dc.contributor.authors |
Guy, N; Atacan, K; Karaca, E; Ozacar, M; |
|
dc.date.accessioned |
2020-02-24T14:20:20Z |
|
dc.date.available |
2020-02-24T14:20:20Z |
|
dc.date.issued |
2018 |
|
dc.identifier.citation |
Guy, N; Atacan, K; Karaca, E; Ozacar, M; (2018). Role of Ag3PO4 and Fe3O4 on the photocatalytic performance of magnetic Ag3PO4/ZnO/Fe3O4 nanocomposite under visible light irradiation. SOLAR ENERGY, 166, 316-308 |
|
dc.identifier.issn |
0038-092X |
|
dc.identifier.uri |
https://doi.org/10.1016/j.solener.2018.03.045 |
|
dc.identifier.uri |
https://hdl.handle.net/20.500.12619/45229 |
|
dc.description.abstract |
Novel magnetically separable nanocomposite photocatalyst Ag3PO4/ZnO/Fe3O4, prepared by the coprecipitation and microwave assisted hydrothermal synthesis, was first investigated as the photocatalyst for congo red degradation under visible light. The nano photocatalysts were systematically characterized with by X-ray diffraction (XRD), scanning electron microscopy (SEM), Fourier transform infrared spectroscopy (ATR-FTIR), vibrational sample magnetometer (VSM) measurements and UV-vis diffuse reflectance/absorbance spectroscopy (DRS). The nanocomposite Ag3PO4/ZnO/Fe3O4 showed enhanced photocatalytic activity compared with ZnO, ZnO/Fe3O4, Ag3PO4/ZnO under the same conditions. The reasons for the highly increased activity of Ag3PO4/ZnO/Fe3O4 are that it allows more visible light absorption and efficient delaying the recombination of charge carriers. Also, the degradation efficiency for congo red is about 97.0% for the Ag3PO4/ZnO/Fe3O4 nanocomposite in the 90 min. At the end of the successful degradation process, the obtained magnetic photocatalyst was effectively separated from the suspension by applying external magnetic field. |
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dc.language |
English |
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dc.publisher |
PERGAMON-ELSEVIER SCIENCE LTD |
|
dc.subject |
Energy & Fuels |
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dc.title |
Role of Ag3PO4 and Fe3O4 on the photocatalytic performance of magnetic Ag3PO4/ZnO/Fe3O4 nanocomposite under visible light irradiation |
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dc.type |
Article |
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dc.identifier.volume |
166 |
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dc.identifier.startpage |
308 |
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dc.identifier.endpage |
316 |
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dc.contributor.department |
Sakarya Üniversitesi/Fen-Edebiyat Fakültesi/Kimya Bölümü |
|
dc.contributor.saüauthor |
Güy, Nuray |
|
dc.contributor.saüauthor |
Atacan, Keziban |
|
dc.contributor.saüauthor |
Karaca, Ertuğrul |
|
dc.contributor.saüauthor |
Özacar, Mahmut |
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dc.relation.journal |
SOLAR ENERGY |
|
dc.identifier.wos |
WOS:000432235100031 |
|
dc.identifier.doi |
10.1016/j.solener.2018.03.045 |
|
dc.contributor.author |
Güy, Nuray |
|
dc.contributor.author |
Atacan, Keziban |
|
dc.contributor.author |
Karaca, Ertuğrul |
|
dc.contributor.author |
Özacar, Mahmut |
|