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Photogenerated Charge Carriers and Paramagnetic Species in (W,N)-Codoped TiO2 Photocatalysts under Visible-Light Irradiation: An EPR Study
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文摘
(W,N)-codoped TiO2 has recently attracted interest due to substantial band gap narrowing in conjunction with good visible-light photocatalytic activities. A complete picture of the fundamental mechanism at the origin of their photoactivity is, however, far from being understood. We present an EPR study on (W,N)-codoped titanias by recording spectra in the dark and under 550 nm visible-light irradiation to identify the major species involved in the formation and migration of photogenerated charge carriers. Interstitial N鈥搇attice O (formally NO2鈥?/sup>) paramagnetic groups with and without a specific close range coupling interaction with a neighboring W, that is, [NiO]W鈼?/sup> and [NiO]鈼?/sup>, respectively, are observed when visible light excites electrons from diamagnetic intraband gap states located at 2.30 V versus RHE (formally NO3鈥?/sup>) to the conductance band at around 鈭?.05 V versus RHE. The [NiO]W鈼?/sup> EPR signal, reported here for the first time, is characterized by a much stronger hyperfine interaction between the unpaired electron and the 14N nucleus than ordinary [NiO]鈼?/sup> found in N-doped TiO2, leading to a much higher spin density on the N center. The overall signal also contains superhyperfine coupling of the unpaired electron with the 183W nuclide (natural abundance 14.31%), the only naturally occurring nuclide of W with a nonzero nuclear spin.

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