Search results for "superfluid"

showing 10 items of 171 documents

Contribution of the normal component to the thermal resistance of turbulent liquid helium

2015

Previous results for the velocity profile of the normal component of helium II in counterflow are used to evaluate the viscous contribution to the effective thermal resistance. It turns out that such a contribution becomes considerably higher than the usual Landau estimate, because in the presence of vortices, the velocity profile is appreciably different from the Poiseuille parabolic profile. Thus, a marked increase in the contribution of the normal component to the thermal resistance with respect to the viscous Landau estimate does not necessarily imply that the normal component is turbulent. Furthermore, we examine the influence of a possible slip flow along the walls when the radius of …

PhysicsCondensed matter physicsTurbulenceApplied MathematicsGeneral MathematicsThermal resistanceQuantum turbulenceGeneral Physics and AstronomyRadiusHagen–Poiseuille equationVortexPhysics::Fluid DynamicsThermal resistance – Superfluid helium – Quantum turbulence – Normal componentBoundary value problemSettore MAT/07 - Fisica MatematicaSuperfluid helium-4Zeitschrift für angewandte Mathematik und Physik
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Vortex mutual friction in rotating superfluid 3He

1996

The Manchester rotating cryostat has been used to measure the longitudinal and transverse coefficients of vortex mutual friction in the A and B phases of superfluid 3He. In the B phase the dominant contribution to the mutual friction is scattering of excitations off occupied bound states in the vortex core. The A phase results are explained quantitatively by assuming that doubly quantised continuous vortices are created with a dynamics determined by the equation of motion of the orbital vector I; the measurements enable us to put an upper limit on the orbital inertia of less than 0.01h{stroke} per Cooper pair. History-dependent textural effects which had to be overcome in order to make mean…

PhysicsCondensed matter physicsmedia_common.quotation_subjectPhase (waves)General Physics and AstronomyEquations of motionInertiaRotationVortexSuperfluidityClassical mechanicsBound stateCooper pairmedia_common
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Sub-MeV dark matter and the Goldstone modes of superfluid helium

2019

We show how the relativistic effective field theory for the superfluid phase of helium-4 can replace the standard methods used to compute the production rates of low momentum excitations due to the interaction with an external probe. This is done by studying the scattering problem of a light dark matter particle in the superfluid, and comparing to some existing results. We show that the rate of emission of two phonons, the Goldstone modes of the effective theory, gets strongly suppressed for sub-MeV dark matter particles due to a fine cancellation between two different tree-level diagrams in the limit of small exchanged momenta. This phenomenon is found to be a consequence of the particular…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhononDark matterFOS: Physical sciencesdark matter detection01 natural sciencesHigh Energy Physics - ExperimentSuperfluidityMomentumHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)effective quantum field theoriesHigh Energy Physics - Phenomenology (hep-ph)Orders of magnitude (time)dark matter detection; effective quantum field theoriesQuantum electrodynamics0103 physical sciencesEffective field theory010306 general physicsLight dark matterSuperfluid helium-4Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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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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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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Non-equilibrium thermodynamics analysis of rotating counterflow superfluid turbulence

2010

In two previous papers two evolution equations for the vortex line density $L$, proposed by Vinen, were generalized to rotating superfluid turbulence and compared with each other. Here, the already generalized alternative Vinen equation is extended to the case in which counterflow and rotation are not collinear. Then, the obtained equation is considered from the viewpoint of non-equilibrium thermodynamics. According with this formalism, the compatibility between this evolution equation for $L$ and that one for the velocity of the superfluid component is studied. The compatibility condition requires the presence of a new term dependent on the anisotropy of the tangle, which indicates how the…

PhysicsFriction forceTurbulenceCondensed Matter::OtherNon-equilibrium thermodynamicsFOS: Physical sciencessuperfluid turbulence Onsager-Casimir reciprocity relation rotating counterflow turbulenceVortexComputer Science ApplicationsSuperfluidityCondensed Matter - Other Condensed MatterFormalism (philosophy of mathematics)Classical mechanicsModeling and SimulationModelling and SimulationEvolution equationAnisotropySettore MAT/07 - Fisica MatematicaOther Condensed Matter (cond-mat.other)
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Coherent magneto-elastic oscillations in superfluid magnetars

2016

We study the effect of superfluidity on torsional oscillations of highly magnetised neutron stars (magnetars) with a microphysical equation of state by means of two-dimensional, magnetohydrodynamical- elastic simulations. The superfluid properties of the neutrons in the neutron star core are treated in a parametric way in which we effectively decouple part of the core matter from the oscillations. Our simulations confirm the existence of two groups of oscillations, namely continuum oscillations that are confined to the neutron star core and are of Alfv\'enic character, and global oscillations with constant phase and that are of mixed magneto-elastic type. The latter might explain the quasi-…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Magnetar01 natural sciencesAsteroseismologyGeneral Relativity and Quantum CosmologyMagnetic fieldSuperfluidityNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceNormal modeQuantum electrodynamics0103 physical sciencesNeutronMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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Constraining properties of high-density matter in neutron stars with magneto-elastic oscillations

2017

We discuss torsional oscillations of highly magnetised neutron stars (magnetars) using two-dimensional, magneto-elastic-hydrodynamical simulations. Our model is able to explain both the low- and high-frequency quasi-periodic oscillations (QPOs) observed in magnetars. The analysis of these oscillations provides constraints on the breakout magnetic-field strength, on the fundamental QPO frequency, and on the frequency of a particularly excited overtone. More importantly, we show how to use this information to generically constraint properties of high-density matter in neutron stars, employing Bayesian analysis. In spite of current uncertainties and computational approximations, our model-depe…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Equation of state (cosmology)OvertoneAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsMagnetar01 natural sciencesSuperfluidityNuclear physicsNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceExcited state0103 physical sciencesMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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On quantum effects near the liquid-vapor transition in helium

2001

The liquid-vapor transition in He-3 and He-4 is investigated by means of path-integral molecular dynamics and the quantum virial expansion. Both methods are applied to the critical isobar and the critical isochore. While previous path-integral simulations have mainly considered the lambda transition and superfluid regime in He-4, we focus on the vicinity of the critical point and obtain good agreement with experimental results for the molar volume and the internal energy down to subcritical temperatures. We find that an effective classical potential that properly describes the two-particle radial distribution function exhibits a strong temperature dependence near the critical temperature. T…

PhysicsInternal energyCondensed matter physicsStatistical Mechanics (cond-mat.stat-mech)Lambda transitionGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesCondensed Matter - Soft Condensed MatterRadial distribution functionSuperfluidityMolecular dynamicschemistryCritical point (thermodynamics)Virial expansionSoft Condensed Matter (cond-mat.soft)Physical and Theoretical ChemistryCondensed Matter - Statistical MechanicsHelium
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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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