“…[61] The use of dispersion corrections and the TZVP basis is well justified for the modeling of interactions on graphene surfaces. [68][69][70] Because the carbonaceous material is one of the main constituents of interstellar grains, a surface model, such as Cor (C 24 H 12 ), [3,4] which has been used to simulate graphite, graphene, and PAH interstellar grains, was used as a model. This molecule, shown in Figure 1A, has been widely used for several authors [23][24][25]27,29,30,32,36,50,[71][72][73][74][75][76][77][78] and for our group [21,41,42,61] as a PAH model of ISM.…”