Search results for "superfluid"

showing 10 items of 171 documents

Quantum field theory of dilute homogeneous Bose-Fermi mixtures at zero temperature: General formalism and beyond mean-field corrections

2002

We consider a dilute homogeneous mixture of bosons and spin-polarized fermions at zero temperature. We first construct the formal scheme for carrying out systematic perturbation theory in terms of single particle Green's functions. We introduce a new relevant object, the renormalized boson-fermion T-matrix which we determine to second order in the boson-fermion s-wave scattering length. We also discuss how to incorporate the usual boson-boson T-matrix in mean-field approximation to obtain the total ground state properties of the system. The next order term beyond mean-field stems from the boson-fermion interaction and is proportional to $a_{\scriptsize BF}k_{\scriptsize F}$. The total groun…

Einstein condensationDegeneracyHigh Energy Physics::LatticeCondensed Matter (cond-mat)FOS: Physical sciencesHE-3-HE-4 mixturesCondensed MatterKinetic energylaw.inventionlawQuantum mechanicsQuantum field theoryBosonPhysicsCondensed Matter::Quantum GasesInstitut für Physik und AstronomieScattering lengthInteraction energyFermionCollisions.Atomic and Molecular Physics and OpticsAtomic gasMean field theorySuperfluidityQuantum electrodynamicsBose–Einstein condensate
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K-ϵ-L model in turbulent superfluid helium

2020

We generalize the K−ϵ model of classical turbulence to superfluid helium. In a classical viscous fluid the phenomenological eddy viscosity characterizing the effects of turbulence depends on the turbulent kinetic energy K and the dissipation function ϵ, which are mainly related to the fluctuations of the velocity field and of its gradient. In superfluid helium, instead, we consider the necessary coefficients for describing the effects of classical and quantum turbulence, involving fluctuations of the velocity, the heat flux, and the vortex line density of the quantized vortex lines. By splitting the several fields into a time-average part and a fluctuating part, some expressions involving t…

Energy cascadeNon-equilibrium thermodynamicHeat transferQuantized vorticeSuperfluid heliumK−ϵ modelQuantum turbulenceSettore MAT/07 - Fisica Matematica
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Effective thermal conductivity of superfluid helium in short channels

2014

The aim of this paper is to explore how the effective thermal conductivity of small channels filled with superfluid helium II in the laminar regime separates from the classical Landau expression as the channel becomes shorter. The Landau expression is valid for fully developed Poiseuille flow for the normal component, and therefore is suitable for long channels. By taking into account entrance effects, we show a transition from a heat flux proportional to ∆T /l (Landau regime) for long channels, to a heat flux proportional to l^(1/3) (∆T /l)^(2/3) for short channels.

Entrance lengthEffective thermal conductivitySuperfluid heliumSettore MAT/07 - Fisica MatematicaPoiseuille flow
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Strongly interacting Fermi gases with density imbalance

2005

We consider density-imbalanced Fermi gases of atoms in the strongly interacting, i.e. unitarity, regime. The Bogoliubov-deGennes equations for a trapped superfluid are solved. They take into account the finite size of the system, as well as give rise to both phase separation and FFLO type oscillations in the order parameter. We show how radio-frequency spectroscopy reflects the phase separation, and can provide direct evidence of the FFLO-type oscillations via observing the nodes of the order parameter.

FOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesElectromagnetic radiation010305 fluids & plasmasSuperconductivity (cond-mat.supr-con)SuperfluidityCondensed Matter - Strongly Correlated ElectronsCondensed Matter::Superconductivity0103 physical sciences010306 general physicsSpectroscopyPhysicsCondensed Matter::Quantum GasesStrongly Correlated Electrons (cond-mat.str-el)UnitarityCondensed matter physicsCondensed Matter::OtherCondensed Matter - SuperconductivityFermionCondensed Matter - Other Condensed MatterQuantum electrodynamicsFermi gasOther Condensed Matter (cond-mat.other)Dimensionless quantityFermi Gamma-ray Space Telescope
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Pairing gap and in-gap excitations in trapped fermionic superfluids

2004

We consider trapped atomic Fermi gases with Feshbach-resonance enhanced interactions in pseudogap and superfluid temperatures. We calculate the spectrum of RF(or laser)-excitations for transitions that transfer atoms out of the superfluid state. The spectrum displays the pairing gap and also the contribution of unpaired atoms, i.e. in-gap excitations. The results support the conclusion that a superfluid, where pairing is a many-body effect, was observed in recent experiments on RF spectroscopy of the pairing gap.

FOS: Physical sciencesRoton01 natural sciences010305 fluids & plasmasSuperfluiditySuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsSuperfluid state0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Physics::Atomic Physics010306 general physicsFeshbach resonanceSpectroscopyCondensed Matter - Statistical MechanicsPhysicsCondensed Matter::Quantum GasesQuantum PhysicsMultidisciplinaryCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsStatistical Mechanics (cond-mat.stat-mech)Strongly Correlated Electrons (cond-mat.str-el)Condensed Matter::OtherCondensed Matter - SuperconductivityPairingPseudogapQuantum Physics (quant-ph)Fermi Gamma-ray Space Telescope
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Supercurrent Induced Charge-Spin Conversion in Spin-Split Superconductors

2017

We study spin-polarized quasiparticle transport in a mesoscopic superconductor with a spin- splitting field in the presence of co-flowing supercurrent. In such a system, the nonequilibrium state is characterized by charge, spin, energy and spin energy modes. Here we show that in the presence of both spin splitting and supercurrent, all these modes are mutually coupled. As a result, the supercurrent can convert charge imbalance, that in the presence of spin splitting decays on a relatively short scale, to a long-range spin accumulation decaying only via inelastic scattering. This effect enables coherent charge-spin conversion controllable by a magnetic flux, and it can be detected by studyin…

Field (physics)superfluid densityFOS: Physical sciences02 engineering and technologyInelastic scattering01 natural sciencessuprajohteetSuperconductivity (cond-mat.supr-con)transport propertiesCondensed Matter::Superconductivity0103 physical sciences010306 general physicsSpin-½PhysicsSuperconductivityspin accumulationMesoscopic physicsspin currentta114Condensed matter physicsCondensed Matter - SuperconductivityCharge (physics)021001 nanoscience & nanotechnologyspin relaxationMagnetic fluxQuasiparticleCondensed Matter::Strongly Correlated Electrons0210 nano-technology
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Thermodynamics of computation and linear stability limits of superfluid refrigeration of a model computing array

2019

We analyze the stability of the temperature profile of an array of computing nanodevices refrigerated by flowing superfluid helium, under variations in temperature, computing rate, and barycentric velocity of helium. It turns out that if the variation in dissipated energy per bit with respect to temperature variations is higher than some critical values, proportional to the effective thermal conductivity of the array, then the steady-state temperature profiles become unstable and refrigeration efficiency is lost. Furthermore, a restriction on the maximum rate of variation in the local computation rate is found.

General MathematicsComputationGeneral Physics and Astronomychemistry.chemical_element01 natural sciences010305 fluids & plasmasSuperfluidityThermal conductivityStability analysi0103 physical sciencesComputer refrigeration; Stability analysis; Superfluid Helium; Thermodynamics of Computation010306 general physicsComputer refrigerationSettore MAT/07 - Fisica MatematicaHeliumPhysicsApplied MathematicsRefrigerationStability analysisMechanicsDissipationThermodynamics of ComputationchemistrySuperfluid helium-4Linear stabilitySuperfluid Helium
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Magneto‐elastic oscillations modulating the emission of magnetars

2017

Magneto-elastic oscillations of neutron stars are believed to explain observed quasi-periodic oscillations (QPOs) in the decaying tail of the giant flares of highly magnetized neutron stars (magnetars). Strong efforts of the theoretical modelling from different groups have increased our understanding of this phenomenon significantly. Here, we discuss some constraints on the matter in neutron stars that arise if the interpretation of the observations in terms of superfluid, magneto-elastic oscillations is correct. To explain the observed modulation of the light curve of the giant flare, we describe a model that allows the QPOs to couple to the stellar exterior through the magnetic field. In …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPhotonScatteringAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMagnetosphereAstronomy and AstrophysicsAstrophysicsMagnetar01 natural sciencesMagnetic fieldMomentumSuperfluidityNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astronomische Nachrichten
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Dark matter, dark photon and superfluid He-4 from effective field theory

2020

We consider a model of sub-GeV dark matter whose interaction with the Standard Model is mediated by a new vector boson (the dark photon) which couples kinetically to the photon. We describe the possibility of constraining such a model using a superfluid He-4 detector, by means of an effective theory for the description of the superfluid phonon. We find that such a detector could provide bounds that are competitive with other direct detection experiments only for ultralight vector mediator, in agreement with previous studies. As a byproduct we also present, for the first time, the low-energy effective field theory for the interaction between photons and phonons.

High Energy Physics - Theorylight dark matterNuclear and High Energy PhysicsPhotonDark matterFOS: Physical scienceshelium01 natural sciencesDark photonVector bosonStandard ModelSuperfluidityeffective theoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theory010306 general physicsphononLight dark matterPhysics010308 nuclear & particles physicslcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsdark photondark photon; effective theory; helium; light dark matter; phononlcsh:Physics
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Positive ion extraction across the superfluid-vapor helium interface

2009

The extraction efficiency of positive (219)Rn ions across the superfluid-vapor helium interface above similar to 1.3 K indicates that extraction results from thermal activation across a barrier of about 20 K. Below similar to 1.3 K, the extraction efficiency is constant at about 0.7%. The evaporation of the superfluid surface by second sound pulses has a negative impact on the ion extraction, but not on the ions themselves. It takes 3.2( 6) s at 1.60 K and 15( 6) s at 1.15 K for the extraction process to recover from a disturbed state of yet unknown nature.

HistoryChemistryExtraction (chemistry)EvaporationAnalytical chemistrychemistry.chemical_elementComputer Science ApplicationsEducationIonSuperfluidityThermalSecond soundAtomic physicsHeliumJournal of Physics: Conference Series 150, 032086 (2009)
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