4.7.2.2. Mean Squared Displacement — MDAnalysis.analysis.msd
- Authors
Hugo MacDermott-Opeskin
- Year
2020
- Copyright
GNU Public License v2
This module implements the calculation of Mean Squared Displacements (MSDs) by the Einstein relation. MSDs can be used to characterize the speed at which particles move and has its roots in the study of Brownian motion. For a full explanation of the theory behind MSDs and the subsequent calculation of self-diffusivities the reader is directed to [Maginn2019]. MSDs can be computed from the following expression, known as the Einstein formula:
where \(N\) is the number of equivalent particles the MSD is calculated over, \(r\) are their coordinates and \(d\) the desired dimensionality of the MSD. Note that while the definition of the MSD is universal, there are many practical considerations to computing the MSD that vary between implementations. In this module, we compute a “windowed” MSD, where the MSD is averaged over all possible lag-times \(\tau \le \tau_{max}\), where \(\tau_{max}\) is the length of the trajectory, thereby maximizing the number of samples.
The computation of the MSD in this way can be computationally intensive due to
its \(N^2\) scaling with respect to \(\tau_{max}\). An algorithm to
compute the MSD with \(N log(N)\) scaling based on a Fast Fourier
Transform is known and can be accessed by setting fft=True
[Calandri2011]
[Buyl2018]. The FFT-based approach requires that the
tidynamics package is
installed; otherwise the code will raise an ImportError
.
Please cite [Calandri2011] [Buyl2018] if you use this module in addition to the normal MDAnalysis citations.
Warning
To correctly compute the MSD using this analysis module, you must supply
coordinates in the unwrapped convention. That is, when atoms pass
the periodic boundary, they must not be wrapped back into the primary
simulation cell. MDAnalysis does not currently offer this functionality in
the MDAnalysis.transformations
API despite having functions with
similar names. We plan to implement the appropriate transformations in the
future. In the meantime, various simulation packages provide utilities to
convert coordinates to the unwrapped convention. In GROMACS for example,
this can be done using gmx trjconv
with the -pbc nojump
flag.
4.7.2.2.1. Computing an MSD
This example computes a 3D MSD for the movement of 100 particles undergoing a
random walk. Files provided as part of the MDAnalysis test suite are used
(in the variables RANDOM_WALK
and
RANDOM_WALK_TOPO
)
First load all modules and test data
import MDAnalysis as mda
import MDAnalysis.analysis.msd as msd
from MDAnalysis.tests.datafiles import RANDOM_WALK_TOPO, RANDOM_WALK
Given a universe containing trajectory data we can extract the MSD
analysis by using the class EinsteinMSD
u = mda.Universe(RANDOM_WALK_TOPO, RANDOM_WALK)
MSD = msd.EinsteinMSD(u, select='all', msd_type='xyz', fft=True)
MSD.run()
The MSD can then be accessed as
msd = MSD.results.timeseries
- Visual inspection of the MSD is important, so let’s take a look at it with a
simple plot.
import matplotlib.pyplot as plt
nframes = MSD.n_frames
timestep = 1 # this needs to be the actual time between frames
lagtimes = np.arange(nframes)*timestep # make the lag-time axis
fig = plt.figure()
ax = plt.axes()
# plot the actual MSD
ax.plot(lagtimes, msd, lc="black", ls="-", label=r'3D random walk')
exact = lagtimes*6
# plot the exact result
ax.plot(lagtimes, exact, lc="black", ls="--", label=r'$y=2 D\tau$')
plt.show()
This gives us the plot of the MSD with respect to lag-time (\(\tau\)). We can see that the MSD is approximately linear with respect to \(\tau\). This is a numerical example of a known theoretical result that the MSD of a random walk is linear with respect to lag-time, with a slope of \(2d\). In this expression \(d\) is the dimensionality of the MSD. For our 3D MSD, this is 3. For comparison we have plotted the line \(y=6\tau\) to which an ensemble of 3D random walks should converge.
Note that a segment of the MSD is required to be linear to accurately determine self-diffusivity. This linear segment represents the so called “middle” of the MSD plot, where ballistic trajectories at short time-lags are excluded along with poorly averaged data at long time-lags. We can select the “middle” of the MSD by indexing the MSD and the time-lags. Appropriately linear segments of the MSD can be confirmed with a log-log plot as is often reccomended [Maginn2019] where the “middle” segment can be identified as having a slope of 1.
plt.loglog(lagtimes, msd)
plt.show()
Now that we have identified what segment of our MSD to analyse, let’s compute a self-diffusivity.
4.7.2.2.2. Computing Self-Diffusivity
Self-diffusivity is closely related to the MSD.
From the MSD, self-diffusivities \(D\) with the desired dimensionality \(d\) can be computed by fitting the MSD with respect to the lag-time to a linear model. An example of this is shown below, using the MSD computed in the example above. The segment between \(\tau = 20\) and \(\tau = 60\) is used to demonstrate selection of a MSD segment.
from scipy.stats import linregress
start_time = 20
start_index = int(start_time/timestep)
end_time = 60
linear_model = linregress(lagtimes[start_index:end_index],
msd[start_index:end_index])
slope = linear_model.slope
error = linear_model.rvalue
# dim_fac is 3 as we computed a 3D msd with 'xyz'
D = slope * 1/(2*MSD.dim_fac)
We have now computed a self-diffusivity!
4.7.2.2.3. Combining Multiple Replicates
It is common practice to combine replicates when calculating MSDs. An example of this is shown below using MSD1 and MSD2.
u1 = mda.Universe(RANDOM_WALK_TOPO, RANDOM_WALK)
MSD1 = msd.EinsteinMSD(u1, select='all', msd_type='xyz', fft=True)
MSD1.run()
u2 = mda.Universe(RANDOM_WALK_TOPO, RANDOM_WALK)
MSD2 = msd.EinsteinMSD(u2, select='all', msd_type='xyz', fft=True)
MSD2.run()
combined_msds = np.concatenate((MSD1.results.msds_by_particle,
MSD2.results.msds_by_particle), axis=1)
average_msd = np.mean(combined_msds, axis=1)
The same cannot be achieved by concatenating the replicas in a single run as the jump between the last frame of the first trajectory and frame 0 of the next trajectory will lead to an artificial inflation of the MSD and hence any subsequent diffusion coefficient calculated.
Notes
There are several factors that must be taken into account when setting up and processing trajectories for computation of self-diffusivities. These include specific instructions around simulation settings, using unwrapped trajectories and maintaining a relatively small elapsed time between saved frames. Additionally, corrections for finite size effects are sometimes employed along with various means of estimating errors [Yeh2004] [Bulow2020]. The reader is directed to the following review, which describes many of the common pitfalls [Maginn2019]. There are other ways to compute self-diffusivity, such as from a Green-Kubo integral. At this point in time, these methods are beyond the scope of this module.
Note also that computation of MSDs is highly memory intensive. If this is
proving a problem, judicious use of the start
, stop
, step
keywords to control which frames are incorporated may be required.
References
- Maginn2019(1,2,3)
Maginn, E. J., Messerly, R. A., Carlson, D. J.; Roe, D. R., Elliott, J. R. Best Practices for Computing Transport Properties 1. Self-Diffusivity and Viscosity from Equilibrium Molecular Dynamics [Article v1.0]. Living J. Comput. Mol. Sci. 2019, 1 (1).
- Yeh2004
Yeh, I. C.; Hummer, G. System-Size Dependence of Diffusion Coefficients and Viscosities from Molecular Dynamics Simulations with Periodic Boundary Conditions. J. Phys. Chem. B 2004, 108 (40), 15873–15879.
- Bulow2020
von Bülow, S.; Bullerjahn, J. T.; Hummer, G. Systematic Errors in Diffusion Coefficients from Long-Time Molecular Dynamics Simulations at Constant Pressure. 2020. arXiv:2003.09205 [Cond-Mat, Physics:Physics].
4.7.2.2.4. Classes
- class MDAnalysis.analysis.msd.EinsteinMSD(u, select='all', msd_type='xyz', fft=True, **kwargs)[source]
Class to calculate Mean Squared Displacement by the Einstein relation.
- Parameters
u (Universe or AtomGroup) – An MDAnalysis
Universe
orAtomGroup
. Note thatUpdatingAtomGroup
instances are not accepted.select (str) – A selection string. Defaults to “all” in which case all atoms are selected.
msd_type ({'xyz', 'xy', 'yz', 'xz', 'x', 'y', 'z'}) – Desired dimensions to be included in the MSD. Defaults to ‘xyz’.
fft (bool) – If
True
, uses a fast FFT based algorithm for computation of the MSD. Otherwise, use the simple “windowed” algorithm. The tidynamics package is required for fft=True. Defaults toTrue
.
- results.timeseries
The averaged MSD over all the particles with respect to lag-time.
- Type
- results.msds_by_particle
The MSD of each individual particle with respect to lag-time.
- Type
- ag
The
AtomGroup
resulting from your selection- Type
AtomGroup
New in version 2.0.0.
- Parameters
u (Universe or AtomGroup) – An MDAnalysis
Universe
orAtomGroup
.select (str) – A selection string. Defaults to “all” in which case all atoms are selected.
msd_type ({'xyz', 'xy', 'yz', 'xz', 'x', 'y', 'z'}) – Desired dimensions to be included in the MSD.
fft (bool) – If
True
, uses a fast FFT based algorithm for computation of the MSD. Otherwise, use the simple “windowed” algorithm. The tidynamics package is required for fft=True.
- run(start=None, stop=None, step=None, frames=None, verbose=None)
Perform the calculation
- Parameters
Changed in version 2.1.0: Added ability to iterate through trajectory by passing a list of frame indices