Jump to content

Radial distribution function

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by BenFrantzDale (talk | contribs) at 00:39, 28 March 2006 (A rough start.). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)

You must add a |reason= parameter to this Cleanup template – replace it with {{Cleanup|reason=<Fill reason here>}}, or remove the Cleanup template.

In computational mechanics, a radial distribution function, g(r), describes an average density as a function of radius normalized by the average density. Considering an atom to be located at its center, for an amorphous solid with atoms of radius σ the density of particles for radii r<2 σ will be g(r) = 0. All particles touching that particle will be at radius 2σ. As r increases, though, g(r) will converge on 1 because at a distance any adjacency effects will go to zero.

Given an energy potential function, the energy of a volume can be determined from the radial distribution function.