Machine learning assisted coarse-grained molecular dynamics modeling of meso-scale interfacial fluids Pei Ge1Linfeng Zhang2 3and Huan Lei1 4

2025-05-02 0 0 7.27MB 21 页 10玖币
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Machine learning assisted coarse-grained molecular dynamics modeling of
meso-scale interfacial fluids
Pei Ge,1Linfeng Zhang,2, 3, and Huan Lei1, 4,
1Department of Computational Mathematics, Science & Engineering,
Michigan State University, East Lansing, MI 48824, USA
2AI for Science Institute, Beijing 100080, China
3DP Technology, Beijing 100080, China
4Department of Statistics & Probability,
Michigan State University, East Lansing, MI 48824, USA
Abstract
A hallmark of meso-scale interfacial fluids is the multi-faceted, scale-dependent interfacial energy, which
often manifests different characteristics across the molecular and continuum scale. The multi-scale nature
imposes a challenge to construct reliable coarse-grained (CG) models, where the CG potential function
needs to faithfully encode the many-body interactions arising from the unresolved atomistic interactions
and account for the heterogeneous density distributions across the interface. We construct the CG models of
both single- and two-component of polymeric fluid systems based on the recently developed deep coarse-
grained potential (DeePCG) [1] scheme, where each polymer molecule is modeled as a CG particle. By only
using the training samples of the instantaneous force under the thermal equilibrium state, the constructed
CG models can accurately reproduce both the probability density function of the void formation in bulk and
the spectrum of the capillary wave across the fluid interface. More importantly, the CG models accurately
predict the volume-to-area scaling transition for the apolar solvation energy, illustrating the effectiveness to
probe the meso-scale collective behaviors encoded with molecular-level fidelity.
linfeng.zhang.zlf@gmail.com
leihuan@msu.edu
1
arXiv:2210.12482v1 [physics.comp-ph] 22 Oct 2022
I. INTRODUCTION
Molecular dynamics (MD) simulations provide a promising avenue to establish the atomistic-
level understanding of many complex systems relevant to biological and materials science. Despite
the overwhelming success during the past decades, a remaining bottleneck roots in the limitation
of the achievable spatio-temporal scales; the gap between the micro-scale atomistic motions and
many meso-scale emerging phenomena remains large. One important problem is the nano-scale
interfacial fluids, which play a crucial role in the hydration and the assembly of the biomolecules
and functional nano-materials [2, 3]. However, it is well-known that such fluid systems gener-
ally exhibit complex and multifaceted nature on different scales. On the small scale (i.e., the
fluid molecule correlation length), the solvation energy is determined by the molecular reorgani-
zation and scales with the volume of the void space. On the large scale, the solvation energy is
determined by the free energy for maintaining a fluid-void interface and scales with the surface
area. The scale-dependent behavior indicates an cross-over regime of the entropy-enthalpy transi-
tion. While theoretical understandings [4–7] of this ubiquitous phenomenon have been developed,
computational modeling often relies on full micro-scale MD simulations to retain the multifaceted
properties, which, however, remain too expensive to achieve the resolved scale for applications
such as nano-scale assembly.
To accelerate the full MD simulations, many coarse-grained (CG) models have been devel-
oped. By modeling the dynamics in terms of a set of CG variables with reduced dimensionality,
the coarse-grained molecular dynamics (CGMD) simulations, in principle, enable us to probe
the collective behaviors on a broader scale. However, in practice, the construction of truly reli-
able CG models can be highly non-trivial, especially for the meso-scale interfacial fluids. There
are two major challenges. The first challenge arises from the many-body nature of CG inter-
actions. Specifically, the equilibrium density distribution of the CG model needs to match the
marginal density distribution of the CG variables of the full model. Due to the unresolved atom-
istic degrees of freedom, the CG potential generally encodes the many-body interactions even if
the full MD force field is governed by two-body interactions [8]. Existing approaches often rely
on various physical intuitions as well as empirical approximations [9–22] that reproduce certain
target thermodynamic quantities and/or structural distributions. For example, the pairwise addi-
tive decomposition based on direct ensemble averaging [11, 12] can recover the thermodynamic
pressure but often fail to recover the pair distribution function. Conversely, the Monte Carlo and
2
Boltzmann inverse approaches [23–25] can reproduce the pairwise distribution function, which,
however, lead to the biased predictions of the equation of state. Several studies account for the
many-body effects by introducing the configuration-independent volume potential [26–28] and the
local density [21, 22, 29–32] into the pairwise interactions. On the other hand, the accuracy of the
high-order structural correlations as well as the direct applications to interfacial systems remains
under-explored.
Besides the many-body effect, the fluid molecules also exhibit heterogeneous density at the in-
terfacial vicinity. What further complicates the problem is the fact that the interfacial fluid density
distribution is scale-dependent. On the small scale, the molecular reorganization generally leads
to a wet interface with larger density than the bulk value. On the large scale, the fluid-void phase
separation generally leads to a dry interface with lower density. The crossover implies complex
molecular correlations near the interface. To capture this multi-faceted property, the constructed
CG potential needs to properly embody the local particle distribution other than the homogeneous
bulk distribution. Conventional structural-based CG potential functions generally show limitations
to incorporate such information. Similar to the many-body dissipative particle dynamics [14], re-
cent studies employed the local density [33–39] as well as the density gradient [40] as the auxiliary
field variables to construct the CG potential functions. While the CG models show significant im-
provement to reproduce the interfacial density profile, the scale-dependent interfacial energy and
fluctuations have not been systematically investigated. In Ref. [41], interfacial energy is integrated
into the continuum fluctuation hydrodynamic equation [42] from the top-down perspective. Fluid
particles essentially represent the Lagrangian discretization points based on the smoothed dissi-
pative particle hydrodynamics [43] instead of the CG molecules; the meso-scale fluid structural
properties can not be retained. Currently, the construction of reliable bottom-up CGMD models
that faithfully encode the multifaceted molecular interactions remains largely open.
In this work, we aim to address the above challenges by constructing CG models of meso-scale
interfacial fluids based on the deep molecular dynamics (DeePMD) scheme [44, 45]. DeePMD is
initially developed for learning the many-body interactions from the ab initio molecular dynamics,
and has been applied to construct the deep coarse-grained (DeePCG) model [1] of liquid water in
bulk. Unlike the conventional forms of the inter-molecular potential function, the DeePMD rep-
resents each particle as an agent and the relative positions of its neighboring particles as the local
environment. Rather than approximating the total potential of the full system by an unified para-
metric function, the DeePMD directly maps the local environment of each agent to the potential
3
energy of that particle through a neural network that strictly preserves the spatial symmetries and
the particle permutation invariance. Accordingly, the construction does not rely on the empirical
decomposition (e.g., pairwise, three-body) of the high-dimensional particle configuration space.
This unique feature is particularly suited for modeling the many-body potential of CGMD models,
where the ensemble-averaged interaction between two CG particles further depends on the other
neighboring CG particles and can not be represented by a pairwise additive function. Moreover,
the heterogeneous particle density distribution across the fluid interface can be naturally incorpo-
rated into the CG potential function as the local environment of each particle. Accordingly, the
constructed CG models can accurately model the multifaceted, scale-dependent interfacial fluctu-
ations and apolar solvation without additional human intervention.
We demonstrate the effectiveness of the CG models by considering both the single- and two-
component fluids in presence of thermal interfacial fluctuations. As discussed in Ref. [2], the
scale-dependent hydrophobic effects can be general for solvent molecules with attractive interac-
tions; polymeric liquids are therefore used as the benchmark problem. We compare the numerical
results from the full MD simulations and the CG description that represents each molecule as a
single particle located at the center of mass. By merely using training samples under equilibrium
thermal fluctuations, the constructed CG models accurately predict the high-order correlations, the
local compressibility, and the interfacial capillary wave. In contrast, the empirical CG potential
constructed based on the pairwise approximation shows apparent deviations. More importantly,
the CG models accurately predict the probability of void formation in bulk as well as the volume-
to-area scaling transition for the solvation energy, and therefore, pave the way for modeling the
nanoscale assembly in aqueous environment.
Before wrapping up this section, we note that the present work focuses on the collective, quasi-
equilibrium properties determined by the conservative potential function of a set of extensive
CG variables; see Refs. [46, 47] for relevant work. For the conformational free energy of non-
extensive CG variables, several machine-learning based approaches [48–55] have been developed;
see also a recent review [56] and the references therein. Furthermore, to accurately predict the
dynamic properties, memory and coherent noise terms [57, 58] arising from the unresolved vari-
ables need to be properly introduced into the CG model [11, 12, 59, 60], which are left to future
investigations.
4
II. METHODS AND MODELS
A. Full model of the polymeric fluids
We consider the micro-scale models of the star polymer melt similar to Ref. [12]. The full
system consists of Mmolecules with a total number of Natoms. Each polymer molecule consists
of a “center” atom connected by Naarms with Nbatoms per arm. The positions of the atoms are
denoted by q= [q1,q2,··· ,qN], where qirepresents the position of the i-th atom. The potential
function is governed by the pairwise and bond interactions, i.e.,
V(q) =
i6=j
Vp(qi j) +
k
Vb(lk),(1)
where Vpis the pairwise interaction between both the intra- and inter-molecular atoms except the
bonded pairs. qi j =kqiqjkis the distance between the i-th and j-th atoms. Vbis the bond
interaction between the neighboring particles of each polymer arm and lkis the length of the k-th
bond. The bond potential Vbis chosen to be the harmonic potential, i.e.,
Vb(l) = 1
2ks(ll0)2,(2)
where ksand l0represent the elastic coefficient and the equilibrium length l0, respectively. The
atom mass is chosen to be unity.
We investigate three fluid systems with micro-scale potential governed by Eq. (1). In Sec. III A,
we consider the polymeric fluids in bulk and examine if the CG models can retain the many-body
interactions and the local compressibility. In particular, we choose Na=12, Nb=6, σ=2.415,
ε=1.0, ks=1.714, l0=2.77 similar to Ref. [12]. Vptakes the form of the Lennard–Jones
potential with cut-off rc, i.e.,
Vp(r) =
VLJ(r)VLJ(rc),r<rc
0,rrc
VLJ(r) = 4εσ
r12 σ
r6,(3)
where ε=1.0 is the dispersion energy and σ=2.415 is the hardcore distance. Also we choose
rc=21/6σso that Vprecovers the Weeks-Chandler-Andersen potential. The full system consists of
N=2120 polymer molecules in a cubic domain 180×180×180 with periodic boundary condition
imposed along each direction. The Nosé-Hoover thermostat is employed to conduct the canonical
ensemble simulation with kBT=3.96.
5
摘要:

Machinelearningassistedcoarse-grainedmoleculardynamicsmodelingofmeso-scaleinterfacialuidsPeiGe,1LinfengZhang,2,3,andHuanLei1,4,†1DepartmentofComputationalMathematics,Science&Engineering,MichiganStateUniversity,EastLansing,MI48824,USA2AIforScienceInstitute,Beijing100080,China3DPTechnology,Beijing10...

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