Strong hybridization between Bi-6s and O-2p orbitals in Sillén–Aurivillius perovskite Bi 4 MO 8 X (M = Nb, Ta; X = Cl, Br), visible light photocatalysts enabling stable water oxidation

Bi 4 NbO 8 Cl with a Sillén–Aurivillius type perovskite structure has recently been demonstrated to stably and efficiently oxidize water under visible light, possibly related to its unique valence band with O-2p orbitals located at unusually high potentials compared with conventional oxides. Here we...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Journal of materials chemistry. A, Materials for energy and sustainability Materials for energy and sustainability, 2018, Vol.6 (7), p.3100-3107
Hauptverfasser: Kunioku, Hironobu, Higashi, Masanobu, Tomita, Osamu, Yabuuchi, Masayoshi, Kato, Daichi, Fujito, Hironori, Kageyama, Hiroshi, Abe, Ryu
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:Bi 4 NbO 8 Cl with a Sillén–Aurivillius type perovskite structure has recently been demonstrated to stably and efficiently oxidize water under visible light, possibly related to its unique valence band with O-2p orbitals located at unusually high potentials compared with conventional oxides. Here we study a series of isostructural oxyhalides, Bi 4 MO 8 X (M = Nb, Ta; X = Cl, Br), to examine how the cation and anion substitution affects the band structure and the resultant photocatalytic activity. We found experimentally and theoretically that both M and X substitutions have little influence on the electronic structures, providing similar valence band maximums (VBMs) and band gaps to those of Bi 4 NbO 8 Cl. They all functioned as stable O 2 -evolving photocatalysts under visible light without suffering from self-oxidative deactivation, as opposed to BiOBr. DFT calculations further revealed a fairly strong hybridization between the Bi-6s orbitals and the O-2p orbitals, which is interpreted using a revised lone pair (RLP) model, thus explaining at least partly why the O-2p orbitals are elevated in energy.
ISSN:2050-7488
2050-7496
DOI:10.1039/C7TA08619A