Structure factor

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


where is the scattering wave-vector modulus

Failed to parse (Conversion error. Server ("https://wikimedia.org/api/rest_") reported: "Cannot get mml. Server problem."): {\displaystyle k=|\mathbf {k} |={\frac {4\pi }{\lambda \sin \left({\frac {\theta }{2}}\right)}}}

The structure factor is basically a Fourier transform of the pair distribution function Failed to parse (Conversion error. Server ("https://wikimedia.org/api/rest_") reported: "Cannot get mml. Server problem."): {\displaystyle {\rm {g}}(r)} ,

At zero wavenumber, i.e. ,

Failed to parse (Conversion error. Server ("https://wikimedia.org/api/rest_") reported: "Cannot get mml. Server problem."): {\displaystyle S(0)=k_{B}T\left.{\frac {\partial \rho }{\partial p}}\right\vert _{T}}

from which one can calculate the isothermal compressibility.

To calculate in molecular simulations one typically uses:

,

where is the number of particles and and are the coordinates of particles and respectively.

The dynamic, time dependent structure factor is defined as follows:

,

The ratio between the static and the dynamic structure factor, <math>S(k,t)/<math>S(k,0), is known as the collective or coherent intermediate scattering function.


References

  1. A. Filipponi, "The radial distribution function probed by X-ray absorption spectroscopy", J. Phys.: Condens. Matter, 6 pp. 8415-8427 (1994)