Copper Deposited on Reduced Titania as Catalyst for the Production of CH4 from Sunlight and Air

Author:

Ali Shahzad12ORCID,Kim Dongyun1,Gong Eunhee1,Lee Junho1,Razzaq Abdul2,Lei Juying3,Kim Ki‐Jeong4,Goddard William A.5,In Su‐Il15ORCID

Affiliation:

1. Department of Energy Science & Engineering DGIST 333 Techno Jungangdaero, Hyeonpung-eup, Dalseong-gun Daegu 42988 Republic of Korea

2. Department of Chemical Engineering COMSATS University Islamabad, Lahore Campus 1.5 KM Defense Road, Off Raiwind Road Lahore 54000 Pakistan

3. School of Resources and Environmental Engineering East China University of Science and Technology, Shanghai 130 Meilong Road Shanghai P.R. China 200237

4. Beamline Research Division Pohang Accelerator Laboratory (PAL) Pohang 37673 Republic of Korea

5. Materials and Process Simulation Center California Institute of Technology Pasadena California 91125 United States

Abstract

AbstractAtmospheric CO2 and H2O adsorbed on the photocatalyst surface undergo sunlight‐assisted conversion to solar products that bridge the gaps between artificial and natural photosynthesis. Herein, we report a Lewis acid‐base interaction derived photocatalyst, Cu deposited on reduced titania, that harvests CO2 and H2O from the air and transforms them to CH4. Photocatalyst surface studies confirm that coordinately unsaturated Cu atoms and oxygen vacancies are formed that facilitate CO2 and H2O adsorption. The mechanistic studies, combined with tandem secondary ion mass spectroscopy and isotopic labelling, confirm the CH4 origin from atmosphere‐adsorbed CO2 and H2O. The contributing factors to photocatalyst instability are explored. We expect that this study will have an impact on the widespread application and economic viability of photocatalytic CO2 reduction.

Publisher

Wiley

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