“…The excited electron will be promoted from the ground state (highest occupied molecular orbital, HOMO) to a higher energy orbital (lowest unoccupied molecular orbital, LUMO) when the photon energy of the incident light matches a possible electronic transition within the molecule, causing heat to be released when the excited electron relaxes back to its ground state (Figure 3C). 7,75 Because of their high light absorption across a wide range of wavelengths, relatively low cost, and high stability, various carbon materials have been investigated as light absorbers for solar evaporation, such as biomass-derived amorphous carbon, 76 graphene, [77][78][79][80][81][82][83][84] graphene oxide (GO)/reduced graphene oxide (rGO), 39,[85][86][87][88][89][90] carbon nanotubes (CNTs), [91][92][93] graphite, 30,[94][95][96] carbon black, 97 etc. In addition, carbon materials can be easily fabricated into various structures desirable for enhanced light absorption and integrated with diverse substrate materials and evaporation structures.…”