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CHEG231MD.py
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CHEG231MD.py
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"""
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CHEG231MD.py
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Simple MD code in Python (it's slow!) for a Lenard-Jones fluid
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based on QuickBASIC code by Richard L. Rowley [1]
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and FORTRAN code by Smit and Frenkel [2]
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Eric M. Furst
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November 2023
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[1] Richard L. Rowley (1994). Statistical Mechanics for Thermophysical Property Calculations. Prentice Hall, New York.
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[2] Daan Frenkel and Berend Smit (2002). Understanding Molecular Simulation, 2nd ed. Academic Press, New York.
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Revisions
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October 2024 - sped up with numba jit of accel routine and LJ calc.
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Requires:
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python (tested with ver. 3.12.4 build h99e199e_1 channel defaults)
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numba (tested with ver. 0.60.0 build py312hd77ebd4_0 channel defaults)
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numpy (tested with ver. 1.26.4 build py312h7f4fdc5_0 channel defaults)
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Needs:
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nn - total number of particles per dimension (thus, N = nn^3)
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rho - dimensionless number density of particles (units of rho/sigma^3)
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vmax - maximum velocity (units of sqrt[epsilon/m])
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Next to do:
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write a 2D animated version
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a challenge for students: dimensionless variables
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can a fast r_cutoff be implemented based on
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from scipy.spatial.distance import pdist, squareform?
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"""
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import numpy as np
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from numba import jit
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X, Y, Z = 0, 1, 2 # helpful for indexing
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class MDSimulation:
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"""
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x - new position coordinate array (N x 3)
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v - velocity array (N x 3)
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"""
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def __init__(self, nn, rho, vmax):
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"""
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Initialize the simulation
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- particles start on a cubic lattice
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- velocities are assigned a random fraction of the maximum
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- velocities are corrected to eliminate net flow
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"""
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# initial variables
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self.N = nn**3 # total number of particles
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self.rho = rho
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self.vol = self.N/rho # volume of the simulation
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self.L = self.vol**(1/3) # size of the simulation
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self.dL = self.L/nn # initial cubic array lattice size
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self.dt = 0.005 # dimensionless time step (0.005 is common)
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self.dt2 = self.dt*self.dt
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# initialize position and acceleration arrays
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self.x = np.zeros((self.N,3)) # init N by 3 array of positions
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self.xnew = np.zeros((self.N,3)) # init N by 3 array of positions
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self.a = np.zeros((self.N,3)) # init N by 3 array of accelerations
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# state of the simulation
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self.pe = 0 # total potential energy
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self.ke = 0 # total kinetic energy
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self.vir = 0 # virial coef
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self.T = 1 # temperature
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self.P = 0 # pressure
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# create a cubic array of particles
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particle = 0
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for i in range(0, nn):
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for j in range(0,nn):
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for k in range(0,nn):
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self.x[particle,X]=(i+0.5)*self.dL
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self.x[particle,Y]=(j+0.5)*self.dL
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self.x[particle,Z]=(k+0.5)*self.dL
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particle += 1
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# assign random velocities from uniform distribution (units?)
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self.v = vmax*np.random.rand(self.N,3) # init N x 3 array of velocities
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# normlize the velocities s/t net velocity is zero
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vcm = np.sum(self.v,axis=0)/self.N # 1x3 array of <vx>, <vy>, <vz>
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for particle in range(0,self.N):
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self.v[particle,:] -= vcm
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# set the initial accelerations
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self.accel()
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def move(self):
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"""
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Verlet velocity algorithm
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"""
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# find new positions
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self.xnew = self.x + self.v*self.dt + self.a*self.dt2/2.
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# apply periodic boundary conditions
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beyond_L = self.xnew[:,:] > self.L # N x 3 Boolean array
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self.xnew[beyond_L] -= self.L
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beyond_zero = self.xnew[:,:] < 0
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self.xnew[beyond_zero] += self.L
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self.x = self.xnew # update positions
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self.v = self.v + self.a*self.dt/2 #half update velocity
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# call accelerate
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self.accel()
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# finish velocity update
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self.v = self.v + self.a*self.dt/2
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# update properties
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self.ke = 0.5*np.sum(self.v*self.v)
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self.T = 2*self.ke/self.N/3
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self.P = self.T*self.rho + self.rho/self.N*self.vir/3
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# Non-JIT-compiled class method
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def accel(self):
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"""
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Acceleration calculated using F = ma
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"""
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self.a = np.zeros((self.N, 3)) # Zero out all accelerations
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self.pe = 0
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self.vir = 0
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# Call the JIT-compiled function to calculate acceleration
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self.pe, self.vir = accel_jit(self.N, self.x, self.a, self.L)
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# Functions are below
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# We're using numba jit to make the loop of the calculation faster
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# JIT-compiled function to calculate acceleration
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# Note: numba works by "pass in reference" with numpy arrays,
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# so self.a values are modified and used in self.move()
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# in addition to returning the values of potential energy and
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# the virial factor
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@jit(nopython=True, parallel=False)
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def accel_jit(N, x, a, L):
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pe = 0
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vir = 0
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for i in range(0, N - 1):
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for j in range(i + 1, N):
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r2 = 0
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dx = x[i, :] - x[j, :] # 1x3 array
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# Apply minimum image convention over periodic boundary conditions
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for k in range(3): # Iterate over X, Y, Z
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if abs(dx[k]) > 0.5 * L:
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dx[k] -= np.sign(dx[k]) * L
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r2 += dx[k] * dx[k]
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# Calculate the force, potential, and virial contribution
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forceri, potential, virij = LJ(r2)
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a[i, :] += forceri * dx
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a[j, :] -= forceri * dx
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pe += potential
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vir += virij
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return pe, vir
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# JIT-compiled function to calculate interaction
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@jit(nopython=True)
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def LJ(r2):
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"""
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Compute force and potential from LJ interaction
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r2 is r^2, forceri returns force/r
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"""
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r2i = 1/r2
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r6i = r2i**3
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potential = 4*(r6i*r6i-r6i)
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virij = 48*(r6i*r6i-0.5*r6i)
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forceri = virij*r2i
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return forceri, potential, virij
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