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WO3/g-C3N4复合光催化剂制备及其可见光催化性能
引用本文:黄有鹏,吴福礼,李兵,杨本宏. WO3/g-C3N4复合光催化剂制备及其可见光催化性能[J]. 复合材料学报, 2021, 38(12): 4265-4272. DOI: 10.13801/j.cnki.fhclxb.20210303.001
作者姓名:黄有鹏  吴福礼  李兵  杨本宏
作者单位:1.合肥学院 生物食品与环境学院,合肥 230601
基金项目:国家自然科学基金(51403048);合肥学院研究生创新研究项目(CX201906)
摘    要:将自制层状石墨相氮化碳(g-C3N4)和WO3纳米片均匀混合,经煅烧制备WO3/g-C3N4复合半导体。利用XRD、SEM、TEM、UV-Vis DRS和PL对其进行表征。结果表明,g-C3N4呈现类石墨烯状片层结构,WO3为纳米片状结构,且分散在g-C3N4表面;与WO3复合后,UV-Vis吸收边发生了红移,拓宽了g-C3N4对可见光的响应。以罗丹明B(RhB)为模拟污染物,考察WO3/g-C3N4的光催化降解性能。WO3/g-C3N4质量比为1∶5时,表现出最佳的光催化活性,可见光照60 min后,RhB降解率可达到94.9%。光催化剂具有良好的稳定性,重复使用6次后,RhB的降解率依然达到88.9%。光催化机制研究表明,超氧自由基(·O2?)是光催化降解RhB的主要活性物种。 

关 键 词:WO3/g-C3N4   复合半导体   罗丹明B   光催化降解   纳米片
收稿时间:2020-12-09

Preparation and visible light catalytic performance of WO3/g-C3N4 composite photocatalyst
Affiliation:1.School of Biology Food and Environmental Engineering, Hefei University, Hefei 230601, China2.School of Energy Materials and Chemical Engineering, Hefei University, Hefei 230601, China
Abstract:The WO3/graphite phase carbon nitride (g-C3N4) composites were prepared by mixing self-made layered g-C3N4 with WO3 nanoplates and afterward calcination process, and were characterized by XRD, SEM, TEM, UV-Vis DRS and PL. The results show that g-C3N4 presents graphene-like layered structure, and WO3 indicates nanoplate structure, and scatters on the surfaces of g-C3N4. After compounding with WO3, the absorption edge of UV-Vis spectrum shifts to red, which widens the response of g-C3N4 to visible light. The photocatalytic degradation properties of WO3/g-C3N4 were examined using rodamine B (RhB) as a simulated pollutant. When the mass ratio of WO3/g-C3N4 is 1∶5, the best photocatalytic activity is obtained. After 60 min of visible light irradiation, the degradation rate of RhB can reach 94.9%. The photocatalyst shows good stability, as the photodegradation rate of RhB reaches 88.9% after repeated use of the same photocatalyst for 6 times. The study of photocatalytic mechanism shows that superoxide radical (·O2?) is the main active species for photocatalytic degradation of RhB. 
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