Statistical mechanics, structure of matter Classical fluids and liquids Example
Hard spheres
Builds on Mayer f-functionCanonical ensemble
Example
The hard-sphere fluid is a classical system of identical balls of diameter in a region of volume in . The balls interact through the pair potential where is the distance between two centres. In the canonical ensemble the Boltzmann factor is if no two balls overlap and otherwise. So the configurational distribution is uniform on the set of non-overlapping configurations, for every temperature.
Check with the second virial coefficient: the Mayer f-function is , equal to for and for . Hence which does not depend on the temperature, and the low-density pressure is with .
Remarks
Because temperature only scales the momenta, the ratio is a function of the packing fraction alone. The packing fraction cannot exceed , the density of the densest sphere packing, by the Kepler conjecture proved by Thomas Hales. In one dimension, hard rods of length (the Tonks gas) are exactly solvable, with . In three dimensions, computer simulations show a transition from a fluid to a crystal as the density grows, driven by entropy alone.
Reading path
To understand this page from the ground up, read these 3 pages in order. The foundations come first.
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- no evidence level
- Canonical ensemble concept
- Mayer f-function concept
- Hard spheres example
Where this leads
4 pages build on this one.
Further reading
About this page
| Tag | 39NMDCPCCV |
|---|---|
| URI | m2://39NMDCPCCV |
| Kind | example |
| Writing | W0 stub |
| MSC | 82B21, 82D15, 52C17 |
| Illustrates | Mayer f-function |
| Uses | Mayer f-function, Canonical ensemble |
| Same as | |
| Changed | 3 November 2026 |
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