Department of Theoretical Chemistry, School of Biotechnology, Royal Institute of Technology, S-106 91 Stockholm, Sweden.
J Phys Chem B. 2010 Oct 21;114(41):13214-22. doi: 10.1021/jp1034745.
In this work we highlight the potential of NEXAFS—near-edge X-ray absorption fine structure—analysis to perform refinements of hydrogen-bond structure in DNA. For this purpose we have carried out first-principle calculations of the N1s NEXAFS spectra of the guanine and cytosine nucleobases and their tautomers, nucleosides, and nucleotides in the gas phase, as well as for five crystal structures of guanine, cytosine, or guanosine. The spectra all clearly show imine (π1*) and amine (π2*) nitrogen absorption bands with a characteristic energy difference (Δ). Among all of the intramolecule covalent connections, the tautomerism of hydrogens makes the largest influence, around ±0.4−0.5 eV change of Δ, to the spectra due to a switch of single−double bonds. Deoxyribose and ribose sugars can cause at most 0.2 eV narrowing of Δ, while the phosphate groups have nearly negligible effects on the spectra. Two kinds of intermolecule interactions are analyzed, the hydrogen bonds and the stacking effect, by comparing “compressed” and “expanded” models or by comparing models including or excluding the nearest stacking molecules. The shortening of hydrogen-bond length by 0.2−0.3 Å can result in the reduction of Δ by 0.2−0.8 eV. This is because the hydrogen bonds make the electrons more delocalized, and the amine and imine nitrogens become less distinguishable. Moreover, the hydrogen bond has a different ability to influence the spectra of different crystals, with guanine crystals as the largest (change by 0.8 eV) and the guanosine crystal as the smallest (change by 0.2 eV). The stacking has negligible effects on the spectra in all studied systems. A comparison of guanosine to guanine crystals shows that the sugars in the crystal could create “blocks” in the π-and hydrogen bonds network of bases and thus makes the imine and amine nitrogens more distinguishable with a larger Δ. Our theoretical calculations offer a good match with experimental findings and explain earlier discrepancies in the NEXAFS analysis.
在这项工作中,我们强调了近边 X 射线吸收精细结构(NEXAFS)分析在改进 DNA 中氢键结构方面的潜力。为此,我们进行了气相中鸟嘌呤和胞嘧啶碱基及其互变异构体、核苷和核苷酸的 N1s NEXAFS 光谱的第一性原理计算,以及 5 种鸟嘌呤、胞嘧啶或鸟苷晶体结构的计算。所有光谱都清楚地显示出亚胺(π1*)和胺(π2*)氮吸收带,其特征能量差(Δ)。在所有分子内共价键中,氢的互变异构作用影响最大,Δ的变化约为±0.4-0.5 eV,这是由于单双键的转换。脱氧核糖和核糖糖最多只能使Δ变窄 0.2 eV,而磷酸基团对光谱几乎没有影响。通过比较“压缩”和“扩展”模型或比较包括或不包括最近堆叠分子的模型,分析了两种分子间相互作用,氢键和堆积效应。氢键长度缩短 0.2-0.3 Å 可使 Δ 降低 0.2-0.8 eV。这是因为氢键使电子更加离域,胺和亚胺氮变得更难以区分。此外,氢键对不同晶体光谱的影响能力不同,其中鸟嘌呤晶体的影响最大(变化 0.8 eV),而鸟苷晶体的影响最小(变化 0.2 eV)。堆积对所有研究系统的光谱几乎没有影响。鸟苷与鸟嘌呤晶体的比较表明,晶体中的糖可能在碱基的π键和氢键网络中形成“块”,从而使亚胺和胺氮具有更大的Δ而更易区分。我们的理论计算与实验结果吻合良好,并解释了 NEXAFS 分析中的早期差异。