UC Irvine UC Irvine Previously Published Works
Title Introduction: Plasmonics and its building blocks
Permalink https://escholarship.org/uc/item/2dt6b3p1
Author Maradudin, AA
Publication Date 2014
DOI 10.1016/B978-0-444-59526-3.00001-X
License https://creativecommons.org/licenses/by/4.0/ 4.0
Peer reviewed
eScholarship.org Powered by the California Digital Library University of California CHAPTER Introduction: Plasmonics and its Building Blocks 1 Alexei A. Maradudin Research Professor, Physics and Astronomy School of Physical Sciences, University of California, Irvine, CA, USA
Plasmonics is the area at the intersection of science and technology in which the interaction of light with matter is mediated by surface electromagnetic excitations at a dielectric-metal interface—surface plasmon polaritons and localized surface plasmons. These excitations are collective oscillations of the electrons in the vicinity of a planar vacuum-metal interface, or in a metallic particle with nanoscale dimensions. They can be generated by illuminating a suitably designed dielectric-metal interface by light. The frequency of the resulting excitations can be made to match that of the incident light, but their wave- length can be significantly shorter. The electromagnetic fields of these excitations are localized to well within a wavelength of the interface, with the result that their excitation produces a significant enhance- ment of the electromagnetic field in the immediate vicinity of the interface. All of these features of surface plasmon polaritons and localized surface plasmons have made them attractive candidates for incorpora- tion into devices for information processing and transmission, and biochemical sensing, that are faster and smaller than existing photonics devices, and faster and at least comparable in size to their electronic counterparts. Thus, they can bridge the size gap between photonics and microelectronic devices. In this chapter we present an overview of the building blocks of plasmonics, surface plasmon polari- tons, and localized surface plasmons, and describe some of their properties that are interesting from a basic science standpoint, and from the potential they show for, or have already shown in, applications. It is intended to serve as an introduction to topics that will be discussed in much greater detail in the remaining chapters of this book.
1.1 Surface Plasmon Polaritons A surface plasmon polariton is an electromagnetic wave that, in its simplest form, propagates along the planar interface between a dielectric and a metal with an amplitude that decays exponentially with increasing distance into each medium from the interface. If the metal is lossy, the amplitude of this wave also decreases exponentially in the direction of its propagation. Such surface electromagnetic waves were first discussed by Zenneck in 1907 [1.1] who showed that Maxwell’s equations together with the corresponding boundary conditions admit a solution that is a surface wave. The electric field of this wave is p polarized (TM polarized), i.e. its magnetic vector is per- pendicular to the sagittal plane, namely the plane defined by the direction of propagation of the wave and the normal to the surface. In the case that the dielectric medium, characterized by a real positive dielectric Modern Plasmonics. http://dx.doi.org/10.1016/B978-0-444-59526-3.00001-X 1 © 2014 Elsevier B.V. All rights reserved. 2 CHAPTER 1 Introduction: Plasmonics and its Building Blocks
constant 0 occupies the half space x3 > 0, and is in contact across the plane x3 = 0 with a medium characterized by a frequency-dependent dielectric function (ω)that occupies the half space x3 < 0, the nonzero component of the magnetic field of this wave propagating in the x1 direction can be written as
H2(x1, x3|ω) = exp[ikx1 − β0x3] x3 > 0, (1.1a) = exp[ikx1 + βx3] x3 < 0. (1.1b)
A time dependence exp (−iωt) has been assumed in writing this field, but is not indicated explicitly. The functions β0 and β, the inverse decay lengths of the field into the medium with 0 and the medium with , respectively, are given by
1 2 2 2 β0 = k − 0(ω/c) , (1.2a)
1 β = k2 − (ω)(ω/c)2 2 , (1.2b) where ω is the frequency of the wave. From the boundary conditions on the field at the interface x3 = 0 the wavenumber k is found to be 1 ω (ω) 2 k(ω) = 0 . (1.3) c 0 + (ω) When this result is substituted into the expressions (1.2a) and (1.2b) for the inverse decay lengths, the latter become
1 ω − 2 2 0 β0(ω) = , (1.4a) c 0 + (ω) 1 ω − 2(ω) 2 β(ω) = . (1.4b) c 0 + (ω)
If the preceding results are to describe a surface wave, we see from Eq. (1.1) that Reβ0 and Reβ must both be positive. This is generally achieved in one of two ways. We can assume that (ω) is real and negative. For historical reasons that will be discussed below, the resulting surface electromagnetic wave has become known as a Fano mode. Its phase velocity is smaller than the speed of light in the dielectric medium with the dielectric constant 0. Alternatively, we can assume that (ω) is complex, (ω) = 1(ω) + i 2(ω) with an imaginary part 2(ω) that is non-negative. In this case we find from Eq. (1.3) that the wavenumber k(ω) is now complex, k(ω) = k1(ω) + ik2(ω), where both k1(ω) and k2(ω) are real. The energy propagation length of the resulting surface wave is then given by
−1 (ω) = (2k2(ω)) . (1.5)
There are now two cases to consider. In the case of a weakly lossy medium for which