Structural and energetic stability of the lowest equilibrium structures of water clusters

IF 1.6 4区 物理与天体物理 Q3 PHYSICS, CONDENSED MATTER
Vishwa K. Bhatt, Sajeev S. Chacko, Nitinkumar M. Bijewar, Balasaheb J. Nagare
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Abstract

Water molecules with their hydrogen bonding capability, exhibit exceptional properties in the bulk as well as in cluster form. In the present work, we study the size-dependent trends in the structure, energetics, bonding, ionisation potential, fragmentation pattern, and optical properties of water clusters in the size range of n = 2–20, and an interplay between them. We have extensively searched for the lowest energy structures of the water clusters using the artificial bee colony algorithm, optimised them first with the classical force field TIP4P and then relaxed at least 10 lowest energy structures using density functional theory. We have found new lowest energy structures for all the sizes as against the ones reported earlier. The structures and stability of water clusters are primarily dictated by the H-bond network. However, we found the weak van der Waals interactions also play a crucial role in stabilising the clusters giving them unique characteristics. Some of the clusters such as those with \(n=4, 8, 10, 12\) and 15 molecules were structurally symmetric, yet a close analysis of various properties reveals that the clusters with \(n=4, 8, 12, 14\) and 19 molecules are more stable than others. Spherical or nearly spherical clusters were found to be the most stable, corroborated by the shape deformation parameters and the fragmentation pattern, which indicated a higher likelihood of forming fragments of sizes \(n=4, 8, 12, 14\), and 16. A blueshift of the H-O-H vibrational modes and a redshift of the O–H stretching modes is seen for most clusters. Such characteristics in the vibrational spectra is associated with an increase in the H-bond strength which is seen to increase with size of the cluster. Large optical band gaps for \(n=4, 8, 12\) and 16 along with blueshifts in optical spectra implies these clusters to be chemically more stable than others.

水团簇最低平衡结构的结构和能量稳定性
具有氢键能力的水分子,无论在团簇形式下,都表现出特殊的性质。在本研究中,我们研究了n = 2-20尺寸范围内水团簇的结构、能量学、成键、电离势、破碎模式和光学性质的尺寸依赖趋势,以及它们之间的相互作用。我们使用人工蜂群算法广泛搜索了水团簇的最低能量结构,首先使用经典力场TIP4P进行优化,然后使用密度泛函理论放松了至少10个最低能量结构。与之前报道的不同,我们发现了所有尺寸的新的最低能量结构。水团簇的结构和稳定性主要由氢键网络决定。然而,我们发现弱范德华相互作用在稳定星团方面也起着至关重要的作用,赋予它们独特的特征。一些团簇,如含有\(n=4, 8, 10, 12\)和15个分子的团簇在结构上是对称的,但对各种性质的仔细分析表明,含有\(n=4, 8, 12, 14\)和19个分子的团簇比其他团簇更稳定。球形或接近球形的团簇是最稳定的,形状变形参数和破碎模式证实了这一点,这表明形成尺寸为\(n=4, 8, 12, 14\)和16的碎片的可能性更高。在大多数星团中,我们可以看到H-O-H振动模式的蓝移和O-H拉伸模式的红移。振动谱中的这种特征与氢键强度的增加有关,氢键强度随着团簇的大小而增加。\(n=4, 8, 12\)和16的大光学带隙以及光谱中的蓝移意味着这些星团在化学上比其他星团更稳定。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
The European Physical Journal B
The European Physical Journal B 物理-物理:凝聚态物理
CiteScore
2.80
自引率
6.20%
发文量
184
审稿时长
5.1 months
期刊介绍: Solid State and Materials; Mesoscopic and Nanoscale Systems; Computational Methods; Statistical and Nonlinear Physics
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