論文

査読有り
2014年7月

Stabilizing conditions of metal mercury in mercury sulfurization using a planetary ball mill

JOURNAL OF HAZARDOUS MATERIALS
  • Naomichi Fukuda
  • ,
  • Masaki Takaoka
  • ,
  • Kazuyuki Oshita
  • ,
  • Tadao Mizuno

276
開始ページ
433
終了ページ
441
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.jhazmat.2014.04.063
出版者・発行元
ELSEVIER SCIENCE BV

This study used a non-heating process to stabilize mercury by mercury sulfurization. Elemental mercury and sulfur were mixed using planetary ball milling under various experimental conditions and the optimal conditions were determined. The labile intermediate, mercury sulfide, was observed in the early stages of milling, and the intermediates were then pulverized into mercury sulfide powder. These phenomena were significantly influenced by the diameter of the planetary ball. A larger diameter enhanced mercury stabilization. For a ball with a 19.04-mm diameter, the toxicity characteristic leaching procedure (TCLP) and the Japanese leaching test (JLT) values were 0.263 mu g/L and 0.0586 mu g/L, respectively, suggesting that mercury leachability was strictly controlled. When the molar ratio of sulfur to mercury was 1.05, the mercury concentration in the headspace was <1 mu g/Nm(3) at 20 degrees C, which was equivalent to the level in pure reagent. The stability of the planetary ball milling product at optimum conditions was either comparable or superior to that in other stabilization techniques. The running cost of this technology was estimated to be 15,360 Yen (154 USD)/ton-Hg. This stabilization technology is cost-effective and environmentally sound for the long-term and safe management of mercury. (C) 2014 Elsevier B.V. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/j.jhazmat.2014.04.063
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000339692700052&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.jhazmat.2014.04.063
  • ISSN : 0304-3894
  • eISSN : 1873-3336
  • Web of Science ID : WOS:000339692700052

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