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Thomas Wriedt - The Generalized Multipole Technique for Light Scattering

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Thomas Wriedt The Generalized Multipole Technique for Light Scattering
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Springer International Publishing AG, part of Springer Nature 2018
Thomas Wriedt and Yuri Eremin (eds.) The Generalized Multipole Technique for Light Scattering Springer Series on Atomic, Optical, and Plasma Physics
1. Principal Modes of Maxwells Equations
Ben Hourahine 1
(1)
SUPA, Department of Physics, University of Strathclyde, Glasgow, G4 0NG, UK
Ben Hourahine (Corresponding author)
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Duncan McArthur
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Francesco Papoff
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Abstract
This chapter reviews the use of principal modesstates which are maximally correlated between two subspaces and hence form pairs unique up to phase factorsin solving Maxwells equations and analysing these solutions for nanoparticles and structures. The mathematical structure of this method allows a computationally efficient generalisation of Mies analytical approach for the sphere to obtain semi-analytical solutions for general geometries with smooth interfaces. We apply this method to investigate a range of single and multiple particle metallic structures in the linear, non-linear and non-local response regimes outside of the quasi-static limit.
1.1 Introduction
The interaction of light with particles with similar or smaller dimensions than the incident wavelength has been intensely investigated for more than a century. New and interesting results continue to be discovered in this regime. This coupling is crucial in the spectroscopy of single molecules and for single and multi-photon processes []. All these effects are due to particle-light interaction, which depends on both the particles shape and composition and also the properties of the incident light. This interaction can become very strong, particularly around resonances. Understanding and controlling fundamental elements of this interaction are essential to design nanostructures with desirable near as well as far field optical responses.
In this chapter we review the theory of principal modes that we have developed over the last 10 years to describe single and multiple particle systems with smooth interfaces. We use the mathematical theory developed by Jordan [].
1.2 Principal Modes of Single Particles
The theory of principal modes can be applied to general particles and structures without sharp edges, this includes both metallic and dielectric particles. When all the characteristic dimensions of the particle (and the skin depth in the case of metallic particles) are larger than the free propagation length of charges, then in this regime local macroscopic permittivities and susceptibilities can describe the interaction between light and the matter inside the particle.
The wave energy scattered by a particle propagates outward towards infinity []; in the case of a local macroscopic permittivity and susceptibility, the tangential components, together with the radiation condition then fully determine the boundary conditions for valid solutions to Maxwells equations. Hence only the projections, f , of the six components of the field onto the boundary of the particle are required , since by construction the internal and external fields are regular and radiating Maxwell solutions. These surface fields have four components, two electric and two magnetic, and form a space, The Generalized Multipole Technique for Light Scattering - image 1 , with defined scalar products in terms of the overlap integrals on the surface of the particle,
The Generalized Multipole Technique for Light Scattering - image 2
(1.1)
where The Generalized Multipole Technique for Light Scattering - image 3 is the complex conjugate of field f , j labels the individual components and we sum over repeated indexes. In this notation the boundary conditions become
The Generalized Multipole Technique for Light Scattering - image 4
(1.2)
which can be interpreted geometrically in the Hilbert space Picture 5 : the projection, Picture 6 , of the incident field, Picture 7 at point x , onto the surface of the particle is equal to the difference between the projections of the internal and scattered fields, Picture 8 and Picture 9 . Therefore, an incident field having small values of the tangential components can then excite large amplitude internal and scattered surface fields, provided that both of these two fields closely match (i.e. they are nearly cancelling each other at the surface). This happens when the difference between these two fields, and therefore the angle between them, is small. These angles are rigorously defined as being between solutions of Maxwells equations for the internal and external media; where these solutions are themselves standing and outgoing waves, respectively, and form two subspaces of Picture 10 . The electromagnetic response of each particle is completely characterised by these angles and their associated waves, which can be calculated with arbitrary precision from any complete set of solutions of Maxwells equations for the internal and external media.
Several sets of exact solutions of the Maxwell equations are linearly independent and complete [] for which Gauss theorem applies.
We use two sets of electric and magnetic multipoles, The Generalized Multipole Technique for Light Scattering - image 11 and The Generalized Multipole Technique for Light Scattering - image 12 for the internal and scattered fields respectively. These are centred at points within the particle []. In other words, The Generalized Multipole Technique for Light Scattering - image 13 is complete and no function in this set is the closure of the linear combinations of all the remaining functions. We note that both the internal and scattered fields exist at the surface of real metallic and dielectric particles, i.e. the union of internal and scattered fields provides completeness in the space Picture 14 of surface fields of the type to which f belongs. Neither the scattered or the internal fields separately are complete. An example of this property is given by spherical particles, where both internal and scattered modes are necessary to form the complete basis of functions that underpins Mie theory .
For numerical applications, we could use any set of solutions for the Maxwell equations which satisfy the Silver-Mller radiation conditions [] .
One can show [] that the coefficients of the internal and scattered fields, that minimise the discrepancy between an incident field and the expansion of - photo 15
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