NNP configuration: keywords
Warning
Documentation under construction…
The NNP settings file (usually named input.nn
) contains the setup of neural
networks and symmetry functions. Each line may contain a single keyword with no,
one or multiple arguments. Keywords and arguments are separated by at least one
whitespace. Lines or part of lines can be commented out with the symbol “#”,
everything right of “#” will be ignored. The order of keywords is not
important, most keywords may only appear once (exceptions: symfunction_short
and atom_energy
). Here is the list of available keywords (if no usage
information is provided, then the keyword does not support any arguments).
General NNP keywords
These keywords provide the basic setup for a neural network potential. Therefore, they are mandatory for most NNP applications and a minimal example setup file would contain at least:
number_of_elements 1
elements H
global_hidden_layers_short 2
global_nodes_short 10 10
global_activation_short t t l
cutoff_type 1
symfunction_short ...
...
These commands will set up a neural network potential for hydrogen atoms (2
hidden layers with 10 neurons each, hyperbolic tangent activation function) and
the cosine cutoff function for all symmetry functions. Of course, further
symmetry functions need to be specified by adding multiple lines starting with
the symfunction_short
keyword.
number_of_elements
Defines the number of elements the neural network potential is designed for.
- Usage:
number_of_elements <integer>
- Examples:
number_of_elements 3
elements
- Usage:
elements <string(s)>
- Examples:
elements O H Zn
This keyword defines all elements via a list of element symbols. The number of
items provided has to be consistent with the argument of the
number_of_elements
keyword. The order of the items is not important,
elements are automatically sorted according to their atomic number. The list
nnp::ElementMap::knownElements
contains a list of recognized element symbols.
atom_energy
- Usage:
atom_energy <string> <float>
- Examples:
atom_energy O -74.94518524
Definition of atomic reference energy. Shifts the total potential energy by the given value for each atom of the specified type. The first argument is the element symbol, the second parameter is the shift energy.
global_nodes_short
- Usage:
global_nodes_short <integer(s)>
- Examples:
global_nodes_short 15 10 5
Sets the number of neurons in the hidden layers of neural networks of all
elements. The number of integer arguments has to be consistent with the
argument of the global_hidden_layers_short
keyword. Note: The number of
input layer neurons is determined by the number of symmetry functions and there
is always only a single output neuron.
global_activation_short
- Usage:
global_activation_short <chars>
- Examples:
global_activation_short t t t l
Sets the activation function per layer for hidden layers and output layers
of neural networks of all elements. The number of integer arguments has to
be consistent with the argument of the global_hidden_layers_short
keyword
(i.e. number of hidden layers + 1). Activation functions are chosen via
single characters from the following table (see also
nnp::NeuralNetwork::ActivationFunction
).
Character |
Activation function type |
---|---|
l |
|
t |
|
s |
|
p |
|
r |
|
g |
|
c |
|
S |
|
e |
|
h |
normalize_nodes
Activates normalized neural network propagation, i.e. the weighted sum of connected neuron values is divided by the number of incoming connections before the activation function is applied. Thus, the default formula to calculate the neuron
is modified according to:
cutoff_type
- Usage:
cutoff_type <integer> <<float>>
- Examples:
cutoff_type 2 0.5
cutoff_type 7
Defines the cutoff function type used for all symmetry functions. The first
argument determines the functional form, see
nnp::CutoffFunction::CutoffType
for all available options. Use one
of the following integer numbers to select the cutoff type. The second argument
is optional and sets the parameter \(\alpha\). If not provided, the default
value is \(\alpha = 0.0\).
Cutoff # |
Cutoff type |
---|---|
0 |
|
1 |
|
2 |
|
3 |
|
4 |
|
5 |
|
6 |
|
7 |
|
8 |
center_symmetry_functions
scale_symmetry_functions
scale_symmetry_functions_sigma
Combining these keywords determines how the symmetry functions are scaled
before they are used as input for the neural network. See
nnp::SymFnc::ScalingType
and the following table for allowed
combinations:
Keywords present |
Scaling type |
---|---|
|
|
|
|
|
|
|
|
|
scale_min_short
scale_max_short
- Usage:
scale_min_short <float>
scale_max_short <float>
- Examples:
scale_min_short 0.0
scale_max_short 1.0
Set minimum \(S_{\min}\) and maximum \(S_{\max}\) for symmetry function
scaling. See nnp::SymmetryFunction::ScalingType
.
symfunction_short
- Usage:
symfunction_short <string> <integer> ...
- Examples:
symfunction_short H 2 H 0.01 0.0 12.0
symfunction_short H 3 O H 0.2 -1.0 4.0 12.0
symfunction_short O 9 H H 0.1 1.0 8.0 16.0
symfunction_short H 12 0.01 0.0 12.0
symfunction_short O 13 0.1 0.2 1.0 8.0 16.0
Defines a symmetry function for a specific element. The first argument is the element symbol, the second sets the type. The remaining parameters depend on the symmetry function type, follow the links in the right column of the table and look for the detailed description of the class.
Type integer |
Symmetry function type |
---|---|
2 |
|
3 |
|
9 |
|
12 |
|
13 |
|
20 |
|
21 |
|
22 |
|
23 |
|
24 |
|
25 |
ewald_truncation_error_method
In 4G the Ewald summation is used if periodic boundary conditions are applied.
Both the reciprocal and the real space sum need to be truncated. For this, two
different schemes are available. This defines the behaviour of ewald_prec
.
- Usage:
ewald_truncation_error_method <mode>
- Examples:
ewald_truncation_error_method 1
0
: default, Method by Jackson & CatlowThis method is based on the idea to truncate all terms that are smaller in magnitude than a certain threshold [3]. It is the method used in RuNNer.
1
: Method by Kolafa & PerramStatistical assumptions are made of the material to incorporate cancelling effects of the energy contributions [4]. It is the recommended method.
ewald_prec
Depending on the mode in ewald_truncation_error_method
this keyword has
different meanings. The parameter <threshold>
determines the cutoff radii in
real and reciprocal space. For both methods a smaller threshold leads to
increased radii and thus to a degrade in performance. Also the memory footprint
can become quite noticeable for very small values.
Warning
If n2p2 crashes in 4G mode because it needs more memory than available on
the machine, it may be related to the <threshold>
parameter. This can
be tested by increasing its value considerably.
If
ewald_truncation_error_method 0
- Usage:
ewald_prec <threshold>
<threshold>
is a dimensionless parameter that controls the accuracy of the Ewald summation. Typical values are in the range of1.e-2
to1.e-7
.If
ewald_truncation_error_method 1
- Usage:
ewald_prec <threshold> <max charge> <<real space cutoff>>
<threshold>
loosely corresponds to the standard deviation of the electrostatic force error one would like to achieve and has to be given in the same units as the forces in the training data. However, the methods tends to overestimate the actual error, so one may test the accuracy for different values. Choosing values that are orders of magnitude smaller than the RMSE of the short-range force errors does not make sense.<max charge>
should be the maximum charge (in magnitude) that appears during training. This does not have to be very precise but should be given in the same units as in the training data. nnp-norm outputs this quantity. The default is1.
.It is important to note that this method has two different modes.
<<real space cutoff>>
is an optional parameter. It fixes the real space cutoff in the Ewald summation and adjusts the Ewald parameter and the reciprocal space cutoff accordingly such that the specified<threshold>
is still satisfied. If<<real space cutoff>>
is chosen unreasonably small, the truncation error estimate may not be reliable anymore and a warning is given. This mode is useful when n2p2 is used in combination with other programs like LAMMPS, since they often expect a fixed cutoff during the simulation. If<<real space cutoff>>
is not specified, an optimal combination of the real and reciprocal space cutoff is computed. However, “optimal” refers to the computational effort inside n2p2. If used in combination with other programs like LAMMPS, it will not be optimal in general. Also note that the optimal cutoffs may change during the simulation since they depend on factors like simulation cell volume, number of atoms etc. In general we recommend the optimal choice of the cutoffs only if n2p2 is used as a standalone tool. If it is used in the interface mode, a good choice is to set<<real space cutoff>>
to the symmetry function cutoff. This choice may also decrease the memory footprint.
Training-specific keywords
The following keywords are solely used for training with nnp-train. All other tools and interfaces will ignore these keywords.
selection_mode
- Usage:
selection_mode <integer> <<pairs of integers>>
- Examples:
selection_mode 0
selection_mode 2 15 1 20 2
Sets the scheme to select energy and force candidates during training (first
integer argument, mandatory). If only one argument is given the chosen mode is
used for the entire training. The optional pairs of integers allow to switch the
selection mode during training. The first integer of each pair determines the
epoch when to switch while the second denotes the selection mode to switch to.
Hence, the above example means: Start the training with selection mode 2
,
then after 15 epochs switch to mode 1
and finally at epoch 20 switch back to
mode 2
until training is completed. There are three selection modes
implemented:
0
: Random selectionSelect training candidates randomly.
1
: Sort by RMSEAt the beginning of each epoch all training candidates are sorted according to their current RMSE. Throughout the epoch this list is then processed sequentially in order of descending RMSE, i.e. from highest to lowest error. This selection scheme can be helpful to decrease the error of outlier forces when used in conjunction with the optional selection mode switching (see above).
2
: Random selection with thresholdSelect training candidates randomly but use the choice only for training if the current error is above a threshold. Otherwise, select another candidate. The threshold can be set for energies and forces separately with the keywords
short_energy_error_threshold
andshort_force_error_threshold
and is expressed in terms of the last epochs RMSE, e.g.short_energy_error_threshold 1.5
means a threshold of \(1.5 \times RMSE\). Training candidates are selected randomly until the threshold condition is fulfilled or a the number of trial choices (keywordrmse_threshold_trials
) is exceeded. If even in the latter case no candidate above the threshold is found, the candidate with the highest error so far is used. This selection scheme is a variation of the adaptive process described by Blank and Brown [1] and is described here [2].
main_error_metric
- Usage:
main_error_metric <string>
- Examples:
main_error_metric RMSEpa
main_error_metric MAE
Selects the error metric to display on the screen during training. Four variants are available:
RMSEpa
: RMSE of energies per atom, RMSE of forces.RMSE
: RMSE of energies, RMSE of forces.MAEpa
: MAE of energies per atom, MAE of forces.MAE
: MAE of energies, MAE of forces.
If this keyword is omitted the default value is RMSEpa
. The keyword does not
influence the output in the learning-curve.out
file. There, all error metrics
are written.
normalize_data_set
- Usage:
normalize_data_set <string>
- Examples:
normalize_data_set ref
normalize_data_set force
Enables automatic data set normalization (see also Units) as a
pre-processing step during training with nnp-train. If this keyword is
present, an additional calculation will be performed after the initialization of
weights. The file and screen output will contain a corresponding section DATA
SET NORMALIZATION
summarizing the results of the data set normalization step.
Three different modes of normalization can be selected:
stats-only
: No or manually provided normalization, compute only statisticsThis option will trigger a calculation of statistics: mean and standard deviation of reference energies and forces will be computed. Also, a first prediction with the (randomly) initialized NN weights will be executed. Finally, statistics for these energy and force predictions will be collected and printed to screen. If present, already given normalization data (keywords
mean_energy
,conv_energy
andconv_length
) in theinput.nn
file will be read and applied.ref
: Normalization based on reference energies and forcesEnergy and force statistics are computed as in mode
stats-only
. The mean and standard deviation of reference energies and forces are used to compute three numbers for normalization: (1) the mean energy per atom, (2) a conversion factor for energies , and (3) a conversion factor for lengths . These are computed in such way that the normalized (indicated by \(^*\)) data satisfies:\[\left<e^*_\text{ref}\right> = 0 \quad \text{and} \quad \sigma_{e^*_\text{ref}} = \sigma_{F^*_\text{ref}} = 1,\]i.e., the mean reference energy per atom vanishes and there is unity standard deviation of reference energies per atom and forces. As the training run continues all necessary quantities are automatically converted to this normalized unit system.
Important
The three numbers (1), (2) and (3) are automatically written to the first lines of
input.nn
as arguments of the keywordsmean_energy
,conv_energy
andconv_length
, respectively. They are read in and normalization is applied by other tools if necessary. No additional user interaction is required. In particular, it is not required to convert settings ininput.nn
(e.g. cutoff radii, some symmetry function parameters), nor the configuration data ininput.data
. All unit conversion will be handled internally.force
: Normalization based on reference and predicted forces (recommended)Same procedure as in mode
ref
but the normalization with respect to standard deviation of energies per atom is omitted. Instead, the standard deviation of predicted forces is set to unity:\[\left<e^*_\text{ref}\right> = 0 \quad \text{and} \quad \sigma_{F^*_\text{NNP}} = \sigma_{F^*_\text{ref}} = 1,\]The prediction is carried out with the previously (randomly) initialized neural network weights. Usually this normalization procedure results in a very uniform distribution of data points in the initial reference-vs-prediction plot of the forces (see the files
train/testforces.000000.out
). This seems to be a good starting point for the HDNNP training often resulting in lower force errors than theref
mode.