Université Paris-Saclay, CEA, CNRS, LIDYL, F-91191 Gif-sur-Yvette, France.
Acc Chem Res. 2021 Mar 2;54(5):1226-1235. doi: 10.1021/acs.accounts.0c00603. Epub 2021 Feb 15.
The intrinsic fluorescence of nucleic acids is extremely weak compared to that of the fluorescent labels used to probe their structural and functional behavior. Thus, for technical reasons, the investigation of the intrinsic DNA fluorescence was limited for a long time. But with the improvement in spectroscopic techniques, the situation started to change around the turn of the century. During the past two decades, various factors modulating the static and dynamic properties of the DNA fluorescence have been determined; it was shown that, under certain conditions, quantum yields may be up 100 times higher than what was known so far. The ensemble of these studies opened up new paths for the development of label-free DNA fluorescence for biochemical applications. In parallel, these studies have shed new light on the primary processes leading to photoreactions that damage DNA when it absorbs UV radiation.We have been studying a variety of DNA systems, ranging from the monomeric nucleobases to double-stranded and four-stranded structures using fluorescence spectroscopy. The specificity of our work resides in the quantitative association of the steady-state fluorescence spectra with time-resolved data recorded from the femtosecond to the nanosecond timescales, made possible by the development of specific methodologies.Among others, our fluorescence studies provide information on the energy and the polarization of electronic transitions. These are valuable indicators for the evolution of electronic excitations in complex systems, where the electronic coupling between chromophores plays a key role. Highlighting collective effects that originate from electronic interactions in DNA multimers is the objective of the present Account.In contrast to the monomeric chromophores, whose fluorescence decays within a few picoseconds, that of DNA multimers persists on the nanosecond timescale. Even if long-lived states represent only a small fraction of electronic excitations, they may be crucial to the DNA photoreactivity because the probability to reach reactive conformations increases over time, owing to the incessant structural dynamics of nucleic acids.Our femtosecond studies have revealed that an ultrafast excitation energy transfer takes place among the nucleobases within duplexes and G-quadruplexes. Such an ultrafast process is possible when collective states are populated directly upon photon absorption. At much longer times, we discovered an unexpected long-lived high-energy emission stemming from what was coined "HELM excitons". These collective states, whose emission increases with the duplex size, could be responsible for the delayed fluorescence of ππ* states observed for genomic DNA.Most studies dealing with excited-state relaxation in DNA were carried out with excitation in the absorption band peaking at around 260 nm. We went beyond this and also performed the first time-resolved study with excitation in the UVA spectral range, where a very weak absorption tail is present. The resulting fluorescence decays are much slower and the fluorescence quantum yields are much higher than for UVC excitation. We showed that the base pairing of DNA strands enhances the UVA fluorescence and, in parallel, increases the photoreactivity because it modifies the nature of the involved collective excited states.
与用于探测其结构和功能行为的荧光标记物相比,核酸的固有荧光极其微弱。因此,出于技术原因,很长一段时间以来,对固有 DNA 荧光的研究都受到限制。但随着光谱技术的进步,这种情况在世纪之交开始发生变化。在过去的二十年中,已经确定了调节 DNA 荧光静态和动态特性的各种因素;结果表明,在某些条件下,量子产率可能比目前已知的高出 100 倍。这些研究的综合结果为生物化学应用中的无标记 DNA 荧光的发展开辟了新的途径。与此同时,这些研究也为导致 DNA 吸收紫外线辐射时发生光反应的初级过程提供了新的认识。我们一直在使用荧光光谱法研究各种 DNA 系统,范围从单体核苷碱到双链和四链结构。我们工作的特异性在于将稳态荧光光谱与飞秒至纳秒时间尺度上记录的时间分辨数据定量关联起来,这是通过开发特定方法实现的。除其他外,我们的荧光研究提供了关于电子跃迁能量和偏振的信息。这些对于复杂系统中电子激发的演变是有价值的指标,其中发色团之间的电子耦合起着关键作用。强调源自 DNA 多聚体中电子相互作用的集体效应是本报告的目的。与荧光寿命在几皮秒内的单体发色团不同,DNA 多聚体的荧光持续时间在纳秒范围内。即使长寿命状态仅代表电子激发的一小部分,但由于核酸的连续结构动力学,它们可能对 DNA 的光反应至关重要,因为随着时间的推移,达到反应性构象的概率会增加。我们的飞秒研究表明,在双链体和 G-四联体中,碱基之间会发生超快的激发能量转移。当直接在光子吸收时填充集体态时,就可以实现这种超快过程。在更长的时间内,我们发现了一种出乎意料的长寿命高能发射,这种发射源于我们所谓的“HELM 激子”。这些集体态的发射随双链体尺寸的增加而增加,可能是导致基因组 DNA 观察到的延迟荧光的原因。大多数涉及 DNA 中激发态弛豫的研究都是在 260nm 左右的吸收带峰值处进行激发的。我们超越了这一点,并首次在 UVA 光谱范围内进行了时间分辨研究,其中存在非常弱的吸收尾。所得荧光衰减慢得多,荧光量子产率比 UVC 激发高得多。我们表明,DNA 链的碱基配对增强了 UVA 荧光,并同时增加了光反应性,因为它改变了涉及的集体激发态的性质。