“…As pH values shifted from 8.0 to 6.2, the Au 25 (pMBA) 18 showed monodispersed single‐cluster distribution with HDs stably controlled at approximately 2.4 nm, indicating that the enhanced emission of Au 25 (pMBA) 18 was originated from the intra‐cluster interaction after partial protonation of carboxyl group at pH 6.2 with decreased electrostatic repulsion. However, with the continued pH value decrease from 6.2 to 5.8, 5.0 and 4.0, the HDs of Au 25 (pMBA) 18 significantly increased from 2.5±0.4 nm to 7.5±1.5 nm, 46.8±9.9 nm, and 1833±366 nm, respectively, while the emission of Au 25 (pMBA) 18 quenched significantly at low pH values (e.g., 5.8 and 4.0), demonstrating that the inter‐cluster interactions of Au 25 (pMBA) 18 occurred to form large aggregates through both π–π stacking and hydrogen bonding interaction [18] . While the emission increase was highly corresponding to the intra‐cluster interactions within one single cluster with well‐maintained low HDs (approximately 2.4 nm) at the pH range from 8.0 to 6.2 (Figure 1E), the emission quenching was resulting from the inter‐cluster interactions among the Au 25 (pMBA) 18 with extremely increased HDs (from 2.5±0.4 nm to 1833±366 nm) at low pH values from 6.2 to 4.0.…”