Title:
Equilibrium properties of fluids in the semiclassical limit

dc.contributor.authorS.K. Sinha
dc.contributor.authorY. Singh
dc.date.accessioned2026-02-09T11:02:33Z
dc.date.issued1976
dc.description.abstractThe problem of calculating the equilibrium properties of dense fluids in the semiclassical limit when the quantum effects are small is studied. Expressions are given for the pressure, free energy, and the radial distribution function in terms of the properties and correlation functions of the classical system and s-body "modified" Mayer functions Finite Part integral sign1,2,...,ss. It is shown that the correct radial distribution function of a fluid in the semiclassical limit is generated from the classical radial distribution function if we replace in turn each Finite Part integral sign0 bond (Finite Part integral sign12 0 = e-βø(1,2) -1) by an effective Finite Part integral signeff bond, where Finite Part integral signeff = Finite Part integral sign0+(1+Finite Part integral sign 0)Finite Part integral signII +(1+Finite Part integral sign0)(1+Finite Part integral signII)〈 and where 〈 is subset of the line-irreducible graphs each of which contain one Finite Part integral signIII bond. The effective pair bond correct to the second order in thermal wavelength λ ( = {2πℏ2β /m} 1/2) for a fluid of hard spheres is calculated for λ/d = 0.1, and 0.2 at reduced densities ρ* = 0.3 and 0.6. The most striking effect of the quantum mechanics on the structure of a hard-sphere fluid is found at and near the point of contact of the hard spheres. Copyright © 1977 American Institute of Physics.
dc.identifier.doi10.1063/1.523278
dc.identifier.issn222488
dc.identifier.urihttps://doi.org/10.1063/1.523278
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/59689
dc.titleEquilibrium properties of fluids in the semiclassical limit
dc.typePublication
dspace.entity.typeArticle

Files

Collections