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Pressure-mediated crystalline g-C3N4 with enhanced spatial charge transport for solar H2 evolution and photocathodic protection of 304 stainless steels

Published 25 Jul 2025 in cond-mat.mtrl-sci | (2507.18914v1)

Abstract: Conjugated polymeric g-C3N4 has emerged as a leading semiconductor for solar-to-chemical energy conversion due to its unique electronic band structure, robust physicochemical stability, and environmental benignity. However, defect engineering-while effective at enhancing visible-light absorption and charge separation-often introduces excessive dangling bonds and lattice disorder, which exacerbate carrier recombination and impair light harvesting. High crystallinity offers a complementary route to improve spatial charge transport, yet strategies that concurrently optimize crystallinity and surface defects remain underexplored. Here we report a pressure-mediated ion thermal synthesis of high-crystalline g-C3N4 (CCN-P) using a NaCl/KCl eutectic salt under elevated pressure. The molten salt facilitates in-plane and cross-plane crystal growth, while applied pressure reduces interlayer spacing and shortens photocarrier pathways. This dual modulation yields CCN-P with balanced surface defects (-CN and -NHx), an electron-trapping resistance (Rtrap) of 11.36 k{\Omega} cm2 and a photocarrier decay rate constant of 0.013 s-1. CCN-P achieves a hydrogen evolution rate of 2168.8 {\mu}mol g-1 h-1 and delivers 78.5% dark photocathodic protection of 304 stainless steel over 7500 s, outperforming bulk and conventionally crystalline g-C3N4. This straightforward pressure-ion thermal approach provides a versatile platform for tailoring crystalline frameworks and defect distributions in polymeric semiconductors for efficient solar energy conversion.

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