Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics · 2003 · 22 citations · 35 references
Natural SciencesPhysicsFluid DynamicsMolecular PhysicsPhysical ChemistryFluid-structure InteractionIntermolecular ForcesMolecular DynamicsMolecular InteractionsMolecular StructureStatistical MechanicsHydrodynamic InteractionsLennard-jones PotentialPair Correlation FunctionsPopulation Density DependenceRadial Distribution FunctionsRdf ModelingStatistical Mechanics Of Identical ParticlesStatistical Mechanics Of Molecular Systems
The paper presents a general formalism for the $n\mathrm{t}\mathrm{h}\ensuremath{-}\mathrm{n}\mathrm{e}\mathrm{a}\mathrm{r}\mathrm{e}\mathrm{s}\mathrm{t}\ensuremath{-}\mathrm{n}\mathrm{e}\mathrm{i}\mathrm{g}\mathrm{h}\mathrm{b}\mathrm{o}\mathrm{r}\phantom{\rule{0ex}{0ex}}\mathrm{d}\mathrm{i}\mathrm{s}\mathrm{t}\mathrm{r}\mathrm{i}\mathrm{b}\mathrm{u}\mathrm{t}\mathrm{i}\mathrm{o}\mathrm{n}$ (NND) of identical interacting particles in a fluid confined in a $\ensuremath{\nu}$-dimensional space. The $n\mathrm{t}\mathrm{h}\ensuremath{-}\mathrm{N}\mathrm{N}\mathrm{D}$ functions, $W(n,\overline{r})$ (for $n=1,2,3,\dots{})$ in a fluid are obtained hierarchically in terms of the pair correlation function and $W(n\ensuremath{-}1,\overline{r})$ alone. The radial distribution function (RDF) profiles obtained from the molecular dynamics (MD) simulation of Lennard-Jones (LJ) fluid is used to illustrate the results. It is demonstrated that the collective structural information contained in the maxima and minima of the RDF profiles being resolved in terms of individual NND functions may provide more insights about the microscopic neighborhood structure around a reference particle in a fluid. Representative comparison between the results obtained from the formalism and the MD simulation data shows good agreement. Apart from the quantities such as $n\mathrm{t}\mathrm{h}\ensuremath{-}\mathrm{N}\mathrm{N}\mathrm{D}$ functions and $n\mathrm{t}\mathrm{h}\ensuremath{-}\mathrm{n}\mathrm{e}\mathrm{a}\mathrm{r}\mathrm{e}\mathrm{s}\mathrm{t}\ensuremath{-}\mathrm{n}\mathrm{e}\mathrm{i}\mathrm{g}\mathrm{h}\mathrm{b}\mathrm{o}\mathrm{r}$ distances, the average neighbor population number is defined. These quantities are evaluated for the LJ model system and interesting density dependence of the microscopic neighborhood shell structures are discussed in terms of them. The relevance of the NND functions in various phenomena is also pointed out.
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Stochastic Problems in Physics and Astronomy
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Random and cooperative sequential adsorption
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