stability constraints. This EoS shall be regarded as a toy-model wi…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsEquation of state (cosmology)Plane (geometry)Nuclear TheoryFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesAstronomy and AstrophysicsPhysics - Fluid DynamicsApprox01 natural sciencesCausality (physics)Complex dynamicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSpeed of sound0103 physical sciencesBaryon numberAstrophysics - High Energy Astrophysical PhenomenaRelativistic quantum chemistry010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Mathematical physics
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The termination region of high-mass microquasar jets

2011

The environment of high-mass X-ray binaries can be characterized either by the SNR that forms these systems, or by the wind from the companion massive star. These regions should be tenuous but very hot, and surrounded by a dense and cold shocked ISM shell. The interaction between the jet and such a complex medium, also affected by the system proper motion, can lead to very different jet termination structures. The evolution of the jet termination regions during the life of a high-mass microquasar is simulated to improve the present understanding of these structures. Also, the evolving emission characteristics are modeled to inform potential observational campaigns for this class of object. …

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)Proper motionShock (fluid dynamics)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsThrustAstrophysics01 natural sciencesWavelength13. Climate actionSpace and Planetary ScienceSpeed of sound0103 physical sciencesPeculiar velocityEjectaAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics
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LiquidHe4andHe3at negative pressure

1992

The critical pressures {ital P}{sub {ital c}} at which liquid {sup 4}He and {sup 3}He each become macroscopically unstable are determined from two kinds of microscopic calculations that reproduce the equation of state. The behavior of the sound velocity {ital c} around this critical pressure is analyzed, and the critical exponent in {ital c}{proportional to}({ital P}{minus}{ital P}{sub {ital c}}){sup {nu}} is found to be {nu}=1/4. A comparison with empirical analysis is also done.

PhysicsLight nucleusEquation of stateLiquid stateHelium-4Helium-3Analytical chemistryThermodynamicsIsotopes of heliumCritical exponentSound wavePhysical Review B
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Attenuation of the fourth sound in liquid helium II via extended thermodynamics

2004

Abstract This work continues a study begun in previous works, where a non-standard model of liquid helium II is proposed, in which a small entropy transfer is associated with the superfluid component. In this work the influence of this superfluid entropy on the propagation of the fourth sound is analyzed. From experimental data for velocities and attenuations of the first and second sound, the model provides speed and attenuation coefficient of the fourth sound in a porous medium as a function of the ratio ss/s between the superfluid entropy ss and the total entropy s. These values are determined in the two limiting cases ss/s=0 and =0.02, for various values of temperature and pressure.

PhysicsLiquid heliumApplied MathematicsMechanical EngineeringAttenuationNon-equilibrium thermodynamicsThermodynamicslaw.inventionSuperfluidityEntropy (classical thermodynamics)Mechanics of MaterialslawAttenuation coefficientSecond soundPorous mediumInternational Journal of Non-Linear Mechanics
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