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Illumina MiSeq sequencing reveals microbial community in HA process for dyeing wastewater treatment fed with different co-substrates.

Authors :
Xie, Xuehui
Liu, Na
Ping, Jing
Zhang, Qingyun
Zheng, Xiulin
Liu, Jianshe
Source :
Chemosphere. Jun2018, Vol. 201, p578-585. 8p.
Publication Year :
2018

Abstract

In present study, a hydrolysis acidification (HA) reactor was used for simulated dyeing wastewater treatment. Co-substrates included starch, glucose, sucrose, yeast extract (YE) and peptone were fed sequentially into the HA reactor to enhance the HA process effects. The performance of the HA reactor and the microbial community structure in HA process were investigated under different co-substrates conditions. Results showed that different co-substrates had different influences on the performance of HA reactor. The highest decolorization (50.64%) and COD removal rate (60.73%) of the HA reactor were obtained when sucrose was as the co-substrate. And it found that carbon co-substrates starch, glucose and sucrose exhibited better decolorization and higher COD removal efficiency of the HA reactor than the nitrogen co-substrates YE and peptone. Microbial community structure in the HA process was analyzed by Illumina MiSeq sequencing. Results revealed different co-substrates had different influences on the community structure and microbial diversity in HA process. It was considered that sucrose could enrich the species such as Raoultella , Desulfovibrio , Tolumonas , Clostridium , which might be capable of degrading the dyes. Sucrose was considered to be the best co-substrate of enhancing the HA reactor’s performance in this study. This work would provide deep insight into the influence of many different co-substrates on HA reactor performance and microbial communities in HA process. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00456535
Volume :
201
Database :
Academic Search Index
Journal :
Chemosphere
Publication Type :
Academic Journal
Accession number :
128804452
Full Text :
https://doi.org/10.1016/j.chemosphere.2018.03.025