Search results for "Statistical physics"

showing 10 items of 1402 documents

Crystalline multilayers of charged colloids in soft confinement: experiment versus theory.

2012

We combine real-space experiments and lattice sum calculations to investigate the phase diagram of charged colloidal particles under soft confinement. In the experiments we explore the equilibrium phase diagram of charged colloidal spheres in aqueous suspensions confined between two parallel charged walls at low background salt concentrations. Motivated by the experiments, we perform lattice sum minimizations to predict the crystalline ground state of point-like Yukawa particles which are exposed to a soft confining wall potential. In the multilayered crystalline regime, we obtain good agreement between the experimental and numerical findings: upon increasing the density we recover the sequ…

Aqueous solutionMaterials scienceCondensed matter physicsDiagramYukawa potentialCondensed Matter PhysicsLattice sumCondensed Matter::Soft Condensed MatterColloidGeneral Materials ScienceSPHERESStatistical physicsGround statePhase diagramJournal of physics. Condensed matter : an Institute of Physics journal
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Semiclassical Methods for the Description of Large Metal Clusters

1996

One of the most fascinating aspects of clusters is that they can be made arbitrarily large and therefore provide links between the microscopic and the macroscopic world. It is challenging to study how their physical properties change when going from atoms and small molecules to the bulk limit of condensed matter. But also the models and mathematical tools themselves, which are used in order to tackle the many-body problem, are an object of study for the theoretician. In particular, the question of how far quantum-mechanics must be carried with increasing size and where classical pictures become appropriate is of great interest. In this spirit, we discuss here some semiclassical methods for …

Arbitrarily largeComputer sciencePeriodic orbitsSemiclassical physicsLimit (mathematics)Statistical physicsAtomic physicsObject (philosophy)Electronic propertiesMetal clusters
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Data mining, dashboards and statistics: a powerful framework for the chemical design of molecular nanomagnets

2021

Abstract Three decades of intensive research in molecular nanomagnets have brought the magnetic memory in molecules from liquid helium to liquid nitrogen temperature. The enhancement of this operational temperature relies on a wise choice of the magnetic ion and the coordination environment. However, serendipity, oversimplified theories and chemical intuition have played the main role. In order to establish a powerful framework for statistically driven chemical design, we collected chemical and physical data for lanthanide-based nanomagnets to create a catalogue of over 1400 published experiments, developed an interactive dashboard (SIMDAVIS) to visualise the dataset, and applied inferentia…

Arrhenius equationPhysicsMolecular nanomagnetsLiquid heliumDashboard (business)chemistry.chemical_elementNanomagnetlaw.inventionsymbols.namesakechemistrylawsymbolsDysprosiumMoleculeStatistical physicsChemical design
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Modeling polyethylene with the bond fluctuation model

1997

This work presents an application of recently developed ideas about how to map real polymer systems onto abstract models. In our case the abstract model is the bond fluctuation model with a Monte Carlo dynamics. We study the temperature dependence of chain dimensions and of the self-diffusion behavior in the melt from high temperatures down to 200 K. The chain conformations are equilibrated over the whole temperature range, which is possible for the abstract type of model we use. The size of the chains as measured by the characteristic ratio is within 25% of experimental data. The simulated values of the chain self-diffusion coefficient have to be matched to experimental information at one …

Arrhenius equationSelf-diffusionWork (thermodynamics)ChemistryMonte Carlo methodGeneral Physics and AstronomyThermodynamicsActivation energyAtmospheric temperature rangesymbols.namesakeViscositysymbolsStatistical physicsPhysical and Theoretical ChemistryScaling
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Contribution to modeling the viscosity Arrhenius-type equation for some solvents by statistical correlations analysis

2014

Abstract Estimation and knowledge of transport properties of fluids are essential for heat and mass flow. Viscosity is one of the important properties which are affected by temperature and pressure. In the present work, based on the use of econometric and statistical techniques for parametric and non-parametric regression analysis and statistical correlation tests, we propose an equation modeling the relationship between the two parameters of viscosity Arrhenius-type equation, such as the Arrhenius energy ( E a ) or the pre-exponential factor ( A s ). In addition, we introduce a third interesting parameter called Arrhenius temperature ( T A ), to enrich the discussion. Empirical validation …

Arrhenius equationWork (thermodynamics)ChemistryGeneral Chemical EngineeringMass flowGeneral Physics and AstronomyThermodynamicsRegression analysisData setViscositysymbols.namesakesymbolsStatistical physicsPhysical and Theoretical ChemistryEnergy (signal processing)Parametric statisticsFluid Phase Equilibria
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N-body simulations with generic non-Gaussian initial conditions I: Power Spectrum and halo mass function

2010

We address the issue of setting up generic non-Gaussian initial conditions for N-body simulations. We consider inflationary-motivated primordial non-Gaussianity where the perturbations in the Bardeen potential are given by a dominant Gaussian part plus a non-Gaussian part specified by its bispectrum. The approach we explore here is suitable for any bispectrum, i.e. it does not have to be of the so-called separable or factorizable form. The procedure of generating a non-Gaussian field with a given bispectrum (and a given power spectrum for the Gaussian component) is not univocal, and care must be taken so that higher-order corrections do not leave a too large signature on the power spectrum.…

AstrofísicaCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)GaussianFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSeparable spacesymbols.namesakeComponent (UML)0103 physical sciencesStatistical physics010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsHalo mass functionSpectral densityAstronomy and AstrophysicsCosmologysymbolsSignature (topology)BispectrumAstrophysics - Cosmology and Nongalactic Astrophysics
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Locating ergostar models in parameter space

2020

Recently, we have shown that dynamically stable ergostar solutions (equilibrium neutron stars that contain an ergoregion) with a compressible and causal equation of state exist [A. Tsokaros, M. Ruiz, L. Sun, S. L. Shapiro, and K. Ury\=u, Phys. Rev. Lett. 123, 231103 (2019)]. These stars are hypermassive, differentially rotating, and highly compact. In this work, we make a systematic study of equilibrium models in order to locate the position of ergostars in parameter space. We adopt four equations of state that differ in the matching density of a maximally stiff core. By constructing a large number of models both with uniform and differential rotation of different degrees, we identify the p…

AstrofísicaPhysicsSurface (mathematics)High Energy Astrophysical Phenomena (astro-ph.HE)Equation of state010308 nuclear & particles physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Parameter space01 natural sciencesGeneral Relativity and Quantum CosmologyStarsNeutron starQuark starPosition (vector)0103 physical sciencesDifferential rotationStatistical physics010306 general physicsAstrophysics - High Energy Astrophysical Phenomena
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Thinking outside the box: effects of modes larger than the survey on matter power spectrum covariance

2012

Considering the matter power spectrum covariance matrix, it has recently been found that there is a potentially dominant effect on mildly non-linear scales due to power in modes of size equal to and larger than the survey volume. This {\it beat coupling} effect has been derived analytically in perturbation theory and while it has been tested with simulations, some questions remain unanswered. Moreover, there is an additional effect of these large modes, which has so far not been included in analytic studies, namely the effect on the estimated {\it average} density which enters the power spectrum estimate. In this article, we work out analytic, perturbation theory based expressions including…

Astrofísicadark matter simulationsCosmology and GravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesBeat (acoustics)Astrophysicspower spectrumAstrophysics01 natural sciences0103 physical sciencesStatistical physics010303 astronomy & astrophysics/dk/atira/pure/core/subjects/cosmologyPhysicsCosmologia010308 nuclear & particles physicsCovariance matrixMatter power spectrumcosmological simulationsSpectral densityFísicaAstronomy and AstrophysicsCovarianceRedshiftGalaxyCosmologyStepping stonegalaxy clusteringAstrophysics - Cosmology and Nongalactic Astrophysics
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Utility of Hovmöller diagrams to diagnose Rossby wave trains

2011

The study investigates and compares various methods that aim to diagnose Rossby wave trains with the help of Hovm¨ oller diagrams. Three groups of methods are distinguished: The first group contains trough-and-ridge Hovm¨ oller diagrams of the meridional wind; they provide full phase information, but differ in the method for latitudinal averaging or weighting. The second group aims to identify Rossby wave trains as a whole, discounting individual troughs and ridges. The third group contains diagnostics which focus on physical mechanisms during the different phases of a Rossby wave train life cycle; they include the analysis of eddy kinetic energy and methods for quantifying Rossby wave brea…

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorology010505 oceanographyMeridional windRossby wavePhase (waves)Eddy kinetic energy910 Geography & travelOceanographysinoptic meteorology01 natural sciencesWeightingRossby waveEarth sciencesHovmöller diagramspredictabilityddc:550TrainStatistical physics910 Geography & travelFocus (optics)0105 earth and related environmental sciencesMathematicsWolkenphysik und Verkehrsmeteorologie
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The Effect of Turbulence on the Accretional Growth of Graupel

2019

Abstract Wind tunnel experiments were carried out to investigate the influence of turbulence on the collection kernel of graupel. The collection kernel defines the growth rate of a graupel accreting supercooled droplets as it falls through a cloud. The ambient conditions were similar to those occurring typically in the mixed-phase zone of convective clouds, that is, at temperatures between −7° and −16°C and with liquid water contents from 0.5 to 1.3 g m−3. Tethered spherical collectors with radii between 220 and 340 μm were exposed in a flow carrying supercooled droplets with a mean volume radius of 10 μm. The vertical root-mean-square fluctuation velocity, the dissipation rate, and the Tay…

Atmospheric Science010504 meteorology & atmospheric sciencesTurbulence01 natural sciences010305 fluids & plasmasPhysics::Fluid DynamicsKernel (statistics)0103 physical sciencesGrowth ratePrecipitationStatistical physicsGraupel0105 earth and related environmental sciencesMathematicsJournal of the Atmospheric Sciences
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