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  4. Spectral dependence of the magnetic modulation of surface plasmon polaritons in noble/ferromagnetic/noble metal films

Spectral dependence of the magnetic modulation of surface plasmon polaritons in noble/ferromagnetic/noble metal films

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Author(s)
Temnov, Vasily V.
•
Armelles, Gaspar
•
Bratschitsch, Rudolf
•
Leitenstorfer, Alfred
•
Martin-Becerra, Diana
•
Thomay, Tim
•
Garcia-Martin, Antonio
•
González, María Ujué
Date Issued
July 2012
Journal
Physical Review B
Publisher
American Physical Society
Citation
Martín-Becerra, Diana et al. “Spectral Dependence of the Magnetic Modulation of Surface Plasmon Polaritons in Noble/ferromagnetic/noble Metal Films.” Physical Review B 86.3 (2012): 035118. © 2012 American Physical Society.
Version
Final published version
Abstract
The magnetic field is an interesting candidate for the development of active plasmonic devices as it is able to modify the surface plasmon polariton (SPP) wave vector. Both real and imaginary parts of the SPP wave vector are affected. Here, we have experimentally determined the contribution of both modulations in the spectral range λ[subscript 0]=500–1000 nm for magnetoplasmonic systems consisting of noble/ferromagnetic/noble multilayered metal films. We have seen that the real part usually exceeds the imaginary one, but in the longer wavelength range the contribution of the imaginary part cannot be neglected. We have analyzed the spectral dependency of the modulation, and we conclude that it is dominated by the evolution of the SPP properties with wavelength and not the magneto-optical parameter. A figure of merit including modulation and propagation distance is also studied for the three ferromagnetic metals, Fe, Co, and Ni.
MIT Department
Massachusetts Institute of Technology. Department of Chemistry
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/72207
DOI of Published Version
https://doi.org/10.1103/PhysRevB.86.035118
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