Observation of a hole-size-dependent energy shift of the surface-plasmon resonance in Ni antidot thin films
Author(s) -
Hui Fang,
Blanca Caballero,
Eser Metin Akinoglu,
Evangelos Th. Papaioannou,
Antonio GarcíaMartín,
Juan Carlos Cuevas,
Michael Giersig,
P. Fumagalli
Publication year - 2015
Publication title -
applied physics letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.182
H-Index - 442
eISSN - 1077-3118
pISSN - 0003-6951
DOI - 10.1063/1.4917513
Subject(s) - nickel , thin film , surface plasmon resonance , materials science , condensed matter physics , polar , surface plasmon , plasmon , kerr effect , dielectric , blueshift , photon energy , photon , molecular physics , optics , physics , optoelectronics , nanotechnology , nanoparticle , nonlinear system , astronomy , quantum mechanics , metallurgy , photoluminescence
A combined experimental and theoretical study of the magneto-optic properties of a series of nickel antidot thin films is presented. The hole diameter varies from 869 down to 636 nm, while the lattice periodicity is fixed at 920 nm. This results in an overall increase of the polar Kerr rotation with decreasing hole diameter due to the increasing surface coverage with nickel. In addition, at photon energies of 2.7 and 3.3 eV, where surface-plasmon excitations are expected, we observe distinct features in the polar Kerr rotation not present in continuous nickel films. The spectral position of the peaks exhibits a red shift with decreasing hole size. This is explained within the context of an effective medium theory by a change in the effective dielectric function of the Ni thin filmsH.F. gratefully acknowledges China Scholarship Council (CSC) for financial support and André Schirmeisen for the data of Ni film. A.G.-M. and B.C. acknowledge funding from Spanish Ministry of Economy and Competitiveness through grants “FUNCOAT” CONSOLIDER CSD2008-00023 and “MAPS” MAT2011-29194-C02-01. J.C.C. acknowledges financial support from the Spanish Ministry of Economy and Competitiveness (Contract No. FIS2011-28851-C02-01) and from the Comunidad de Madrid (Contract No. S2013/MIT- 2740). E.M.A. and M.G. acknowledge financial support by the European Union under the project CosmoPHOS with the number “310337
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