Search results for "Superfluidity"

showing 10 items of 110 documents

Quasiparticles, coherence and nonlinearity: exact simulations of RF-spectroscopy of strongly interacting one-dimensional Fermi gases

2008

We consider RF-spectroscopy of ultracold Fermi gases by exact simulations of the many-body state and the coherent dynamics in one dimension. Deviations from the linear response sum rule result are found to suppress the pairing contribution to the RF line shifts. We compare the coherent rotation and quasiparticle descriptions of RF-spectroscopy which are analogous to NMR experiments in superfluid $^3$He and tunneling in solids, respectively. We suggest that RF-spectroscopy in ultracold gases provides an interesting crossover between these descriptions that could be used for studying decoherence in quantum measurement, in the context of many-body quantum states.

PhysicsCondensed Matter::Quantum GasesQuantum decoherenceCondensed matter physicsCondensed Matter - SuperconductivityFOS: Physical sciencesAtomic and Molecular Physics and OpticsSuperfluiditySuperconductivity (cond-mat.supr-con)Condensed Matter - Other Condensed MatterQuantum statePairingQuantum mechanicsQuasiparticleSum rule in quantum mechanicsSpectroscopyCoherence (physics)Other Condensed Matter (cond-mat.other)
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The growth of atomically rough 4He crystals

1986

We have studied the growth of atomically rough bcc and hcp4He crystals from the superfluid phase for temperaturesT>0.9 K. The growth coefficient displays a temperature dependence which can be represented bym 4 K∝ $$e^{\Delta E/k_B T} $$ . The parameter ΔE is found to be in close agreement with the energy gap of rotons, suggesting that these thermal excitations dominate the growth kinetics. Besides, the absolute value of the growth coefficient depends on crystal orientation, with an anisotropy for the hcp phase of about a factor of 2.5 between the $$\left\{ {10\bar 10} \right\}$$ and {0001} planes.

PhysicsCondensed matter physicsBand gapCondensed Matter::OtherThermodynamicsAbsolute valueCrystal growthCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsSuperfluidityHelium-4Phase (matter)General Materials Scienceddc:530AnisotropyBar (unit)
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Nonlocal effects in superfluid turbulence: Application to the low-density- to high-density-state transition and to vortex decay

2005

We discuss a phenomenological equation for the evolution of vortex tangle in counterflow superfluid turbulence, which takes into account the influence of the nonlocal effects, introducing into the original equation of Vinen two simple corrective terms dependent on a nonvanishing ratio between the average separation between vortex lines and the diameter of the channel. The equation allows one to describe, in relatively good agreement with experimental results, the two turbulent regimes present in counterflow superfluid turbulence and the transition between them. The decay rate of the vortex line density L, when the heat flux is suddenly turned off, is also investigated; due to the simplicity…

PhysicsCondensed matter physicsCondensed Matter::OtherTurbulenceQuantum vortexCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsVortexSuperfluidityHelium-4Heat fluxQuantum electrodynamicsPhenomenological modelIsotopes of heliumPhysical Review B
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Spin-S Kagome quantum antiferromagnets in a field with tensor networks

2016

Spin-$S$ Heisenberg quantum antiferromagnets on the Kagome lattice offer, when placed in a magnetic field, a fantastic playground to observe exotic phases of matter with (magnetic analogs of) superfluid, charge, bond or nematic orders, or a coexistence of several of the latter. In this context, we have obtained the (zero temperature) phase diagrams up to $S=2$ directly in the thermodynamic limit thanks to infinite Projected Entangled Pair States (iPEPS), a tensor network numerical tool. We find incompressible phases characterized by a magnetization plateau vs field and stabilized by spontaneous breaking of point group or lattice translation symmetry(ies). The nature of such phases may be se…

PhysicsCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Semiclassical physicsFOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural sciences3. Good healthSuperfluidityMagnetizationCondensed Matter - Strongly Correlated ElectronsQuantum mechanics0103 physical sciencesThermodynamic limitCondensed Matter::Strongly Correlated ElectronsSymmetry breakingQuantum spin liquid[PHYS.COND.CM-SCE]Physics [physics]/Condensed Matter [cond-mat]/Strongly Correlated Electrons [cond-mat.str-el]010306 general physics0210 nano-technologyTranslational symmetryComputingMilieux_MISCELLANEOUSPhase diagram
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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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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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