論文

査読有り
2017年4月

Ion Distribution and Hydration Structure in the Stern Layer on Muscovite Surface

LANGMUIR
  • Kazuya Kobayashi
  • ,
  • Yunfeng Liang
  • ,
  • Sumihiko Murata
  • ,
  • Toshifumi Matsuoka
  • ,
  • Satoru Takahashi
  • ,
  • Naoya Nishi
  • ,
  • Tetsuo Sakka

33
15
開始ページ
3892
終了ページ
3899
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1021/acs.langmuir.7b00436
出版者・発行元
AMER CHEMICAL SOC

Based on molecular dynamics simulations of eight ions (Na+, K+, Rb+, Cs+, Mg2+, Ca2+, Sr2+, and Ba2+) on muscovite mica surfaces in water, we demonstrate that experimental data on the muscovite mica surface can be rationalized through a unified picture of adsorption structures including the hydration structure, cation heights from the muscovite surface, and state stability. These simulations enable us to categorize the inner-sphere surface complex into two different species: an inner-sphere surface complex in a ditrigonal cavity (IS1) and that on top of Al (IS2). By considering the presence of the two inner-sphere surface complexes, the experimental finding that the heights of adsorbed cations from the muscovite surface are proportional to the ionic radius for K+ and Cs+ but inversely proportional to the ionic radius for Ca2+ and Ba2+ was explained. We find that Na+, Ca2+, Sr2+, and Ba2+ can form both IS1 and 1S2; Rb+, and Cs+ can form only IS1; and Mg2+ can form only IS2. It is suggested that the formation of IS1 and IS2 is governed by the charge density of the ions. Among the eight ions, we also find that the hydration structure for the outer-sphere surface complexes of divalent cations differs from that of the monovalent cations by one adsorbed water molecule (i.e., a water molecule located in a ditrigonal cavity).

リンク情報
DOI
https://doi.org/10.1021/acs.langmuir.7b00436
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000399860000038&DestApp=WOS_CPL
ID情報
  • DOI : 10.1021/acs.langmuir.7b00436
  • ISSN : 0743-7463
  • Web of Science ID : WOS:000399860000038

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