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空间“吸引力”:并非仅由色散作用产生。

Steric "attraction": not by dispersion alone.

作者信息

Gryn'ova Ganna, Corminboeuf Clémence

机构信息

Institut des Sciences et Ingénierie Chimiques, École polytechnique fédérale de Lausanne, CH-1015 Lausanne, Switzerland.

出版信息

Beilstein J Org Chem. 2018 Jun 19;14:1482-1490. doi: 10.3762/bjoc.14.125. eCollection 2018.

DOI:10.3762/bjoc.14.125
PMID:30013675
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6037011/
Abstract

Non-covalent interactions between neutral, sterically hindered organic molecules generally involve a strong stabilizing contribution from dispersion forces that in many systems turns the 'steric repulsion' into a 'steric attraction'. In addition to London dispersion, such systems benefit from electrostatic stabilization, which arises from a short-range effect of charge penetration and gets bigger with increasing steric bulk. In the present work, we quantify this contribution for a diverse set of molecular cores, ranging from unsubstituted benzene and cyclohexane to their derivatives carrying -butyl, phenyl, cyclohexyl and adamantyl substituents. While the importance of electrostatic interactions in the dimers of sp-rich (e.g., π-conjugated) cores is well appreciated, less polarizable assemblies of sp-rich systems with multiple short-range CH···HC contacts between the bulky cyclohexyl and adamantyl moieties are also significantly influenced by electrostatics. Charge penetration is drastically larger in absolute terms for the sp-rich cores, but still has a non-negligible effect on the sp-rich dimers, investigated herein, both in terms of their energetics and equilibrium interaction distances. These results emphasize the importance of this electrostatic effect, which has so far been less recognized in aliphatic systems compared to London dispersion, and are therefore likely to have implications for the development of force fields and methods for crystal structure prediction.

摘要

中性、空间位阻有机分子之间的非共价相互作用通常涉及色散力的强大稳定作用,在许多体系中,这种作用会将“空间排斥”转变为“空间吸引”。除了伦敦色散作用外,此类体系还受益于静电稳定作用,这种作用源于电荷穿透的短程效应,且随着空间体积的增大而增强。在本工作中,我们对一系列不同的分子核心量化了这种贡献,这些分子核心包括未取代的苯和环己烷及其带有丁基、苯基、环己基和金刚烷基取代基的衍生物。虽然富sp(例如,π共轭)核心的二聚体中静电相互作用的重要性已得到充分认识,但富sp体系中具有多个短程CH···HC接触的空间位阻较大的环己基和金刚烷基部分的极化率较低的组装体也受到静电的显著影响。从绝对值来看,富sp核心的电荷穿透要大得多,但对本文研究的富sp二聚体的能量学和平衡相互作用距离而言,电荷穿透仍具有不可忽略的影响。这些结果强调了这种静电效应的重要性,与伦敦色散相比,这种效应在脂肪族体系中迄今尚未得到充分认识,因此可能对力场和晶体结构预测方法的发展产生影响。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/e7c5ce701967/Beilstein_J_Org_Chem-14-1482-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/4014a9fb0f26/Beilstein_J_Org_Chem-14-1482-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/e20ea6b209bf/Beilstein_J_Org_Chem-14-1482-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/9e16009be6da/Beilstein_J_Org_Chem-14-1482-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/8104b25ea479/Beilstein_J_Org_Chem-14-1482-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/e7c5ce701967/Beilstein_J_Org_Chem-14-1482-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/4014a9fb0f26/Beilstein_J_Org_Chem-14-1482-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/e20ea6b209bf/Beilstein_J_Org_Chem-14-1482-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/9e16009be6da/Beilstein_J_Org_Chem-14-1482-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/8104b25ea479/Beilstein_J_Org_Chem-14-1482-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/abbc/6037011/e7c5ce701967/Beilstein_J_Org_Chem-14-1482-g006.jpg

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