論文

査読有り
2017年5月

Vapor-phase elemental mercury adsorption by activated carbon co-impregnated with sulfur and chlorine

CHEMICAL ENGINEERING JOURNAL
  • Akira Sano
  • ,
  • Masaki Takaoka
  • ,
  • Kenji Shiota

315
1
開始ページ
598
終了ページ
607
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.cej.2017.01.035
出版者・発行元
ELSEVIER SCIENCE SA

In this study, a novel activated carbon appropriate for mercury (Hg) removal from flue gas was developed by co-impregnation with chlorine (CI) and sulfur (S). The adsorption performance was investigated through laboratory-scale Hg adsorption tests. Additionally, changes in the chemical species on activated carbon with Hg adsorption were clarified by the X-ray absorption near edge structure (XANES) spectra of Hg, Cl, and S edges. CI impregnation and S impregnation resulted in 80 and 50 times greater Hg adsorption than raw activated carbon, respectively. Calcium chloride and potassium sulfide were effective impregnants for the Hg removal. Co-impregnation with both Cl and S resulted in over 200 times greater Hg adsorption than that with raw activated carbon. The results show clearly that co-impregnation is a remarkably effective method for Hg adsorption. The XANES spectra of CI revealed that calcium chloride and potassium chloride were immobilized on co-impregnated activated carbon, while the XANES spectra of S showed that sulfide and sulfate were immobilized on co-impregnated activated carbon. Hg was captured mainly as a chemical species of S during Hg adsorption by co-impregnated activated carbons. The Hg species estimated from XANES spectra were consistent with the possible reaction formulae during impregnation and adsorption processes. (C) 2017 Elsevier B.V. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/j.cej.2017.01.035
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000395212300060&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.cej.2017.01.035
  • ISSN : 1385-8947
  • eISSN : 1873-3212
  • Web of Science ID : WOS:000395212300060

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