Velocity Autocorrelation Functions of Hard-Sphere Fluids: Long-Time Tails upon Undercooling

Stephen R. Williams, G. Bryant, I. K. Snook, and W. van Megen
Phys. Rev. Lett. 96, 087801 – Published 28 February 2006

Abstract

Molecular dynamics simulations are employed to obtain the velocity autocorrelation function (VAF) for hard spheres, spanning a wide range of volume fractions from dilute to high-density metastable fluids. For all volume fractions below freezing, Alder’s classical positive 3/2 long-time tail is observed. For volume fractions from 0.45 to 0.48 the VAF becomes negative, before becoming positive and decaying with the positive 3/2 long-time tail. At the freezing volume fraction (0.494) the Alder 3/2 tail is not observed. At higher volume fractions a negative tail with an exponent of 5/2 emerges, which coincides with the long-time tail of a Lorentz gas.

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  • Received 16 December 2005

DOI:https://doi.org/10.1103/PhysRevLett.96.087801

©2006 American Physical Society

Authors & Affiliations

Stephen R. Williams1, G. Bryant2, I. K. Snook2, and W. van Megen2

  • 1Research School of Chemistry, Australian National University, Canberra, ACT 0200, Australia
  • 2Department of Applied Physics, Royal Melbourne Institute of Technology, Melbourne, Victoria 3000, Australia

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Issue

Vol. 96, Iss. 8 — 3 March 2006

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