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分子方法在二氧化碳光催化还原制备太阳能燃料中的应用。

Molecular approaches to the photocatalytic reduction of carbon dioxide for solar fuels.

机构信息

Department of Chemistry, Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218, USA.

出版信息

Acc Chem Res. 2009 Dec 21;42(12):1983-94. doi: 10.1021/ar9001679.

DOI:10.1021/ar9001679
PMID:19928829
Abstract

The scientific community now agrees that the rise in atmospheric CO(2), the most abundant green house gas, comes from anthropogenic sources such as the burning of fossil fuels. This atmospheric rise in CO(2) results in global climate change. Therefore methods for photochemically transforming CO(2) into a source of fuel could offer an attractive way to decrease atmospheric concentrations. One way to accomplish this conversion is through the light-driven reduction of carbon dioxide to methane (CH(4(g))) or methanol (CH(3)OH((l))) with electrons and protons derived from water. Existing infrastructure already supports the delivery of natural gas and liquid fuels, which makes these possible CO(2) reduction products particularly appealing. This Account focuses on molecular approaches to photochemical CO(2) reduction in homogeneous solution. The reduction of CO(2) by one electron to form CO(2)(-) is highly unfavorable, having a formal reduction potential of -2.14 V vs SCE. Rapid reduction requires an overpotential of up to 0.6 V, due at least in part to the kinetic restrictions imposed by the structural difference between linear CO(2) and bent CO(2)(-). An alternative and more favorable pathway is to reduce CO(2) though proton-assisted multiple-electron transfer. The development of catalysts, redox mediators, or both that efficiently drive these reactions remains an important and active area of research. We divide these reactions into two class types. In Type I photocatalysis, a molecular light absorber and a transition metal catalyst work in concert. We also consider a special case of Type 1 photocatalysis, where a saturated hydrocarbon links the catalyst and the light absorber in a supramolecular compound. In Type II photocatalysis, the light absorber and the catalyst are the same molecule. In these reactions, transition-metal coordination compounds often serve as catalysts because they can absorb a significant portion of the solar spectrum and can promote activation of small molecules. This Account discusses four classes of transition-metal catalysts: (A) metal tetraaza-macrocyclic compounds; (B) supramolecular complexes; (C) metalloporphyrins and related metallomacrocycles; (D) Re(CO)(3)(bpy)X-based compounds where bpy = 2,2'-bipyridine. Carbon monoxide and formate are the primary CO(2) reduction products, and we also propose bicarbonate/carbonate production. For comprehensiveness, we briefly discuss hydrogen formation, a common side reaction that occurs concurrently with CO(2) reduction, though the details of that process are beyond the scope of this Account. It is our hope that drawing attention both to current mechanistic hypotheses and to the areas that are poorly understood will stimulate research that could one day provide an efficient solution to this global problem.

摘要

科学界现在一致认为,大气中二氧化碳(最丰富的温室气体)的增加来自于人为来源,如化石燃料的燃烧。这种大气中二氧化碳的增加导致了全球气候变化。因此,将二氧化碳光化学转化为燃料来源的方法可能提供了一种减少大气浓度的有吸引力的方法。实现这种转化的一种方法是通过用光驱动将二氧化碳还原为甲烷(CH(4(g)))或甲醇(CH(3)OH((l))),同时从水中获得电子和质子。现有的基础设施已经支持天然气和液体燃料的输送,这使得这些可能的二氧化碳还原产物特别有吸引力。本账户重点介绍均相溶液中二氧化碳光化学还原的分子方法。通过一个电子将二氧化碳还原为 CO(2)(-)是非常不利的,其形式还原电位为-2.14 V 对 SCE。由于至少部分原因是线性 CO(2)和弯曲 CO(2)(-)之间结构差异所施加的动力学限制,快速还原需要高达 0.6 V 的超电势。另一种更有利的途径是通过质子辅助多电子转移还原 CO(2)。开发能够有效驱动这些反应的催化剂、氧化还原介体或两者仍然是一个重要且活跃的研究领域。我们将这些反应分为两类。在 I 型光催化中,分子光吸收剂和过渡金属催化剂协同工作。我们还考虑了 I 型光催化的一个特殊情况,其中饱和烃将催化剂和光吸收剂连接在超分子化合物中。在 II 型光催化中,光吸收剂和催化剂是同一分子。在这些反应中,过渡金属配合物通常用作催化剂,因为它们可以吸收太阳光谱的很大一部分,并可以促进小分子的激活。本账户讨论了四类过渡金属催化剂:(A)金属四氮杂大环化合物;(B)超分子配合物;(C)金属卟啉和相关金属大环;(D)基于 Re(CO)(3)(bpy)X 的化合物,其中 bpy = 2,2'-联吡啶。一氧化碳和甲酸盐是 CO(2)还原的主要产物,我们还提出了碳酸氢盐/碳酸盐的产生。为了全面起见,我们简要讨论了氢气的形成,这是与 CO(2)还原同时发生的常见副反应,尽管该过程的细节超出了本账户的范围。我们希望引起人们对当前的机制假设和理解不足的领域的关注,这将激发研究,有朝一日可能为这个全球性问题提供一个有效的解决方案。

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