徑向分布函數g(r)代表了球殼內的平均數密度為離中心分子距離為r，體積為 的球殼內的瞬時分子數。具體參見李如生，《平衡和非平衡統計力學》科學出版社：1995
CODE:
Here are the computer codes for this article:
md_rdf.cpp
find_rdf.m
test_rdf.m
Calculating radial distribution function in molecular dynamics
First I recommend a very good book on molecular dynamics (MD) simulation: the book entitled "Molecular dynamics simulation: Elementary methods" by J. M. Haile. I read this book 7 years ago when I started to learn MD simulation, and recently I enjoyed a second reading of this fantastic book. If a beginner askes me which book he/she should read about MD, I will only recommend this. This is THE BEST introductory book on MD. It tells you what is model, what is simulation, what is MD simulation, and what is the correct attitude for doing MD simulations.
In my last blog article, I have presented a Matlab code for calculating velocity autocorrelation function (VACF) and phonon density of states (PDOS) from saved velocity data. In this article, I will present a Matlab code for calculating the radial distribution function (RDF) from saved position data. The relevant definition and algorithm are nicely presented in Section 6.4 and Appendix A of Haile's book. Here I only present a C code for doing MD simulation and a Matlab code for calculating and plotting the RDF. We aim to reproduce Fig. 6.22 in Haile's book!
Step 1.
Use the C code provided above to do an MD simulation. Note that I have used a different unit systems than that used in Haile's book (he used the LJ unit system). This code only takes 14 seconds to run in my desktop. Here are my position data (there are 100 frames and each frame has 256 atoms):
r.txt
Step 2.
Write a Matlab function which can calculate the RDF for one frame of positions:
function [g] = find_rdf(r, L, pbc, Ng, rc)
% determine some parameters
N = size(r, 1); % number of particles
L_times_pbc = L .* pbc; % deal with boundary conditions
rho = N / prod(L); % global particle density
dr = rc / Ng; % bin size
% accumulate
g = zeros(Ng, 1);
for n1 = 1 : (N - 1) % sum over the atoms
for n2 = (n1 + 1) : N % skipping half of the pairs
r12 = r(n2, :) - r(n1, :); % position difference vector
r12 = r12 - round(r12 ./L ) .* L_times_pbc; % minimum image convention
d12 = sqrt(sum(r12 .* r12)); % distance
if d12 < rc % there is a cutoff
index = ceil(d12 / dr); % bin index
g(index) = g(index) + 1; % accumulate
end
% normalize
for n = 1 : Ng
g(n) = g(n) / N * 2; % 2 because half of the pairs have been skipped
dV = 4 * pi * (dr * n)^2 * dr; % volume of a spherical shell
g(n) = g(n) / dV; % now g is the local density
g(n) = g(n) / rho; % now g is the RDF
Step 3.
Write a Matlab script to load the position data, call the function above, and plot the results:
clear; close all;
load r.txt; % length in units of Angstrom
% parameters from MD simulation
N = 256; % number of particles
L = 5.60 * [4, 4, 4]; % box size
pbc = [1, 1, 1]; % boundary conditions
% number of bins (number of data points in the figure below)
Ng = 100;
% parameters determined automatically
rc = min(L) / 2; % the maximum radius
Ns = size(r, 1) / N; % number of frames
% do the calculations
g = zeros(Ng, 1); % The RDF to be calculated
for n = 1 : Ns
r1 = r(((n - 1) * N + 1) : (n * N), :); % positions in one frame
g = g + find_rdf(r1, L, pbc, Ng, rc); % sum over frames
g = g / Ns; % time average in MD
% plot the data
r = (1 : Ng) * dr / 3.405;
figure;
plot(r, g, 'o-');
xlim([0, 3.5]);
ylim([0, 3.5]);
xlabel('r^{\ast}', 'fontsize', 15)
ylabel('g(r)', 'fontsize', 15)
set(gca, 'fontsize', 15);
Here is the figure I obtained:
Does it resemble Fig. 6. 22 in Haile's book?
本站轉載的文章為個人學習借鑒使用，本站對版權不負任何法律責任。如果侵犯了您的隱私權益，請聯系本站郵箱yoyou2525@163.com刪除。
