Loeffler Troy D, Chan Henry, Narayanan Badri, Cherukara Mathew J, Gray Stephen, Sankaranarayanan Subramanian K R S
J Phys Chem B. 2018 Jul 19;122(28):7102-7110. doi: 10.1021/acs.jpcb.8b01791. Epub 2018 Jul 5.
Coarse-grained molecular dynamics (MD) simulations represent a powerful approach to simulate longer time scale and larger length scale phenomena than those accessible to all-atom models. The gain in efficiency, however, comes at the cost of atomistic details. The reverse transformation, also known as back mapping, of coarse-grained beads into their atomistic constituents represents a major challenge. Most existing approaches are limited to specific molecules or specific force fields and often rely on running a long-time atomistic MD of the back-mapped configuration to arrive at an optimal solution. Such approaches are problematic when dealing with systems with high diffusion barriers. Here, we introduce a new extension of the configurational-bias Monte Carlo (CBMC) algorithm, which we term the crystalline-configurational-bias Monte Carlo (C-CBMC) algorithm, which allows rapid and efficient conversion of a coarse-grained model back into its atomistic representation. Although the method is generic, we use a coarse-grained water model as a representative example and demonstrate the back mapping or reverse transformation for model systems ranging from the ice-liquid water interface to amorphous and crystalline ice configurations. A series of simulations using the TIP4P/Ice model are performed to compare the new CBMC method to several other standard Monte Carlo and molecular dynamics-based back-mapping techniques. In all of the cases, the C-CBMC algorithm is able to find optimal hydrogen-bonded configuration many thousand evaluations/steps sooner than the other methods compared within this paper. For crystalline ice structures, such as a hexagonal, cubic, and cubic-hexagonal stacking disorder structures, the C-CBMC was able to find structures that were between 0.05 and 0.1 eV/water molecule lower in energy than the ground-state energies predicted by the other methods. Detailed analysis of the atomistic structures shows a significantly better global hydrogen positioning when contrasted with the existing simpler back-mapping methods. The errors in the radial distribution functions (RDFs) of back-mapped configuration relative to reference configuration for the C-CBMC, MD, and MC were found to be 6.9, 8.7, and 12.9, respectively, for the hexagonal system. For the cubic system, the relative errors of the RDFs for the C-CBMC, MD, and MC were found to be 18.2, 34.6, and 39.0, respectively. Our results demonstrate the efficiency and efficacy of our new back-mapping approach, especially for crystalline systems where simple force-field-based relaxations have a tendency to get trapped in local minima.
粗粒度分子动力学(MD)模拟是一种强大的方法,用于模拟比全原子模型所能处理的更长时间尺度和更大长度尺度的现象。然而,效率的提升是以牺牲原子细节为代价的。将粗粒度珠子反向转换为其原子组成部分(也称为反向映射)是一项重大挑战。大多数现有方法仅限于特定分子或特定力场,并且通常依赖于对反向映射构型运行长时间的原子MD来获得最优解。在处理具有高扩散势垒的系统时,这些方法存在问题。在此,我们引入了构型偏置蒙特卡罗(CBMC)算法的一种新扩展,我们称之为晶体构型偏置蒙特卡罗(C-CBMC)算法,它允许将粗粒度模型快速有效地转换回其原子表示形式。尽管该方法具有通用性,但我们以粗粒度水模型作为代表性示例,并展示了从冰-液态水界面到非晶态和晶体冰构型的模型系统的反向映射或反向转换。使用TIP4P/Ice模型进行了一系列模拟,以将新的CBMC方法与其他几种基于标准蒙特卡罗和分子动力学的反向映射技术进行比较。在所有情况下,C-CBMC算法能够比本文中比较的其他方法早数千次评估/步骤找到最优氢键构型。对于晶体冰结构,如六方、立方和立方-六方堆积无序结构,C-CBMC能够找到能量比其他方法预测的基态能量低0.05至0.1 eV/水分子的结构。对原子结构的详细分析表明,与现有的更简单的反向映射方法相比,全局氢定位有显著改善。对于六方系统,C-CBMC、MD和MC的反向映射构型相对于参考构型的径向分布函数(RDF)误差分别为6.9、8.7和12.9。对于立方系统,C-CBMC、MD和MC的RDF相对误差分别为18.2、34.6和39.0。我们