4.7.2.1. Radial Distribution Functions — `MDAnalysis.analysis.rdf`

This module contains two classes to calculate radial pair distribution functions (radial distribution functions or “RDF”). The RDF \(g_{ab}(r)\) between types of particles \(a\) and \(b\) is

\[g_{ab}(r) = (N_{a} N_{b})^{-1} \sum_{i=1}^{N_a} \sum_{j=1}^{N_b} \langle \delta(|\mathbf{r}_i - \mathbf{r}_j| - r) \rangle\]

which is normalized so that the RDF becomes 1 for large separations in a homogenous system. The RDF effectively counts the average number of \(b\) neighbours in a shell at distance \(r\) around a \(a\) particle and represents it as a density.

The radial cumulative distribution function is

\[G_{ab}(r) = \int_0^r \!\!dr' 4\pi r'^2 g_{ab}(r')\]

and the average number of \(b\) particles within radius \(r\)

\[N_{ab}(r) = \rho G_{ab}(r)\]

(with the appropriate density \(\rho\)). The latter function can be used to compute, for instance, coordination numbers such as the number of neighbors in the first solvation shell \(N(r_1)\) where \(r_1\) is the position of the first minimum in \(g(r)\).

We provide options for calculating the density of particle \(b\) in a shell at distance \(r\) around a \(a\) particle, which is

\[n_{ab}(r) = \rho g_{ab}(r)\]

class MDAnalysis.analysis.rdf.InterRDF(g1, g2, nbins=75, range=(0.0, 15.0), norm='rdf', exclusion_block=None, exclude_same=None, **kwargs)[source]

Radial distribution function

InterRDF is a tool to calculate average radial distribution functions between two groups of atoms. Suppose we have two AtomGroups A and B. A contains atom A1, A2, and B contains B1, B2. Given A and B to InterRDF, the output will be the average of RDFs between A1 and B1, A1 and B2, A2 and B1, A2 and B2. A typical application is to calculate the RDF of solvent with itself or with another solute.

The radial distribution function is calculated by histogramming distances between all particles in g1 and g2 while taking periodic boundary conditions into account via the minimum image convention.

The exclusion_block keyword may be used to exclude a set of distances from the calculations.

Results are available in the attributes results.rdf and results.count.

Parameters

g1 (AtomGroup) – First AtomGroup
g2 (AtomGroup) – Second AtomGroup
nbins (int) – Number of bins in the histogram
range (tuple or list) – The size of the RDF
norm (str, {'rdf', 'density', 'none'}) –
For ‘rdf’ calculate \(g_{ab}(r)\). For ‘density’ the single particle density \(n_{ab}(r)\) is computed. ‘none’ computes the number of particles occurences in each spherical shell.

New in version 2.3.0.
exclusion_block (tuple) – A tuple representing the tile to exclude from the distance array.
exclude_same (str) – Will exclude pairs of atoms that share the same “residue”, “segment”, or “chain”. Those are the only valid values. This is intended to remove atoms that are spatially correlated due to direct bonded connections.
verbose (bool) – Show detailed progress of the calculation if set to True

results.bins

numpy.ndarray of the centers of the nbins histogram bins.

New in version 2.0.0.

Type: numpy.ndarray

bins

Alias to the results.bins attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.bins instead.

Type: numpy.ndarray

results.edges

numpy.ndarray of the nbins + 1 edges of the histogram bins.

New in version 2.0.0.

Type: numpy.ndarray

edges

Alias to the results.edges attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.edges instead.

Type: numpy.ndarray

results.rdf

numpy.ndarray of the radial distribution function values for the results.bins.

New in version 2.0.0.

Type: numpy.ndarray

rdf

Alias to the results.rdf attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.rdf instead.

Type: numpy.ndarray

results.count

numpy.ndarray representing the radial histogram, i.e., the raw counts, for all results.bins.

New in version 2.0.0.

Type: numpy.ndarray

count

Alias to the results.count attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.count instead.

Type: numpy.ndarray

Example

First create the InterRDF object, by supplying two AtomGroups then use the run() method

rdf = InterRDF(ag1, ag2)
rdf.run()

Results are available through the results.bins and results.rdf attributes:

plt.plot(rdf.results.bins, rdf.results.rdf)

The exclusion_block keyword allows the masking of pairs from within the same molecule. For example, if there are 7 of each atom in each molecule, the exclusion mask (7, 7) can be used.

New in version 0.13.0.

Changed in version 1.0.0: Support for the start, stop, and step keywords has been removed. These should instead be passed to InterRDF.run().

Changed in version 2.0.0: Store results as attributes bins, edges, rdf and count of the results attribute of AnalysisBase.

class MDAnalysis.analysis.rdf.InterRDF_s(u, ags, nbins=75, range=(0.0, 15.0), norm='rdf', density=False, **kwargs)[source]

Site-specific radial distribution function

Calculates site-specific radial distribution functions. Instead of two groups of atoms it takes as input a list of pairs of AtomGroup, [[A, B], [C, D], ...]. Given the same A and B to InterRDF_s, the output will be a list of individual RDFs between A1 and B1, A1 and B2, A2 and B1, A2 and B2 (and similarly for C and D). These site-specific radial distribution functions are typically calculated if one is interested in the solvation shells of a ligand in a binding site or the solvation of specific residues in a protein.

Parameters

u (Universe) –
a Universe that contains atoms in ags

Deprecated since version 2.3.0: This parameter is superflous and will be removed in MDAnalysis 3.0.0.
ags (list) – a list of pairs of AtomGroup instances
nbins (int) – Number of bins in the histogram
range (tuple or list) – The size of the RDF
norm (str, {'rdf', 'density', 'none'}) –
For ‘rdf’ calculate \(g_{ab}(r)\). For ‘density’ the single particle density \(n_{ab}(r)\) is computed. ‘none’ computes the number of particles occurences in each spherical shell.

New in version 2.3.0.
density (bool) –
False: calculate \(g_{ab}(r)\); True: calculate the true single particle density \(n_{ab}(r)\). density overwrites the norm parameter.

New in version 1.0.1: This keyword was available since 0.19.0 but was not documented. Furthermore, it had the opposite meaning. Since 1.0.1 it is officially supported as documented.

Deprecated since version 2.3.0: Instead of density=True use norm=’density’

results.bins

numpy.ndarray of the centers of the nbins histogram bins; all individual site-specific RDFs have the same bins.

New in version 2.0.0.

Type: numpy.ndarray

bins

Alias to the results.bins attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.bins instead.

Type: numpy.ndarray

results.edges

array of the nbins + 1 edges of the histogram bins; all individual site-specific RDFs have the same bins.

New in version 2.0.0.

Type: numpy.ndarray

edges

Alias to the results.edges attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.edges instead.

Type: numpy.ndarray

results.rdf

list of the site-specific radial distribution functions if norm=’rdf’ or density functions for the bins if norm=’density’. The list contains len(ags) entries. Each entry for the i-th pair [A, B] = ags[i] in ags is a numpy.ndarray with shape (len(A), len(B)), i.e., a stack of RDFs. For example, results.rdf[i][0, 2] is the RDF between atoms A[0] and B[2].

New in version 2.0.0.

Type: list

rdf

Alias to the results.rdf attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.rdf instead.

Type: list

results.count

list of the site-specific radial histograms, i.e., the raw counts, for all results.bins. The data have the same structure as results.rdf except that the arrays contain the raw counts.

New in version 2.0.0.

Type: list

count

Alias to the results.count attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.count instead.

Type: list

results.cdf

list of the site-specific cumulative counts, for all results.bins. The data have the same structure as results.rdf except that the arrays contain the cumulative counts.

This attribute only exists after get_cdf() has been run.

New in version 2.0.0.

Type: list

cdf

Alias to the results.cdf attribute.

Deprecated since version 2.0.0: This attribute will be removed in 3.0.0. Use results.cdf instead.

Type: list

Example

First create the InterRDF_s object, by supplying one Universe and one list of pairs of AtomGroups, then use the run() method:

from MDAnalysisTests.datafiles import GRO_MEMPROT, XTC_MEMPROT
u = mda.Universe(GRO_MEMPROT, XTC_MEMPROT)

s1 = u.select_atoms('name ZND and resid 289')
s2 = u.select_atoms('(name OD1 or name OD2) and resid 51 and sphzone 5.0 (resid 289)')
s3 = u.select_atoms('name ZND and (resid 291 or resid 292)')
s4 = u.select_atoms('(name OD1 or name OD2) and sphzone 5.0 (resid 291)')
ags = [[s1, s2], [s3, s4]]

rdf = InterRDF_s(u, ags)
rdf.run()

Results are available through the results.bins and results.rdf attributes:

plt.plot(rdf.results.bins, rdf.results.rdf[0][0, 0])

(Which plots the rdf between the first atom in s1 and the first atom in s2)

To generate the cumulative distribution function (cdf) in the sense of “particles within radius \(r\)”, i.e., \(N_{ab}(r)\), use the get_cdf() method

cdf = rdf.get_cdf()

Results are available through the results.cdf attribute:

plt.plot(rdf.results.bins, rdf.results.cdf[0][0, 0])

(Which plots the cdf between the first atom in s1 and the first atom in s2)

New in version 0.19.0.

Changed in version 1.0.0: Support for the start, stop, and step keywords has been removed. These should instead be passed to InterRDF_s.run().

Changed in version 2.0.0: Store results as attributes bins, edges, rdf, count and cdf of the results attribute of AnalysisBase.

Changed in version 2.3.0: Introduce norm and exclusion_blocks attributes.

Deprecated since version 2.3.0: Instead of density=True use norm=’density’

Deprecated since version 2.3.0: The universe parameter is superflous.

get_cdf()[source]

Calculate the cumulative counts for all sites.

This is the cumulative count within a given radius, i.e., \(N_{ab}(r)\).

The result is returned and also stored in the attribute results.cdf.

Returns: cdf – list of arrays with the same structure as results.rdf
Return type: list

4.7.2.1. Radial Distribution Functions — MDAnalysis.analysis.rdf

4.7.2.1. Radial Distribution Functions — `MDAnalysis.analysis.rdf`