Search results for "PLASMA"

showing 10 items of 4043 documents

Properties of the Ising magnet confined in a corner geometry

2007

Abstract The properties of Ising square lattices with nearest neighbor ferromagnetic exchange confined in a corner geometry, are studied by means of Monte Carlo simulations. Free boundary conditions at which boundary magnetic fields ± h are applied, i.e., at the two boundary rows ending at the lower left corner a field + h acts, while at the two boundary rows ending at the upper right corner a field − h acts. For temperatures T less than the critical temperature T c of the bulk, this boundary condition leads to the formation of two domains with opposite orientation of the magnetization direction, separated by an interface which for T larger than the filling transition temperature T f ( h ) …

PhysicsCondensed matter physicsTransition temperatureGeneral Physics and AstronomyBoundary (topology)GeometrySurfaces and InterfacesGeneral ChemistryCondensed Matter Physics01 natural sciences010305 fluids & plasmasSurfaces Coatings and FilmsMagnetic fieldMagnetizationFerromagnetism0103 physical sciencesIsing modelBoundary value problem010306 general physicsConfined spaceApplied Surface Science
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Radiation resonant transmission and reflection by a thin layer of an anisotropic plasma

2005

The possibility of radiation resonant transmission and reflection by a thin layer of a plasma possessing an anisotropic electron velocity distribution strongly elongated in the direction of the incident wave polarization is established.

PhysicsCondensed matter physicsbusiness.industryAnisotropic plasmaThin layerGeneral Physics and AstronomyPlasmaRadiationPolarization (waves)Electron velocityOpticsIncident wavebusinessAnisotropyPhysics Letters A
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Low-frequency internal waves in magnetized rotating stellar radiation zones

2012

Context. With the progress of observational constraints on dynamical processes in stars, it becomes necessary to understand the angular momentum and the rotation profile history. In this context, internal waves constitute an efficient transport mechanism over long distances in stellar radiation zones. Indeed, they could be one of the mechanisms responsible for the quasi-flat rotation profile of the solar radiative region up to 0.2 R ⊙ .Aims. Angular momentum transport induced by internal waves depends on the properties of their excitation regions and of their dissipation during propagation. Then, the bottom of convective envelopes (the top of convective cores, respectively) are differential…

PhysicsConvectionAngular momentumAstronomy and AstrophysicsAstrophysicsInternal wave01 natural sciences010305 fluids & plasmasMagnetic fieldsymbols.namesakeClassical mechanicsSpace and Planetary ScienceQuantum electrodynamics0103 physical sciencesAngular momentum of lightsymbolsRadiative transferDifferential rotation010303 astronomy & astrophysicsLorentz forceAstronomy & Astrophysics
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Convective stability of hot matter in ultrarelativistic heavy-ion collisions

1992

Abstract The convective stability of strongly interacting matter undergoing hydrodynamic flow in ultrarelativistic heavy-ion collisions is studied in both the quark-gluon plasma and hadron gas phases. We find that this stability depends on the form of the initial conditions assumed for the hydrodynamic flow. In the case of initial conditions corresponding to partial transparency the flow of the quark-gluon plasma is stable whereas the flow of the hadron gas is convectively unstable. The timescale for hydrodynamic oscillations around the (stable or unstable) equilibrium state is found to be larger than the expected lifetime of the system, suggesting that the flow in either case is close to n…

PhysicsConvectionNuclear and High Energy PhysicsThermodynamic equilibriumNuclear TheoryHigh Energy Physics::PhenomenologyHadronPlasmaStability (probability)Physics::Fluid DynamicsFlow (mathematics)High Energy Physics::ExperimentHeavy ionAtomic physicsNuclear ExperimentHydrodynamic flowNuclear Physics A
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Spatial distribution and statistical properties of small-scale convective vortex-like motions in a quiet-Sun region

2011

High-resolution observations of a quiet Sun internetwork region taken with the Solar 1-m Swedish Telescope in La Palma are analyzed. We determine the location of small-scale vortex motions in the solar photospheric region by computing the horizontal proper motions of small-scale structures on time series of images. These plasma convectively-driven swirl motions are associated to: (1) downdrafts (that have been commonly explained as corresponding to sites where the plasma is cooled down and hence returned to the interior below the visible photospheric level), and (2) horizontal velocity vectors converging into a central point. The sink cores are proved to be the final destination of passive …

PhysicsConvectionScale (ratio)Series (mathematics)Astronomy and AstrophysicsAstrophysicsPlasmaSpatial distributionlaw.inventionVortexTelescopeSpace and Planetary SciencelawQUIETAstrophysics::Solar and Stellar AstrophysicsMonthly Notices of the Royal Astronomical Society
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Modeling dark photon oscillations in our inhomogeneous Universe

2020

A dark photon may kinetically mix with the Standard Model photon, leading to observable cosmological signatures. The mixing is resonantly enhanced when the dark photon mass matches the primordial plasma frequency, which depends sensitively on the underlying spatial distribution of electrons. Crucially, inhomogeneities in this distribution can have a significant impact on the nature of resonant conversions. We develop and describe, for the first time, a general analytic formalism to treat resonant oscillations in the presence of inhomogeneities. Our formalism follows from the theory of level crossings of random fields and only requires knowledge of the one-point probability distribution func…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonRandom fieldPhoton conversion010308 nuclear & particles physicsFOS: Physical sciencesObservableProbability density functionElectronAstrophysics::Cosmology and Extragalactic AstrophysicsPlasma oscillation01 natural sciencesDark photonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamics0103 physical sciences010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Unravelling cosmic velocity flows: a Helmholtz-Hodge decomposition algorithm for cosmological simulations

2021

In the context of intra-cluster medium turbulence, it is essential to be able to split the turbulent velocity field in a compressive and a solenoidal component. We describe and implement a new method for this aim, i.e., performing a Helmholtz-Hodge decomposition, in multi-grid, multi-resolution descriptions, focusing on (but not being restricted to) the outputs of AMR cosmological simulations. The method is based on solving elliptic equations for a scalar and a vector potential, from which the compressive and the solenoidal velocity fields, respectively, are derived through differentiation. These equations are addressed using a combination of Fourier (for the base grid) and iterative (for t…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Solenoidal vector fieldField (physics)Adaptive mesh refinementMathematical analysisScalar (physics)General Physics and AstronomyFOS: Physical sciencesContext (language use)Astrophysics - Astrophysics of Galaxies01 natural sciences010305 fluids & plasmassymbols.namesakeHardware and ArchitectureHelmholtz free energyAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencessymbolsVector fieldAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics - Cosmology and Nongalactic AstrophysicsVector potential
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Effect of Static Disorder in an Electron-Fabry Perot Interferometr with Two Quantum Scattering Centers

2007

In a recent paper -- F. Ciccarello \emph{et al.}, New J. Phys. \textbf{8}, 214 (2006) -- we have demonstrated that the electron transmission properties of a one-dimensional (1D) wire with two identical embedded spin-1/2 impurities can be significantly affected by entanglement between the spins of the scattering centers. Such effect is of particular interest in the control of transmission of quantum information in nanostructures and can be used as a detection scheme of maximally entangled states of two localized spins. In this letter, we relax the constraint that the two magnetic impurities are equal and investigate how the main results presented in the above paper are affected by a static d…

PhysicsCoupling constantQuantum PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsSpinsScatteringFOS: Physical sciencesQuantum entanglementElectronCondensed Matter Physics01 natural sciencesIndustrial and Manufacturing EngineeringAtomic and Molecular Physics and Optics3. Good health010305 fluids & plasmasMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesCondensed Matter::Strongly Correlated ElectronsScattering theoryQuantum informationQuantum Physics (quant-ph)010306 general physicsInstrumentationFabry–Pérot interferometer
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Sensitivity of Measurement-Based Purification Processes to Inner Interactions

2017

The sensitivity of a repeated measurement-based purification scheme to additional undesired couplings is analyzed, focusing on the very simple and archetypical system consisting of two two-level systems interacting with a repeatedly measured one. Several regimes are considered and in the strong coupling (i.e., when the coupling constant of the undesired interaction is very large) the occurrence of a quantum Zeno effect is proven to dramatically jeopardize the efficiency of the purification process.

PhysicsCoupling constantQuantum PhysicspurificationFOS: Physical sciencesCondensed Matter Physics01 natural sciencesAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della Materia010305 fluids & plasmas0103 physical sciencesStrong couplingSensitivity (control systems)quantum Zeno effect010306 general physicsBiological systementanglementQuantum Physics (quant-ph)Mathematical PhysicsQuantum Zeno effect
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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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