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Anyang Peng
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Anyang Peng
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from typing import ( | ||
Dict, | ||
List, | ||
Optional, | ||
Union, | ||
) | ||
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import numpy as np | ||
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||
from deepmd.dpmodel.output_def import ( | ||
FittingOutputDef, | ||
OutputVariableDef, | ||
) | ||
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from .base_atomic_model import ( | ||
BaseAtomicModel, | ||
) | ||
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from deepmd.utils.pair_tab import ( | ||
PairTab, | ||
) | ||
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class PairTabModel(BaseAtomicModel): | ||
"""Pairwise tabulation energy model. | ||
This model can be used to tabulate the pairwise energy between atoms for either | ||
short-range or long-range interactions, such as D3, LJ, ZBL, etc. It should not | ||
be used alone, but rather as one submodel of a linear (sum) model, such as | ||
DP+D3. | ||
Do not put the model on the first model of a linear model, since the linear | ||
model fetches the type map from the first model. | ||
At this moment, the model does not smooth the energy at the cutoff radius, so | ||
one needs to make sure the energy has been smoothed to zero. | ||
Parameters | ||
---------- | ||
tab_file : str | ||
The path to the tabulation file. | ||
rcut : float | ||
The cutoff radius. | ||
sel : int or list[int] | ||
The maxmum number of atoms in the cut-off radius. | ||
""" | ||
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def __init__( | ||
self, tab_file: str, rcut: float, sel: Union[int, List[int]], **kwargs | ||
): | ||
super().__init__() | ||
self.tab_file = tab_file | ||
self.rcut = rcut | ||
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self.tab = PairTab(self.tab_file, rcut=rcut) | ||
self.ntypes = self.tab.ntypes | ||
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self.tab_info, self.tab_data = self.tab.get() | ||
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if isinstance(sel, int): | ||
self.sel = sel | ||
elif isinstance(sel, list): | ||
self.sel = sum(sel) | ||
else: | ||
raise TypeError("sel must be int or list[int]") | ||
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def get_fitting_output_def(self) -> FittingOutputDef: | ||
return FittingOutputDef( | ||
[ | ||
OutputVariableDef( | ||
name="energy", shape=[1], reduciable=True, differentiable=True | ||
) | ||
] | ||
) | ||
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def get_rcut(self) -> float: | ||
return self.rcut | ||
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def get_sel(self) -> int: | ||
return self.sel | ||
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def distinguish_types(self) -> bool: | ||
# to match DPA1 and DPA2. | ||
return False | ||
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def serialize(self) -> dict: | ||
return {"tab_file": self.tab_file, "rcut": self.rcut, "sel": self.sel} | ||
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@classmethod | ||
def deserialize(cls, data) -> "PairTabModel": | ||
tab_file = data["tab_file"] | ||
rcut = data["rcut"] | ||
sel = data["sel"] | ||
return cls(tab_file, rcut, sel) | ||
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def forward_atomic( | ||
self, | ||
extended_coord, | ||
extended_atype, | ||
nlist, | ||
mapping: Optional[np.array] = None, | ||
do_atomic_virial: bool = False, | ||
) -> Dict[str, np.array]: | ||
self.nframes, self.nloc, self.nnei = nlist.shape | ||
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# this will mask all -1 in the nlist | ||
masked_nlist = np.clip(nlist, 0) | ||
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atype = extended_atype[:, : self.nloc] # (nframes, nloc) | ||
pairwise_dr = self._get_pairwise_dist( | ||
extended_coord | ||
) # (nframes, nall, nall, 3) | ||
pairwise_rr = pairwise_dr.pow(2).sum(-1).sqrt() # (nframes, nall, nall) | ||
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self.tab_data = self.tab_data.reshape( | ||
self.tab.ntypes, self.tab.ntypes, self.tab.nspline, 4 | ||
) | ||
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# (nframes, nloc, nnei) | ||
j_type = extended_atype[ | ||
np.arange(extended_atype.size(0))[:, None, None], masked_nlist | ||
] | ||
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# slice rr to get (nframes, nloc, nnei) | ||
rr = np.take_along_axis(pairwise_rr[:, : self.nloc, :], masked_nlist, 2) | ||
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raw_atomic_energy = self._pair_tabulated_inter(nlist, atype, j_type, rr) | ||
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atomic_energy = 0.5 * np.sum( | ||
np.where( | ||
nlist != -1, raw_atomic_energy, np.zeros_like(raw_atomic_energy) | ||
), | ||
dim=-1, | ||
) | ||
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return {"energy": atomic_energy} | ||
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def _pair_tabulated_inter( | ||
self, | ||
nlist: np.array, | ||
i_type: np.array, | ||
j_type: np.array, | ||
rr: np.array, | ||
) -> np.array: | ||
"""Pairwise tabulated energy. | ||
Parameters | ||
---------- | ||
nlist : np.array | ||
The unmasked neighbour list. (nframes, nloc) | ||
i_type : np.array | ||
The integer representation of atom type for all local atoms for all frames. (nframes, nloc) | ||
j_type : np.array | ||
The integer representation of atom type for all neighbour atoms of all local atoms for all frames. (nframes, nloc, nnei) | ||
rr : np.array | ||
The salar distance vector between two atoms. (nframes, nloc, nnei) | ||
Returns | ||
------- | ||
np.array | ||
The masked atomic energy for all local atoms for all frames. (nframes, nloc, nnei) | ||
Raises | ||
------ | ||
Exception | ||
If the distance is beyond the table. | ||
Notes | ||
----- | ||
This function is used to calculate the pairwise energy between two atoms. | ||
It uses a table containing cubic spline coefficients calculated in PairTab. | ||
""" | ||
rmin = self.tab_info[0] | ||
hh = self.tab_info[1] | ||
hi = 1.0 / hh | ||
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self.nspline = int(self.tab_info[2] + 0.1) | ||
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uu = (rr - rmin) * hi # this is broadcasted to (nframes,nloc,nnei) | ||
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# if nnei of atom 0 has -1 in the nlist, uu would be 0. | ||
# this is to handle the nlist where the mask is set to 0, so that we don't raise exception for those atoms. | ||
uu = np.where(nlist != -1, uu, self.nspline + 1) | ||
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if np.any(uu < 0): | ||
raise Exception("coord go beyond table lower boundary") | ||
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idx = uu.astype(np.int) | ||
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uu -= idx | ||
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table_coef = self._extract_spline_coefficient( | ||
i_type, j_type, idx, self.tab_data, self.nspline | ||
) | ||
table_coef = table_coef.reshape(self.nframes, self.nloc, self.nnei, 4) | ||
ener = self._calcualte_ener(table_coef, uu) | ||
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# here we need to overwrite energy to zero at rcut and beyond. | ||
mask_beyond_rcut = rr >= self.rcut | ||
# also overwrite values beyond extrapolation to zero | ||
extrapolation_mask = rr >= self.tab.rmin + self.nspline * self.tab.hh | ||
ener[mask_beyond_rcut] = 0 | ||
ener[extrapolation_mask] = 0 | ||
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return ener | ||
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@staticmethod | ||
def _get_pairwise_dist(coords: np.array) -> np.array: | ||
"""Get pairwise distance `dr`. | ||
Parameters | ||
---------- | ||
coords : np.array | ||
The coordinate of the atoms shape of (nframes * nall * 3). | ||
Returns | ||
------- | ||
np.array | ||
The pairwise distance between the atoms (nframes * nall * nall * 3). | ||
""" | ||
return np.expand_dims(coords, 2) - np.expand_dims(coords, 1) | ||
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@staticmethod | ||
def _extract_spline_coefficient( | ||
i_type: np.array, | ||
j_type: np.array, | ||
idx: np.array, | ||
tab_data: np.array, | ||
nspline: int, | ||
) -> np.array: | ||
"""Extract the spline coefficient from the table. | ||
Parameters | ||
---------- | ||
i_type : np.array | ||
The integer representation of atom type for all local atoms for all frames. (nframes, nloc) | ||
j_type : np.array | ||
The integer representation of atom type for all neighbour atoms of all local atoms for all frames. (nframes, nloc, nnei) | ||
idx : np.array | ||
The index of the spline coefficient. (nframes, nloc, nnei) | ||
tab_data : np.array | ||
The table storing all the spline coefficient. (ntype, ntype, nspline, 4) | ||
nspline : int | ||
The number of splines in the table. | ||
Returns | ||
------- | ||
np.array | ||
The spline coefficient. (nframes, nloc, nnei, 4), shape may be squeezed. | ||
""" | ||
# (nframes, nloc, nnei) | ||
expanded_i_type = np.broadcast_to(i_type[:, :, np.newaxis], (i_type.shape[0], i_type.shape[1], j_type.shape[-1])) | ||
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# (nframes, nloc, nnei, nspline, 4) | ||
expanded_tab_data = tab_data[expanded_i_type, j_type] | ||
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# (nframes, nloc, nnei, 1, 4) | ||
expanded_idx = np.broadcast_to(idx[..., np.newaxis, np.newaxis], idx.shape + (1, 4)) | ||
clipped_indices = np.clip(expanded_idx, 0, nspline - 1).astype(int) | ||
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# (nframes, nloc, nnei, 4) | ||
final_coef = np.squeeze(np.take_along_axis(expanded_tab_data, clipped_indices, 3)) | ||
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# when the spline idx is beyond the table, all spline coefficients are set to `0`, and the resulting ener corresponding to the idx is also `0`. | ||
final_coef[expanded_idx.squeeze() > nspline] = 0 | ||
return final_coef | ||
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@staticmethod | ||
def _calcualte_ener(coef: np.array, uu: np.array) -> np.array: | ||
"""Calculate energy using spline coeeficients. | ||
Parameters | ||
---------- | ||
coef : np.array | ||
The spline coefficients. (nframes, nloc, nnei, 4) | ||
uu : np.array | ||
The atom displancemnt used in interpolation and extrapolation (nframes, nloc, nnei) | ||
Returns | ||
------- | ||
np.array | ||
The atomic energy for all local atoms for all frames. (nframes, nloc, nnei) | ||
""" | ||
a3, a2, a1, a0 = torch.unbind(coef, dim=-1) | ||
etmp = (a3 * uu + a2) * uu + a1 # this should be elementwise operations. | ||
ener = etmp * uu + a0 # this energy has the extrapolated value when rcut > rmax | ||
return ener |