Search results for "quantity"

showing 10 items of 151 documents

Anti-phase wave patterns in a ring of electrically coupled oscillatory neurons

2013

International audience; Space-time dynamics of the network system modeling collective behavior of electrically coupled nonlinear cells is investigated. The dynamics of a local cell is described by the dimensionless Morris-Lecar system. It is shown that such a system yields a special class of traveling localized collective activity so called "anti-phase wave patterns". The mechanisms of formation of the patterns are discussed and the region of their existence is obtained by using the weakly coupled oscillators theory.

PhysicsCollective behaviorDynamics (mechanics)Phase (waves)General Physics and AstronomySpecial classRing (chemistry)01 natural sciences010305 fluids & plasmas[SPI.TRON]Engineering Sciences [physics]/Electronics[ SPI.TRON ] Engineering Sciences [physics]/Electronics010101 applied mathematicsNonlinear systemClassical mechanics0103 physical sciencesGeneral Materials ScienceStatistical physics0101 mathematicsPhysical and Theoretical ChemistryDimensionless quantity
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Effects of nonlinear sweep in the Landau-Zener-Stueckelberg effect

2002

We study the Landau-Zener-Stueckelberg (LZS) effect for a two-level system with a time-dependent nonlinear bias field (the sweep function) W(t). Our main concern is to investigate the influence of the nonlinearity of W(t) on the probability P to remain in the initial state. The dimensionless quantity epsilon = pi Delta ^2/(2 hbar v) depends on the coupling Delta of both levels and on the sweep rate v. For fast sweep rates, i.e., epsilon << l and monotonic, analytic sweep functions linearizable in the vicinity of the resonance we find the transition probability 1-P ~= epsilon (1+a), where a>0 is the correction to the LSZ result due to the nonlinearity of the sweep. Further increase …

PhysicsCondensed Matter - Materials ScienceStatistical Mechanics (cond-mat.stat-mech)Zero (complex analysis)Materials Science (cond-mat.mtrl-sci)FOS: Physical sciencesResonanceState (functional analysis)Type (model theory)Coupling (probability)ExponentComplex planeCondensed Matter - Statistical MechanicsMathematical physicsDimensionless quantity
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Heat diffusion in the disordered electron gas

2015

We study the thermal conductivity of the disordered two-dimensional electron gas. To this end we analyze the heat density-heat density correlation function concentrating on the scattering processes induced by the Coulomb interaction in the sub-temperature energy range. These scattering processes are at the origin of logarithmic corrections violating the Wiedemann-Franz law. Special care is devoted to the definition of the heat density in the presence of the long-range Coulomb interaction. To clarify the structure of the correlation function, we present details of a perturbative calculation. While the conservation of energy strongly constrains the general form of the heat density-heat densit…

PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)ScatteringFOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesConserved quantityCondensed Matter - Strongly Correlated ElectronsCorrelation function (statistical mechanics)Thermal conductivity0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)CoulombHeat equation010306 general physics0210 nano-technologyFermi gasSpin-½
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Delocalization-Localization Transition due to Anharmonicity

2008

Analytical and numerical calculations for a reduced Fermi-Pasta-Ulam chain demonstrate that energy localization does not require more than one conserved quantity. Clear evidence for the existence of a sharp delocalization-localization transition at a critical amplitude is given. Approaching the critical amplitude from above and below, diverging time scales occur. Above the critical amplitude, the energy packet converges towards a discrete breather. Nevertheless, ballistic energy transportation is present, demonstrating that its existence does not necessarily imply delocalization.

PhysicsCondensed matter physicsBreatherAnharmonicityGeneral Physics and AstronomyFOS: Physical sciencesConserved quantityCondensed Matter - Other Condensed MatterDelocalized electronAmplitudeChain (algebraic topology)Quantum mechanicsEnergy (signal processing)Other Condensed Matter (cond-mat.other)
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A study of free convection in air around horizontal cylinders of different diameters based on holographic interferometry. Temperature field equations…

2002

Abstract Holographic interferometry is used to study free convection in air around horizontal cylinders of different diameters and equal length, involving different surface temperatures, with the aim of defining the corresponding temperature fields. Interferograms were obtained to determine the temperature (T) of each point as well as its distance (x) from the surface of the cylinder. These values in turn made it possible to define functions (of an exponential nature in our case), T=f(x), that satisfactorily reproduced the temperature fields. Posteriorly, these functions were used to calculate the local convection coefficients, determining their dependency upon temperature and the direction…

PhysicsConvectionNatural convectionHeat transferGeneral EngineeringThermodynamicsMechanicsHeat transfer coefficientCondensed Matter PhysicsHolographic interferometryNusselt numberDimensionless quantityForced convectionInternational Journal of Thermal Sciences
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Thermal conduction by dark matter with velocity and momentum-dependent cross-sections

2014

We use the formalism of Gould and Raffelt to compute the dimensionless thermal conduction coefficients for scattering of dark matter particles with standard model nucleons via cross-sections that depend on the relative velocity or momentum exchanged between particles. Motivated by models invoked to reconcile various recent results in direct detection, we explicitly compute the conduction coefficients $\alpha$ and $\kappa$ for cross-sections that go as $v_{\rm rel}^2$, $v_{\rm rel}^4$, $v_{\rm rel}^{-2}$, $q^2$, $q^4$ and $q^{-2}$, where $v_{\rm rel}$ is the relative DM-nucleus velocity and $q$ is the momentum transferred in the collision. We find that a $v_{\rm rel}^{-2}$ dependence can sig…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterRelative velocityFOS: Physical sciencesAstronomy and AstrophysicsThermal conduction01 natural sciencesOuter coreComputational physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Solar coreAstrophysics - Solar and Stellar Astrophysics0103 physical sciencesThermalNucleon010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Dimensionless quantityAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark sectors with dynamical coupling

2019

Coupled dark matter-dark energy scenarios are modeled via a dimensionless parameter $��$, which controls the strength of their interaction. While this coupling is commonly assumed to be constant, there is no underlying physical law or symmetry that forbids a time-dependent $��$ parameter. The most general and complete interacting scenarios between the two dark sectors should therefore allow for such a possibility, and it is the main purpose of this study to constrain two possible and well-motivated coupled cosmologies by means of the most recent and accurate early and late-time universe observations. We find that CMB data alone prefers $��(z) >0$ and therefore a smaller amount of dark ma…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsmedia_common.quotation_subjectDark matterCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCoupling (probability)01 natural sciencesSymmetry (physics)UniverseGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciences010306 general physicsConstant (mathematics)Energy (signal processing)media_commonDimensionless quantityAstrophysics - Cosmology and Nongalactic Astrophysics
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Convergent Strong-Coupling Expansions from Divergent Weak-Coupling Perturbation Theory

1995

Divergent weak-coupling perturbation expansions for physical quantities can be converted into sequences of uniformly and exponentially fast converging approximations. This is possible with the help of an additional variational parameter to be optimized order by order. The uniformity of the convergence for any coupling strength allows us to take all expressions directly to the strong-coupling limit, yielding a simple calculation scheme for the coefficients of convergent strong-coupling expansions. As an example, we determine these coefficients for the ground state energy of the anharmonic oscillator up to 22nd order with a precision of about 20 digits.

PhysicsCoupling strengthMathematical analysisAnharmonicityStrong couplingGeneral Physics and AstronomyPerturbation (astronomy)Ground statePhysical quantityPhysical Review Letters
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Comment on "Direct linear term in the equation of state of plasmas"

2015

In a recent paper [Phys. Rev. E 91, 013108 (2015)], Kraeft et al. criticize known exact results on the equation of state of quantum plasmas, which have been obtained independently by several authors. They argue about a difference in the definition of the direct two-body function Q(x), which appears in virial expansions of thermodynamical quantities, but Q(x) is not a measurable quantity in itself. Differences in definitions of intermediate quantities are irrelevant, and only differences in physical quantities are meaningful. Beyond Kraeft et al.'s broad statement that there is no agreement at order ρ(5/2) in the virial equation for the pressure, we show that their published results for this…

PhysicsEquation of stateLinear termQuantum mechanicsOrder (group theory)PlasmaFunction (mathematics)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]QuantumVirial theoremComputingMilieux_MISCELLANEOUSPhysical quantityMathematical physics
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Effect of spin on the inspiral of binary neutron stars

2019

We perform long-term simulations of spinning binary neutron stars, with our highest dimensionless spin being $\chi \sim 0.32$. To assess the importance of spin during the inspiral we vary the spin, and also use two equations of state, one that consists of plain nuclear matter and produces compact stars (SLy), and a hybrid one that contains both nuclear and quark matter and leads to larger stars (ALF2). Using high resolution that has grid spacing $\Delta x\sim 98$ m on the finest refinement level, we find that the effects of spin in the phase evolution of a binary system can be larger than the one that comes from tidal forces. Our calculations demonstrate explicitly that although tidal effec…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AstrofísicaParticle physicsSpins010308 nuclear & particles physicsBinary numberFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Nuclear matter01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyNeutron starStarsStrange matter0103 physical sciencesAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSpin-½Dimensionless quantity
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