# Analysis of MD trajectories. How to calculate static structure factor?

Posted by Vasilii Triandafilidi on April 20, 2015

## Applications. Why do we need it?

Molecular Dynamics (MD) simulations provide us with a great tool that can analyze behavior on an atomic level. It predicts the motion of atoms on the scale not reachable to experimental techniques. A natural question arises how one does build a bridge between MD simulations and experimental results. One way of doing that would be to obtain integrated quantities such Pressure, Temperature or Static Structure Factor(SSF), which can be directly seen from the experiment. For example SSF is proportional to intensity of the diffracted light in the x-ray Diffraction experiment. Interested readers are encouraged to find more about SF in the following ## Mathematical background

To be able to understand certain physical phenomena one needs to be familiar with its mathematical background. For example Static Structure Factor is impossible to understand without the prior knowledge of Fourier Transform.

a Fourier series - is a way to represent a wave-like function as the sum of plain sine waves – wikipedia.org

In other words: for every function $f(x)$ (mathematically good enough) coefficients ($a_n$, $b_n$, $\omega_n$) can be found which will fit this function.

These: $a_n$ and $b_n$ are called Fourier coefficients, $cos (\omega_n x)$, $sin(\omega_nx)$ are called Fourier harmonics.

If we rewrite our Fourier Transform using complex numbers it will look like this: $f(x) = \Sigma c_n e^{-i \omega_n x}$

In many physical applications only absolute value squared plays role, because it represents the intensity of physical value, and experiments in the physical world can measure only intensity, rather than fields. For example Static Structure Factor, which is to be discussed in further detail below. Therefore value which we are interested in is:

For better understanding let us consider following example:

Fourier series of a simple function $f(x) = cos(x)$ is the function itself. Therefore: $a_1 = 1$, $a_i = 0$ for every $i \neq 1$, $b_i = 0$ for every $i$. So an infinite curve can be represented by a single value.

Fourier Transform is very based on Fourier Series Fourier_transform. For every function in the regular space, we find a number in the reciprocal space. In other words, we define an operator which maps functions onto numbers. Therefore we analyze function by their image, which we call a spectrum. For example in the figure below we have a $cos$ function of specified period, this period corresponds to the spectrum of the function in reciprocal space. Note: Infinite curve after Fourier Transform becomes a single value, whereas a peak becomes an infinite curve. This has profound and fundamental consequences and is directly related to the uncertainty principle.

Interested reader might have already noticed that the bigger the period is by x, the smaller is the $k$ value - the wave vector.

## Theoretical background Let us look at the Fig. 2.. Visually we can identify periodic structure on the left side and a random structure on the right side. How can one quantify this order?

To be able to quantify this order may use Radial Distribution Function(RDF) RDF . By now we will define RDF as an average number of atoms on the distance $r$ from a given atom, averaged by all atoms. Later we will define RDF more rigorously.

We see an apparent periodicity on the plot, which corresponds to the periodicity of the structure. Although Radial Distribution Function seems to provide us with valuable information about system structure, it is still not very convenient to use. Things get even more complicated when we have to periodic structures ( a structure within other structure) like in the Fig. 3.

So we are not there yet. We want to be able to identify a periodic structure by just a number, not a function.

If we recall our Fourier series whenever we had something periodic in distance space, we will have a peak in the reciprocal space. And that is what we want - an easy way to track positions of atoms!

Now, if we have a structure with two characteristic distances we will be represented by two peaks in the reciprocal space. Now let’s formulate statements above in a mathematically sound way:

If we have a system of atoms with positions $\mathbf{r}_{j}$, then Radial distribution function $g(r)$:

with $\vec{r}_{ij}:= \vec{r}_{j} - \vec{r}_{i}$

, the static structure factor is defined as:

Which is an absolute value of Fourier coefficient squared. It can equally expressed the following way:

Which is the definition we will work with.

Implementation:

Now several points need to be clarified:

To implement the algorithm above, we need to figure out how to :

1. to evaluate integral
2. to deal with delta function

Evaluating integral with exponent would be performing a Fourier transform, therefore we can use tools available for that: FFT - fast fourier transform.

Delta function will be considered by binning and histogramming our atomic positions $\mathbf{r}_{j}$, which will be demonstrated on 2D example for convenience. To start with let’s import everything that we will need for our program:

import numpy as np
from MDAnalysis import \*
import os
import save_plots
from numpy.fft import fftn, fftshift
import scipy
import matplotlib
matplotlib.use('Agg')
import matplotlib.pyplot as plt


Lets define some necessary variables and bin the data:

u = Universe(psffile+'.psf', args.traj)
Ndiv = 201
# create arrays of positions, get the box dimenstions
X = u.atoms.positions
box = u.trajectory.ts.dimensions[:-3]
length_x = box[-1]  # be careful here
x = np.linspace(-length_x, length_x, Ndiv+1, endpoint=True)
# binning and histogramming
f, edges = np.histogramdd(X, bins=(Ndiv, Ndiv, Ndiv))
delta = x-x


Ok, now we are all set to do Fourier Transform and “go” to reciprocal space

ftk = (fftshift(fftn(fftshift(f))\*delta))
sk = np.abs(ftk\*\*2) / float(Natoms)
# basis in reciporal space
omega = 2\*np.pi\*np.arange(Ndiv-1) / (length_x)
omega -= omega[int(Ndiv/2)-1]


We are almost all set, the only thing is that we need to radially average our data, since we are interested only in the $|q|$

C = norm_sq(sk, k1, k2, k3, Ndiv, kmax)

def norm_sq(sk, k1, k2, k3, Ndiv, kmax):
"""
calculates normk = norm of each vector in grid=|k1,k2,k3|
bins in, calculating average sq of each bin
output: C[Nbins,3] = binindex, kval = normk, sq
"""
normk = np.sqrt(k1\*k1 + k2\*k2 + k3\*k3)
# array to histogram - dk,kmax,Nbins
Nbins = int(1.5\*Ndiv)
dk = kmax/float(Nbins)
C = np.ones((Nbins+1, 3))
for i in range(Ndiv-1):
for j in range(Ndiv-1):
for k in range(Ndiv-1):
kval = normk[i, j, k]
bindex = int(kval/dk)
C[bindex, 0] += 1
C[bindex, 1] += kval
C[bindex, 2] += sk[i, j, k]
C[:,2] /= C[:,0]
C[:,1] /= C[:,0]
return C


Special thanks to Amanda Parker.