New Chemistry Unit, Jawaharlal Nehru Centre for Advanced Scientific Research (JNCASR), Jakkur, Bangalore 560064, India.
Phys Chem Chem Phys. 2020 Dec 7;22(46):26669-26681. doi: 10.1039/d0cp03557b.
n → π* has emerged as an important noncovalent interaction that can affect the conformations of both small- and macromolecules including peptides and proteins. Carbonyl-carbonyl (COCO) n → π* interactions involving CO groups are well studied. Recent studies have shown that the COCO n → π* interactions are the most abundant secondary interactions in proteins with a frequency of 33 interactions per 100 residues and, among the various secondary interactions, n → π* interactions are expected to provide the highest enthalpic contributions to the conformational stability of globular proteins. However, n → π* interactions are relatively weak and provide an average stabilization of about 0.25 kcal mol-1 per interaction in proteins. The strongest n → π* interaction could be as strong as a moderate hydrogen bond. Therefore, it is challenging to detect and quantify these weak interactions, especially in solution in the presence of perturbation from other intermolecular interactions. Accordingly, spectroscopic investigations that can provide direct evidence of n → π* interaction are limited, and the majority of papers published in this area have relied on X-ray crystallography and/or theoretical calculations to establish the presence of this interaction. The aim of this perspective is to discuss the studies where a spectroscopic signature in support of n → π* interaction was observed. As the "n → π* interaction" is a relatively new terminology, there remains the possibility of there being earlier studies where spectroscopic evidence for n → π* interactions was obtained but it was not discussed in light of the n → π* terminology. We noticed several such studies and, as can be expected, these studies were often overlooked in the discussion of n → π* interactions in the recent literature. In this perspective, we have also discussed these studies and provided computational support for the presence of n → π* interaction.
n → π* 相互作用已成为一种重要的非共价相互作用,可影响包括肽和蛋白质在内的小分子和大分子的构象。羰基-羰基 (COCO) n → π* 相互作用涉及 CO 基团,研究得比较充分。最近的研究表明,COCO n → π* 相互作用是蛋白质中最丰富的次级相互作用,每 100 个残基有 33 个相互作用,在各种次级相互作用中,n → π* 相互作用预计对球状蛋白质的构象稳定性提供最高的焓贡献。然而,n → π* 相互作用较弱,在蛋白质中每个相互作用平均稳定约 0.25 kcal mol-1。最强的 n → π* 相互作用可能与中等强度的氢键相当。因此,检测和量化这些弱相互作用具有挑战性,特别是在存在其他分子间相互作用干扰的溶液中。因此,能够提供 n → π* 相互作用直接证据的光谱研究有限,该领域发表的大多数论文都依赖于 X 射线晶体学和/或理论计算来确定这种相互作用的存在。本文的目的是讨论观察到支持 n → π* 相互作用的光谱特征的研究。由于“n → π* 相互作用”是一个相对较新的术语,因此仍有可能存在更早的研究,其中获得了 n → π* 相互作用的光谱证据,但没有根据 n → π* 术语进行讨论。我们注意到了一些这样的研究,正如预期的那样,在最近的文献中讨论 n → π* 相互作用时,这些研究往往被忽略了。在本文中,我们还讨论了这些研究,并为 n → π* 相互作用的存在提供了计算支持。