“…1,7,12,13 Unfortunately, achieving efficient and long-lived RTP or afterglow is hindered by the spin-forbidden nature of triplet exciton transition, the rapid non-radiative decay of the triplet excitons, and proneness to quenching by oxygen and solvents. 2,14,15 To achieve efficient and long-lived RTP, many strategies have been proposed to promote the intersystem crossing (ISC) process and to stabilize the excitons at triplet states, such as introducing of heavy atoms, lone pair electrons, clusterization, host-guest interactions, crosslinking and matrix rigidification. 1,5,14,[16][17][18][19] Although these strategies have greatly improved the emission efficiencies and lifetime, most of the emission bands of organic afterglow materials located in the wavelength range from 500 to 600 nm, due to the bathochromic shifts and relatively low-lying exciton energies modulated by these strategies.…”