論文

査読有り
2002年12月

Enhancement of optical absorption and photocurrents in solar cells of merocyanine Langmuir-Blodgett films utilizing surface plasmon excitations

MATERIALS SCIENCE & ENGINEERING C-BIOMIMETIC AND SUPRAMOLECULAR SYSTEMS
  • K Kato
  • ,
  • H Tsuruta
  • ,
  • T Ebe
  • ,
  • K Shinbo
  • ,
  • F Kaneko
  • ,
  • T Wakamatsu

22
2
開始ページ
251
終了ページ
256
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/S0928-4931(02)00174-1
出版者・発行元
ELSEVIER SCIENCE BV

Short-circuit photocurrents (I-SC) due to surface plasmon (SP) excitations were investigated for the solar cells using Langmuir-Blodgett (LB) films of merocyanine (MC) dye molecules. The Schottky photoelectric devices with two kinds of structures, that is, prism/Al/MC LB film/Ag (type A) and prism/MgF2/AlMC LB film/Ag (type B) were prepared. Type A has the Kretschmann configuration and type B has both the Kretschmann and the Otto configurations. In the attenuated total reflection (ATR) measurements, SPs were resonantly excited at the interface between Ag and air for type A and at the interfaces between MgF2 and Al and between Ag and air for type B. The ATR and I-SC properties were simultaneously measured as a function of the incident angles of the laser beams. The peaks of I-SC corresponded to the resonant angles of the ATR curves. The electric fields and optical absorption in the cells were also estimated. The calculated absorption in the MC layers as a function of the incident angles corresponded to the I-SC curves. The optical absorption in the MC layers turns out to be correlated directly to the profiles of I-SC. It was estimated that I-SC could be enhanced by the excitations of SPs in the ATR configurations. (C) 2002 Elsevier Science B.V. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/S0928-4931(02)00174-1
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000179929800025&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/S0928-4931(02)00174-1
  • ISSN : 0928-4931
  • Web of Science ID : WOS:000179929800025

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