The structure factor,
, for a monatomic system is defined by:

where
is the scattering wave-vector modulus

The structure factor is basically a Fourier transform of the pair distribution function
,

At zero wavenumber, i.e.
,

from which one can calculate the isothermal compressibility.
To calculate
in computer simulations one typically uses:

- Failed to parse (syntax error): {\displaystyle S(k) = \frac{1}{N} \sum^{N}_{i,j=1} \left< \exp(-i(r_i-r_j)) \right>}
References
- A. Filipponi, "The radial distribution function probed by X-ray absorption spectroscopy", J. Phys.: Condens. Matter, 6 pp. 8415-8427 (1994)