New composite materials based on g-C3N4 loaded with Copper(I) oxalate as promoters of C-C coupling in CO2-H2O co-processing under solar irradiation

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Authors: Michele Aresta, Domenico Caringella, Ernesto Mesto, Christopher Habu, Angela Dibenedetto
Cited by: 1
References: 30

Abstract

New composites made of copper(I)oxalate mixed with g-C 3 N 4 by High Energy Milling (HEM) (at 800 rpm) in various w/w percentage (10, 20, 50 % w/w) and for different milling times (30–90 min) are shown to be active as gas-phase photocatalysts in coprocessing “CO 2 and H 2 O” under solar irradiation (0.1 W cm −2 ) at room temperature to afford ethene or acetone in the range of 20–50 μmol g −1 h −1 . The materials have been characterized by UV–VIS DRS, FTIR, elemental analyses, XRD, SEM, Band-gap and chopped photocurrent. The CO2RPs have been identified through GC, GC-MS and multinuclear NMR. Materials have been tested for over 15 h in gas-phase photochemical reactions and shown to be stable towards: the exchange with 13 CO 2 , used to exclude “false positives”, disproportionation to afford CO and CO 3 2- , and oxalate anion reduction. Cu(I)-oxalate modifies the properties of g-C 3 N 4 and most likely is even implied in C-C coupling, as the Cu-Cu distance (255 pm, as determined by XRD in this work) is suited for promoting C-C coupling and is kept constant during operation by the backbone-action of the oxalate anion, which avoids Cu-centres random distribution, that would cause C-C coupling regression. • Cu(I)oxalate is shown to be able to modify the photoelectronic properties of g-C 3 N 4 • The oxalate dianion acts as a backbone for the two Cu(I) centres. • The Cu-Cu distance in the twin-set is kept at 255 pm. • The new composite induces the C-C coupling in CO 2 -H 2 O coprocessing under solar light.

Fields of Study & Subjects

Advanced Photocatalysis Techniques CO2 Reduction Techniques and Catalysts TiO2 Photocatalysis and Solar Cells

Publication details

Journal / source
Journal of CO2 Utilization
Publisher
Elsevier BV
Volume
104
Pages
103317–103317
Publication date
10 January 2026
Language
EN