Abstract:A method for calculating the electromagnetic scattering for the truncation of the multipolar expansions describproperties of a cluster of spheres of arbitrary radii and ing the scattered field. The convergence of the expan-(possibly complex) refractive indexes is proposed. The sions is tested through the application to the simple but approach takes proper account of multiple scattering significant system of two spheres with varying interpareffects and does not require any approwinlation except ticle separation. Show more
“…Nevertheless, it will be advantageous to retain the sphere-centered formulation of the T matrix in formulating the orientation-averaged cross sections of the cluster. The representation of the scattered field from the cluster in a single expansion has been discussed by Borghese et al 3 and Mackowski. 8 The first step in the process is to identify an origin of the cluster.…”
Section: Nmentioning
confidence: 99%
“…Developed first by Brunning and Lo 2 and later independently obtained by Borghese et al, 3 this analysis constructs the scattered field from the cluster as a superposition of individual fields scattered from each of the spheres. The individual fields, in turn, are expressed in terms of expansions of vector spherical harmonics written about the origin of the sphere.…”
A method for calculating the extinction, absorption, and scattering cross sections of clusters of neighboring spheres for both fixed and random orientations is developed. The analysis employs the superposition formulation for radiative interactions among spheres, in which the total field from the cluster is expressed as a superposition of vector spherical harmonic expansions about each of the spheres in the cluster. Through the use of addition theorems a matrix equation for the expansion coefficients is obtained. Further application of addition theorems on the inverse of the coefficient matrix is shown to yield analytical expressions for the orientation-averaged total cross sections of the sphere cluster. Calculations of the cross sections of pairs of spheres and fractal aggregates of several spheres are presented. It is found that a dipole representation of the field in each sphere does not adequately predict the absorption cross section of clusters of small-size-parameter spheres when the spheres are highly conducting. For this situation several multipole orders are required for an accurate calculation of the absorption cross section. In addition, the predicted absorption of sphere clusters can be significantly greater than that estimated from the sum of the isolated-sphere cross sections.
“…Nevertheless, it will be advantageous to retain the sphere-centered formulation of the T matrix in formulating the orientation-averaged cross sections of the cluster. The representation of the scattered field from the cluster in a single expansion has been discussed by Borghese et al 3 and Mackowski. 8 The first step in the process is to identify an origin of the cluster.…”
Section: Nmentioning
confidence: 99%
“…Developed first by Brunning and Lo 2 and later independently obtained by Borghese et al, 3 this analysis constructs the scattered field from the cluster as a superposition of individual fields scattered from each of the spheres. The individual fields, in turn, are expressed in terms of expansions of vector spherical harmonics written about the origin of the sphere.…”
A method for calculating the extinction, absorption, and scattering cross sections of clusters of neighboring spheres for both fixed and random orientations is developed. The analysis employs the superposition formulation for radiative interactions among spheres, in which the total field from the cluster is expressed as a superposition of vector spherical harmonic expansions about each of the spheres in the cluster. Through the use of addition theorems a matrix equation for the expansion coefficients is obtained. Further application of addition theorems on the inverse of the coefficient matrix is shown to yield analytical expressions for the orientation-averaged total cross sections of the sphere cluster. Calculations of the cross sections of pairs of spheres and fractal aggregates of several spheres are presented. It is found that a dipole representation of the field in each sphere does not adequately predict the absorption cross section of clusters of small-size-parameter spheres when the spheres are highly conducting. For this situation several multipole orders are required for an accurate calculation of the absorption cross section. In addition, the predicted absorption of sphere clusters can be significantly greater than that estimated from the sum of the isolated-sphere cross sections.
“…(2)-(3) of MESI (Borghese et al, 1984) can be written in symmetrized form as (Hamermesh, 1962;Knox and Gold, 1964) Decomposition of the incident field [Eq. (la)] of MESI (Borghese et al, 1984) into parts belonging to the rows of the irreducible representations of 9 yields where W,,, is defined by Eq.…”
Section: Symmetry Adapted Multipolar Expansions Of the Fieldsmentioning
confidence: 99%
“…In a previous paper (Borghese et al, 1984) we proposed a method for studying the scattering properties of a cluster of spheres. Our approach, aimed at improving the Rayleigh-Debye theory (Rayleigh, 1881(Rayleigh, , 1910(Rayleigh, , 1914(Rayleigh, , 1918Debye, 1915) for the scattering of electromagnetic waves from molecules, is quite general in that it does not imply any restriction on either the effective index of refraction or the size and geometry of the cluster.…”
Section: Introductionmentioning
confidence: 99%
“…The multipoles transform according to the rows of the irreducible representations of the symmetry group. The symmetrization need not be applied to the Aerosol Sc~ence and Technology 3.237-243 (1984) field withn the spheres for, as shown in Section 4 of MESI (Borghese et al, 1984), the expansion coefficients of the internal field can be eliminated from the final equations.…”
Group theory is used to factorize systems of equations scattered by a cluster of spheres. Simple but significant for the expansion coefficients of the electromagnetic field examples are given.
Scattering‐type scanning near‐field optical microscopy (s‐SNOM) is becoming a premier method for the nanoscale optical investigation of materials well beyond the diffraction limit. A number of popular numerical methods exist to predict the near‐field contrast for axisymmetric configurations of scatterers on a surface in the quasi‐electrostatic approximation. Here, a fully electrodynamic approach is given for the calculation of near‐field contrast of several scatterers in arbitrary configuration, based on the generalized Mie scattering method. Examples for the potential of this new approach are given by showing the coupling of hyperbolic phonon polaritons in hexagonal boron nitride (hBN) layers and showing enhanced scattering in core–shell systems. In general, this method enables the numerical calculation of the near‐field contrast in a variety of strongly resonant scatterers and is able to accurately recreate spatial near‐field maps.
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