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Humic like substances for the treatment of scarcely soluble pollutants by mild photo-Fenton process

Humic-like substances (HLS) extracted from urban wastes have been tested as auxiliaries for the photo-Fenton removal of thiabendazole (TBZ) under simulated sunlight. Experimental design methodology based on Doehlert matrices was employed to check the effects of hydrogen peroxide concentration, HLS a...

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Bibliographic Details
Published in:Chemosphere (Oxford) 2018-05, Vol.198, p.139-146
Main Authors: Caram, Bruno, García-Ballesteros, Sara, Santos-Juanes, Lucas, Arques, Antonio, García-Einschlag, Fernando S.
Format: Article
Language:English
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Summary:Humic-like substances (HLS) extracted from urban wastes have been tested as auxiliaries for the photo-Fenton removal of thiabendazole (TBZ) under simulated sunlight. Experimental design methodology based on Doehlert matrices was employed to check the effects of hydrogen peroxide concentration, HLS amount as well as TBZ loading; this last parameter was studied in the range 25–100 mg/L, to include values below and above the limit of solubility at pH = 5. Very satisfactory results were reached when TBZ was above solubility if HLS and H2O2 amounts were high. This could be attributed to an interaction of HLS-TBZ that enhances the solubility of the pollutant. Additional evidence supporting the latter interaction was obtained by fluorescence measurements (excitation emission matrices) and parallel factor analysis (PARAFAC). Humic-like substances extracted from urban wastes enhance photo-Fenton removal of scarcely soluble pollutants under UVA-visible irradiation. [Display omitted] •waste valorization as the humic-like substances are isolated from urban wastes.•Use of these substances in wastewater treatment.•UVA-visible light is used, and hence, it can be driven under real sunlight.•Extends the use of photo-Fenton towards circumneutral conditions (e.g. avoids acidification).•Prevents the use of surfactants to dissolve suspensions of non-soluble pollutants.
ISSN:0045-6535
1879-1298
DOI:10.1016/j.chemosphere.2018.01.074