“…Here, we note that a distortion effect of the PBI core is negligible since the twist of gPBI-CP (23.1°) lies between hitherto reported PBI dimers (0° for orange PBI dimer and 27° for rPBI-CP ) showing the excimer formation (Table S2). A photoexcited rPBI-CP exhibits the broad ESA band covering 600–950 nm, which is characteristic of the excimer, as shown in Figure a . Especially, except for a minor increase at 610–640 nm (Figure b), the overall shape of ESA retains its spectral characteristics during excimer formation ( k = 200 fs –1 ). ,,,− By contrast, the TA spectra of gPBI-CP show a prominent increase with a time constant of ∼180 fs in the ESA band (∼825 nm), corresponding to the radical anionic band, in both TOL and BCN (Figures c,d and S27).…”