Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Satellite peaks in the scattering of light from the two-dimensional randomly rough surface of a dielectric film on a planar metal surface

Open Access Open Access

Abstract

A nonperturbative, purely numerical, solution of the reduced Rayleigh equation for the scattering of p- and s-polarized light from a dielectric film with a two-dimensional randomly rough surface deposited on a planar metallic substrate, has been carried out. It is found that satellite peaks are present in the angular dependence of the elements of the mean differential reflection coefficient in addition to an enhanced backscattering peak. This result resolves a conflict between the results of earlier approximate theoretical studies of scattering from this system.

© 2012 Optical Society of America

In the earliest analytic [1] and computer simulation [2,3] studies of the multiple scattering of light from clean one-dimensional randomly rough surfaces of perfect conductors or of penetrable media, the focus was on the phenomenon of enhanced backscattering. This is the presence of a well-defined peak in the retroreflection direction in the angular dependence of the intensity of the light that has been scattered incoherently (diffusely).

In subsequent work on the multiple scattering of light from free-standing or supported films with a one-dimensional randomly rough surface that support two or more guided waves, new effects were discovered [4]. These include enhanced transmission, which is the presence of a well-defined peak in the anti-specular direction in the angular dependence of the intensity of the light transmitted through the film [5]. Perhaps more interesting was the discovery of satellite peaks in the angular dependence of the intensity of the light scattered from or transmitted through the film. These are well-defined peaks present on both sides of the enhanced backscattering and enhanced transmission peaks, respectively, that arise from the coherent interference of guided waves with the frequency of the incident light, but with different wavenumbers [6].

It should be noted, however, that the prediction of these satellite peaks was first made in the context of the scattering of electromagnetic waves from a dielectric film containing a random distribution of volume scatterers [7], rather than from a randomly rough surface, when the thickness of the film is small compared to the mean free path of the electromagnetic wave in the random medium.

In analytic [810] and computer simulation calculations [1113] of the multiple scattering of light from clean two-dimensional randomly rough surfaces of perfect conductors and penetrable media, enhanced backscattering was observed in the results. However, when attention turned to the scattering of light from a perfectly conducting surface coated with a dielectric film, conflicting results were obtained. In these studies the dielectric-perfect conductor interface was assumed to be planar, while the vacuum-dielectric interface was assumed to be a two-dimensional randomly rough interface. In the first of these studies Kawanishi et al. [14] applied the stochastic functional approach to this problem and found no evidence for satellite peaks in their results. They suggested that the ensemble averaging of the intensity of the scattered field restores isotropy in the mean scattering plane, and thereby eliminates the occurrence of special scattering angles at which satellite peaks could occur. In subsequent work in which the reduced Rayleigh equation for scattering from this structure [10,15] was solved in the form of expansions of the amplitudes of the p- and s-polarized components of the scattered field in powers of the surface profile function through terms of third order, satellite peaks were found. However, the contribution to the scattering amplitudes associated with the third-order term was larger than that from the first-order term for the roughness and experimental parameters assumed in that work. It is therefore possible that these values fell outside the ranges for which a perturbative solution of the reduced Rayleigh equation is reliable.

Although satellite peaks were observed in experiments carried out by Méndez et al. [16] that utilized the double passage of polarized light through a random phase screen, the experimental conditions were sufficiently different from those studied theoretically in Refs. [10, 14], that these results could not be used to support the predictions of either of these studies.

In an effort to resolve the issue of whether satellite peaks do or do not exist in the scattering of light from a rough dielectric film deposited on the planar surface of a metal, in this paper we carry out a nonperturbative, purely numerical, solution of the reduced Rayleigh equation [17] for the scattering of p- and s-polarized light from a structure consisting of a dielectric film deposited on a metal substrate when the dielectric-metal interface is planar, while the vacuum-dielectric interface is a two-dimensional randomly rough interface. This is an approach that was used successfully in recent calculations of the scattering of p- and s-polarized light from a two-dimensional randomly rough interface between a dielectric and a metal [17, 18], which prompts its application to the present problem.

The system we study consists of vacuum (ε1) in the region x3 > d + ζ (x), where x = (x1, x2, 0); a dielectric film (ε2) in the region 0 < x3 < d + ζ (x); and a lossy metal (ε3) in the region x3 < 0. The surface profile function ζ (x) is assumed to be a single-valued function of x that is differentiable with respect to x1 and x2, and constitutes a zero-mean, stationary, isotropic, Gaussian random process defined by

ζ(x)ζ(x)=δ2W(|xx|).
The angle brackets here denote an average over the ensemble of realizations of the surface profile function, and δ = 〈ζ2 (x)〉1/2 is the rms height of the surface roughness.

The electric field in the vacuum [x3 > d +ζ (x)] is the sum of an incident field and a scattered field, E(x;t) = [E(x|ω)inc + E(x|ω)sc] exp(−iωt), where

E(x|ω)inc={cω[k^α1(k)+x^3k]Bp(k)+(x^3×k^)Bs(k)}×exp(ikxiα1(k)x3)
E(x|ω)sc=d2q(2π)2{cω[q^α1(q)x^3q]Ap(q)+(x^3×q^)As(q)}×exp(iqx+iα1(q)x3),
while the subscripts p and s denote the p-polarized and s-polarized components of these fields with respect to the local planes of incidence and scattering. A caret over a vector indicates that it is a unit vector, and the vector k is defined as k = (k1, k2, 0) (with similar definitions for q and p). The functions αi(q) (i = 1,2,3) are defined by
αi(q)=[ɛi(ωc)2q2]1/2,Reαi(q)>0,Imαi(q)>0.

A linear relation exists between the amplitudes Aα (q) and Bβ (k) (α, β = p,s), which we write as

Aα(q)=βRαβ(q|k)Bβ(k)
where Rαβ is the scattering amplitude for incident β-polarized light scattered into α-polarized light. The convention we use with respect to the polarization subscripts is
R(q|k)=(Rpp(q|k)Rps(q|k)Rsp(q|k)Rss(q|k)).

It has been shown by Soubret et al. [10] and Leskova [19] that the scattering amplitudes [Rαβ (q|k)] satisfy the matrix integral equation

d2q(2π)2M(p|q)R(q|k)=N(p|k),
called a reduced Rayleigh equation because it is an equation for only the scattered field in the medium of incidence, and not for the fields in the film and in the substrate.The effects of the latter two fields are contained in the elements of the matrices M(p|q) and N(p|k). With the shorthand notation α (q,ω) ≡ α(q), the elements of these matrices in the forms obtained by Leskova [19] are
Mpp(p|q)=[pq+α2(p)(p^q^)α1(q)]×Γp(p)exp(i[α2(p)α1(q)]d)I(α2(p)α1(q)|pq)α2(p)α1(q)+[pqα2(p)(p^q^)α1(q)]×Δp(p)exp(i[α2(p)+α1(q)]d)I([α2(p)+α1(q)]|pq)α2(p)+α1(q)
Mps(p|q)=ωcα2(p)(p^×q^)3(Γp(p)exp(i[α2(p)α1(q)]d)I(α2(p)α1(q)|pq)α2(p)α1(q)Δp(p)exp(i[α2(p)+α1(q)]d)I([α2(p)+α1(q)]|pq)α2(p)+α1(q))
Msp(p|q)=ωc(p^×q^)3α1(q)(Γs(p)exp(i[α2(p)α1(q)]d)I(α2(p)α1(q)|pq)α2(p)α1(q)+Δs(p)exp(i[α2(p)+α1(q)]d)I([α2(p)+α1(q)]|pq)α2(p)+α1(q))
Mss(p|q)=ω2c2(p^q^)(Γs(p)exp(i[α2(p)α1(q)]d)I(α2(p)α1(q)|pq)α2(p)α1(q)+Δs(p)exp(i[α2(p)+α1(q)]d)I([α2(p)+α1(q)]|pq)α2(p)+α1(q)),
and
Npp(p|k)=[pkα2(p)(p^k^)α1(k)]×Γp(p)exp(i[α2(p)+α1(k)]d)I(α2(p)+α1(k)|pk)α2(p)+α1(k)[pk+α2(p)(p^k^)α1(k)]×Δp(p)exp(i[α2(p)α1(k)]d)I([α2(p)α1(k)]|pk)α2(p)α1(k)
Nps(p|k)=ωcα2(p)(p^×k^)3×(Γp(p)exp(i[α2(p)+α1(k)]d)I(α2(p)+α1(k)|pk)α2(p)+α1(k)Δp(p)exp(i[α2(p)α1(k)]d)I([α2(p)α1(k)]|pk)α2(p)α1(k))
Nsp(p|k)=ωc(p^×k^)3α1(k)×(Γs(p)exp(i[α2(p)+α1(k)]d)I(α2(p)+α1(k)|pk)α2(p)+α1(k)+Δs(p)exp(i[α2(p)α1(k)]d)I([α2(p)α1(k)]|pk)α2(p)α1(k))
Nss(p|k)=ω2c2(p^k^)×(Γs(p)exp(i[α2(p)+α1(k)]d)I(α2(p)+α1(k)|pk)α2(p)+α1(k)+Δs(p)exp(i[α2(p)α1(k)]d)I([α2(p)α1(k)]|pk)α2(p)α1(k)).

In writing Eqs. (7) and (8) we have introduced the functions

Γp(p)=ɛ2α3(p,ω)+ɛ3α2(p,ω)
Δp(p)=ɛ2α3(p,ω)ɛ3α2(p,ω)
and
Γs(p)=α3(p,ω)+α2(p,ω)
Δs(p)=α3(p,ω)α2(p,ω),
as well as
I(γ|Q)=d2xexp(iQx)exp[iγζ(x)].
The scattering amplitudes [Rαβ (q|k)] play a central role in the present theory because the mean differential reflection coefficient, an experimentally measurable function, can be expressed in terms of these amplitudes. The differential reflection coefficient (∂R/∂Ωs) is defined such that (∂R/∂Ωs)dΩs is the fraction of the total time-averaged flux incident on the surface that is scattered into the element of solid angle dΩs about the scattering direction (θs,ϕs). Since we are studying the scattering of light from a randomly rough surface, it is the average of this function over the ensemble of realizations of the surface profile function that we need to calculate. The contribution to the mean differential reflection coefficient from the incoherent (diffuse) component of the scattered light, when incident light of β polarization whose wave vector has the projection k on the mean scattering surface is scattered into light of α polarization whose wave vector has the projection q on the mean scattering surface, denoted 〈∂Rαβ/Ωsincoh, is given by
RppΩsincoh=1Sɛ14π2ωcα12(q)α1(k)[|Rpp(q|k)|2|Rpp(q|k)|2]
RpsΩsincoh=1Sɛ13/24π2ωcα12(q)α1(k)[|Rps(q|k)|2|Rps(q|k)|2]
RspΩsincoh=1S14π2ɛ1ωcα12(q)α1(k)[|Rsp(q|k)|2|Rsp(q|k)|2]
RssΩsincoh=1Sɛ14π2ωcα12(q)α1(k)[|Rss(q|k)|2|Rss(q|k)|2],
where S is the area of the plane x3 = 0 covered by the rough surface. The two-dimensional wave vectors k and q are defined in terms of the polar and azimuthal angles of incidence (θ0,ϕ0) and scattering (θs,ϕs), respectively, by k=ɛ1(ω/c)sinθ0(cosϕ0,sinϕ0,0) and q=ɛ1(ω/c)sinθs(cosϕs,sinϕs,0). Thus these wave vectors in Eq. (12) are restricted to the domains k<ɛ1(ω/c) and q<ɛ1(ω/c) of the q1q2 plane.

Up to now Eq. (6) has been solved by small-amplitude perturbation theory through terms of third order in the surface profile function [10, 20]. Here we present results for the mean differential reflection coefficient and for the full angular distribution of the intensity of the scattered light obtained by a nonperturbative, purely numerical solution of Eqs. (6)(11), as described in Ref. [17]. This was done by generating a realization of the surface profile function numerically on a grid of Nx2 points within a square region of the x1x2 plane of edge L, so that the (linear) sampling interval was Δx = L/Nx. A two-dimensional version of the filtering method used in [17, 21] was used to generate the profile function [13]. The function I(γ|Q) was then evaluated by expanding the integrand in powers of the surface profile function ζ(x), and calculating the Fourier transform of ζn(x) by the fast Fourier transform. In evaluating the integral over q in Eq. (6) the infinite limits were replaced by finite ones: (q12+q22)1/2Q/2. The Nyquist sampling theorem requires that |q1| and |q2| be smaller than Qc = π/Δx [22, p. 605]. The components of the vector pq entering I(γ|pq) lie in the interval [−Q,Q], so we have chosen Q = Qc. A grid with a grid constant Δq1 = Δq2 = Δq = 2π/L was constructed within the circular region of the q1q2 plane where (q12+q22)Q/2. The integral over this region in Eq. (6) was carried out by a two-dimensional version of the extended midpoint method [22, p. 161] and the values of Rαβ (q|k) were calculated for values of q at the points of this grid for a given value of k, which was also a point on this grid. The resulting matrix equations were solved by LU factorization and backsubstitution. The values of Rαβ (q|k) and |Rαβ (q|k)|2 were then calculated for Np realizations of the surface profile function. An arithmetic average of the Np results for each of these functions yielded the averages 〈Rαβ (q|k)〉 and 〈|Rαβ (q|k)|2〉, from which the incoherent contribution to the mean differential reflection coefficients were calculated according to Eq. (12).

We apply this approach to the scattering of p- and s-polarized plane waves, whose wavelength is λ = 633 nm, incident from vacuum (ε1 = 1) on a dielectric film (ε2 = 2.6896+0.01i) coating a silver surface (ε3 = −18.28 + 0.481i) [23]. The mean thickness of the film is d = 0.756λ = 478.5 nm. The roughness of the vacuum-dielectric interface is characterized by a two-dimensional version of the West–O’Donnell power spectrum [24] given by [8]

g(|k|)=4πk+2k2θ(|k|k)θ(k+|k|),
where θ(x) is the Heaviside unit step function, and k = 0.82(ω/c), k+ = 1.97(ω/c). The rms height of the surface roughness was assumed to be δ = λ/40 = 15.82 nm, the surface was discretized on a grid of resolution Δx1 = Δx2 = 0.123λ = 77.6 nm and the edge of the (quadratic) surface was L = 55λ = 34.8 μm.

The contribution to the mean differential reflection coefficient 〈∂Rαβ (q|k)/Ωsincoh from single-scattering processes [second order in ζ (x)] is proportional to g(|qk|) [8]. Since the power spectrum (13) is identically zero for |k| < k, there is no contribution to the mean differential reflection coefficient from the light scattered incoherently by single-scattering processes when the wave vectors q and k satisfy the inequality |qk| < k. The contribution to 〈∂Rαβ (q|k)/Ωsincoh when this condition is satisfied is due only to multiple-scattering processes, including the enhanced backscattering peak and the satellite peaks. These features are more clearly visible in this case because they do not ride on a large background due to single-scattering processes. This is the reason that the calculations whose results are presented here were carried out on the basis of the power spectrum (13).

In Fig. 1(a) we present the contribution to the mean differential reflection coefficient from the light scattered incoherently as functions of the polar scattering angle θs for the in-plane (ϕs = ϕ0 = 45°) co-(p→p, s→s) and cross-(p→s, s→p) polarized scattering when a p- or s-polarized plane wave is incident on the dielectric surface at angles of incidence (θ0,ϕ0) given by (0.74°, 45°). (In figures showing in-plane or out-of-plane scattering, we depart from the commonly accepted principle of not using negative polar angles, in that we allow for negative θs.). An arithmetic average of results obtained for Np = 11,165 realizations of the surface profile function was carried out to produce these figures. In Fig. 1(b) we present the analogous results for out-of-plane (ϕs = ϕ0 ± 90°) scattering when the roughness and experimental parameters have the values assumed in generating Fig. 1(a).

 figure: Fig. 1

Fig. 1 (a) The contributions to the mean differential reflection coefficient as functions of the polar scattering angle θs from the in-plane (ϕs = ϕ0) co-polarized (p→p, s→s) and cross-polarized (p→s, s→p) scattering of light incident on the two-dimensional randomly rough surface of a dielectric film deposited on the planar surface of silver, whose dielectric constant is ε3 = −18.28 + 0.481i. The wavelength of the incident light is λ = 633 nm, the angles of incidence are (θ0,ϕ0) = (0.74°, 45°). The dielectric constant of the film is ε2 = 2.6896+ 0.01i, and its mean thickness is d = 478.5 nm. The roughness of the surface is characterized by the power spectrum in Eq. (13), with k = 0.82(ω/c), k+ = 1.97(ω/c), and its rms height is δ = λ/40 = 15.82 nm. (b) The same as (a) for out-of-plane (ϕs = ϕ0 + 90°) scattering.

Download Full Size | PDF

In the results depicted in Fig. 1(a) [1(b)] single-scattering processes give no contributions to the mean differential reflection coefficient for −53.8° < θs < 56.4° (−55.08° < θs < 55.08°). In both figures a well-defined enhanced backscattering peak is seen in the retroreflection direction. In addition, in Fig. 1(a) additional peaks are seen on both sides of the enhanced backscattering peak in the s → s co-polarized scattering contribution to the mean differential reflection coefficient. These peaks are identified as satellite peaks.

We base this identification on the following consideration. It was shown in [6] that in the in-plane co-polarized scattering of light of frequency ω from a one-dimensional randomly rough surface of a film system when the plane of incidence is perpendicular to the generators of the surface, satellite peaks occur at scattering angles given by

sinθs(m,n)=sinθ0±cωɛ1[qm(ω)qn(ω)].
The wave numbers q1(ω),q2(ω),...,qN(ω) are the wavenumbers of the guided waves supported by the film structure at the frequency of the incident light. Not all of the peaks predicted by Eq. (14) may be present in the mean differential reflection coefficient. This happens when the absolute value of the right-hand side of Eq. (14) is greater than unity. Then the corresponding peak lies in the nonradiative region of the q1q2 plane. In addition, among the real satellite peaks that should appear in the radiative region, not all may be sufficiently intense to be observable.

The scattering angles defined by Eq. (14) are expected to give the angles at which satellite peaks occur in the in-plane co-polarized scattering from the two-dimensional randomly rough surface of the film system studied here.

In the absence of absorption and roughness the {qj(ω)} are the solutions of the dispersion relation

α2(q,ω)=12ɛ1ɛ3(ɛ2[ɛ1β3(q,ω)+ɛ3β1(q,ω)]cot[α2(q,ω)d]±{ɛ22[ɛ1β3(q,ω)+ɛ3β1(q,ω)]2cot2[α2(q,ω)d]+4ɛ1ɛ22ɛ3β1(q,ω)β3(q,ω)}1/2)
in p polarization, and
α2(q,ω)=12([β1(q,ω)+β3(q,ω)]cot[α2(q,ω)d]±{[β1(q,ω)+β3(q,ω)]2cot2[α2(q,ω)d]+4β1(q,ω)+β3(q,ω)}1/2)
in s polarization. In these equations βi(q,ω)=[q2ɛi(ω/c)2]1/2 for i = 1,3, while α2(q, ω) is defined in Eq. (3). The film structure studied in this paper is found to support two guided waves in p-polarization, whose wave numbers are
q1(ω)=1.4391(ω/c),q2(ω)=1.0119(ω/c),
and two guided waves in s polarization, with wave numbers
q1(ω)=1.5467(ω/c),q2(ω)=1.2432(ω/c).
These results predict satellite peaks at scattering angles θs = −25.22° and 23.74° in p polarization and at θs = −18.13° and 16.65° in s polarization when we are considering in-plane scattering, assuming the same angles of incidence as in Fig. 1. These scattering angles are indicated by vertical dotted lines in Fig. 1(a). The peaks at θs = −18.13° and 16.65° are seen in the s→s co-polarized scattering contribution to the mean differential reflection coefficient. There is no evidence of satellite peaks at θs(1,2)=25.22°and23.74° in the p→p co-polarized scattering contribution to the mean differential reflection coefficient, presumably because they are too weak to be seen. These results disagree with those of [10], in which no satellite peaks were found in the in-plane s→s scattering contribution to the mean differential reflection coefficient (although they are present in this contribution when the dielectric film is deposited on a planar perfectly conducting surface). However, in [10] the surface roughness was characterized by a Gaussian power spectrum, not the West–O’Donnell power spectrum assumed here. The results of earlier calculations [25] of the scattering of p- and s-polarized light from a film with a one-dimensional randomly rough surface characterized by a Gaussian power spectrum that is deposited on a planar perfectly conducting surface, display satellite peaks more weakly than when the roughness is characterized by a West–O’Donnell power spectrum [26].

Turning now to the results for out-of-plane scattering presented in Fig. 1(b), we see that an enhanced backscattering peak is present in each scattering configuration. It is cut off in each configuration. This is an artifact of the present calculation that results from the line defined by ϕs = ϕ0 ± 90° being exactly one grid point away from the backscattering direction. It is important to note that in out-of-plane scattering the predominant contribution to the differential reflection coefficient is in the cross-polarized part. We see that the satellite peaks are now observed in the p→s scattering configuration, meaning that incident p-polarized light excites both of the s-polarized guided modes with wave vectors in the ϕ = ϕ0 ± 90° directions, which subsequently interfere to cause satellite peaks in out-of-plane scattering. Hence, the well-known “satellite peaks” found in scattering from 1D surfaces turn into a kind of “satellite rings” for scattering from 2D surfaces, where part of the ring is co-polarized (s→s in-plane) and part of the ring is cross-polarized (p→s out-of-plane).

In Fig. 2 we present contour plots of the complete angular distribution of the mean differential reflection coefficient for the light scattered incoherently from the film system studied here. The material and experimental parameters used in producing these results have the same values used in obtaining Fig. 1.

 figure: Fig. 2

Fig. 2 The complete angular distribution of the mean differential reflection coefficient 〈∂Rαβ/Ωsincoh for the light scattered incoherently from the film structure. The material and experimental parameters assumed here are those used in obtaining the plots presented in Fig. 1. Light of either p (left column) or s (right column) polarization is incident on the structure. In (a) and (d) all (diffusely) scattered light is recorded. In (b) and (e) only the p-polarized scattered light is recorded, while in (c) and (f) only the s-polarized scattered light is recorded. The dark dot in each panel indicates the enhanced backscattering peak. Note that the gray scale bar is cut at both ends in order to enhance the satellite rings. Also note that the contribution from single scattering is suppressed, i.e. the differential reflection coefficient is artificially set to 0 for |qk|>k.

Download Full Size | PDF

Light of p polarization (left column) or s polarization (right column) is incident on the structure. In Figs. 2(a) and 2(d) all of the scattered light is recorded; in Figs. 2(b) and 2(e) only the p-polarized scattered light is recorded; while in Figs. 2(c) and 2(f) only the s-polarized scattered light is recorded. In Fig. 2(f) we see two regions of high intensity in the in-plane polarized (s→s) intensity distribution, centered at radii of approximately 0.29(ω/c) at ϕs = 45°, and 0.31 (ω/c) at ϕs = 225°. These are the satellite peaks seen in the plot of 〈∂Rss/Ωsincoh presented in Fig. 1(a). No such regions of high intensity are seen in Fig. 2(b) at radii of 0.34(ω/c) at ϕs = 45° and 0.52(ω/c) at ϕs = 225°, where satellite peaks are predicted by Eq. (14) for in-plane co-polarized scattering of p-polarized incident light. This result is consistent with the absence of satellite peaks in the result for 〈∂Rpp/Ωsincoh presented in Fig. 1(a). The intensity maxima in the out-of-plane cross-polarized (p→s) scattering intensity distribution depicted in Fig. 2(c) correspond to the peaks at θs ≈ 19° seen in the plot of 〈∂Rsp/Ωsincoh presented in Fig. 1(b).

The result that satellite peaks are observed in scattering processes in which the scattered light is s polarized, independent of the polarization of the incident light, is an interesting result of the present calculations. It may be connected with the fact that s-polarized light is reflected more strongly from a dielectric surface than is p-polarized light.

In Fig. 3 we present results analogous to those presented in Fig. 1, but for angles of incidence (θ0,ϕ0) = (5.19°,45°). In Fig. 3(a) we present results for the in-plane (ϕs = ϕ0) co-(p→p, s→s) and cross-(p→s, s→p) polarized scattering, while in Fig. 3(b) we present results for out-of-plane (ϕs = ϕ0 ± 90°) co-(p→p, s→s) and cross-(p→s, s→p) polarized scattering. In the results presented in Fig. 3(a) [3(b)] single-scattering processes give no contribution to the mean differential reflection coefficient for −46.85° < θs < 65.57° (−54.59° < θs < 54.59°). The limits of these angular regions are clearly seen in these figures.

 figure: Fig. 3

Fig. 3 The same as Fig. 1, but for angles of incidence given by (θ0,ϕ0) = (5.19°, 45°).

Download Full Size | PDF

A well-defined enhanced backscattering peak is seen in the results plotted in Fig. 3(a). Satellite peaks are predicted by Eq. (14) to occur (in-plane) at θs(1,2)=31.18°and19.68° for p-polarized incident light, and at θs(1,2)=23.20°and12.30° for s-polarized incident light, when the angles of incidence were the same as in Fig. 3. These scattering angles are indicated by vertical dotted lines in this figure. Peaks at θs = −23.20° and θs = 12.30° are present in the s→s co-polarized scattering contribution to the mean differential reflection coefficient. There is no suggestion of peaks at θs = −31.8° and 19.68° in the p→p co-polarized scattering contribution to the mean differential reflection coefficient, nor any suggestions of peaks in the cross-polarized (p→s, s→p) contribution to it.

The results for out-of-plane scattering presented in Fig. 3(b) show no enhanced backscattering peaks. The reason for this is simply that since the abscissa points along ϕ = ϕ0 ± 90°, it does not cut through the backscattering peak, localized at (θs,ϕs) = (θ0,ϕ0 + 180°). We do see some remainders of the satellite ring structure; the low peaks around θs ≈ ±20° are part of the rings to the upper left in Fig. 4. As the rings decay in strength away from the direction ϕ = ϕ0 ± 90°, they are weaker than what is seen in-plane.

 figure: Fig. 4

Fig. 4 The same as Fig. 2, but for angles of incidence given by (θ0,ϕ0) = (5.19°, 45°). Note that the color bar is cut at both ends in order to enhance the satellite rings. Also note that the contribution from single scattering is suppressed, i.e. the differential reflection coefficient is artificially set to 0 for |qk|>k.

Download Full Size | PDF

As a necessary, but not sufficient, condition of the validity of our simulation results is energy conservation. If all materials in the scattering system are lossless, i.e. Im(εi) = 0 (i = 1,2,3), the power of the scattered light has to be equal to the power of the incident light. Under these conditions, energy was conserved within 0.03% in our simulations.

In conclusion, in this paper we have presented a nonperturbative approach to the solution of the reduced Rayleigh equation for the scattering of polarized light from a dielectric film with a two-dimensional randomly rough surface deposited on a planar metallic surface. We have applied this result to calculate the contributions to the mean differential reflection coefficient from the in-plane co- and cross-polarized components of the light scattered incoherently, as well as from the out-of-plane co-and cross-polarized components of the light scattered incoherently. The out-of-plane scattering contributions have not been calculated in earlier perturbative studies of this problem [10, 14]. In addition, we have calculated the full angular distribution of the intensity of the scattered light, which has helped to refine the conclusions drawn from the calculations of the mean differential reflection coefficient. The main physical result obtained in this work is the demonstration that satellite peaks (or rings) can arise in scattering from the film structure studied here. This result is in agreement with the results of Soubret et al. [10] but not with those of Kawanishi et al. [14]. A detailed study of the conditions under which satellite peaks occur is lacking, but perhaps the approach developed here will be used to determine them. The work reported here also opens the door to the possibility of calculating other properties of the light scattered from the film system studied here, such as all the elements of the associated Mueller matrix, and offers the possibility of designing such structures to possess specified scattering properties. These are problems that have to be left to the future.

Acknowledgments

The research of T.N., P.A.L., and I.S. was supported in part by NTNU by the allocation of computer time. The research of A.A.M. was supported in part by AFRL contract FA9453-08-C-0230. T.N., P.A.L., and I.S. would like to thank Dr. Jamie Cole at the University of Edinburgh for his kind hospitality and fruitful discussions. They would also like to acknowledge the assistance of Dr. Fiona Reid and Dr. Christopher Johnson at the EPCC in parallelizing and optimizing the simulation code. The work by T.N. and P.A.L. was partially carried out under the HPC-EUROPA2 project (project number: 228398) with the support of the European Commission—Capacities Area—Research Infrastructures.

References and links

1. A. R. McGurn, A. A. Maradudin, and V. Celli, “Localization effects in the scattering of light from a randomly rough grating,” Phys. Rev. B 31, 4866–4871 (1985). [CrossRef]  

2. M. Nieto-Vesperinas and J. M. Soto-Crespo, “Monte Carlo simulations for scattering of electromagnetic waves from perfectly conductive random rough surfaces,” Opt. Lett. 12, 979–981 (1987). [CrossRef]   [PubMed]  

3. A. A. Maradudin, E. R. Méndez, and T. Michel, “Backscattering effects in the elastic scattering of p-polarized light from a large-amplitude random metallic grating,” Opt. Lett. 14, 151–153 (1989). [CrossRef]   [PubMed]  

4. I. Simonsen, “Optics of surface disordered systems,” Eur. Phys. J.–Spec. Top. 181, 1–103 (2010). [CrossRef]  

5. A. McGurn and A. Maradudin, “An analogue of enhanced backscattering in the transmission of light through a thin film with a randomly rough surface,” Opt. Commun. 72, 279–285 (1989). [CrossRef]  

6. V. Freilikher, E. Kanzieper, and A. Maradudin, “Coherent scattering enhancement in systems bounded by rough surfaces,” Phys. Rep. 288, 127–204 (1997). [CrossRef]  

7. V. Freilikher, M. Pustilnik, and I. Yurkevich, “Wave scattering from a bounded medium with disorder,” Phys. Lett. A 193, 467–470 (1994). [CrossRef]  

8. A. McGurn and A. Maradudin, “Perturbation theory results for the diffuse scattering of light from two-dimensional randomly rough metal surfaces,” Wave. Random Media 6, 251–267 (1996). [CrossRef]  

9. J. T. Johnson, “Third-order small-perturbation method for scattering from dielectric rough surfaces,” J. Opt. Soc. Am. A 16, 2720–2736 (1999). [CrossRef]  

10. A. Soubret, G. Berginc, and C. Bourrely, “Application of reduced Rayleigh equations to electromagnetic wave scattering by two-dimensional randomly rough surfaces,” Phys. Rev. B 63, 245411 (2001). [CrossRef]  

11. I. Simonsen, A. A. Maradudin, and T. A. Leskova, “Scattering of electromagnetic waves from two-dimensional randomly rough perfectly conducting surfaces: The full angular intensity distribution,” Phys. Rev. A 81, 013806 (2010). [CrossRef]  

12. I. Simonsen, A. A. Maradudin, and T. A. Leskova, “Scattering of electromagnetic waves from two-dimensional randomly rough penetrable surfaces,” Phys. Rev. Lett. 104, 223904 (2010). [CrossRef]   [PubMed]  

13. I. Simonsen, J. B. Kryvi, A. A. Maradudin, and T. A. Leskova, “Light scattering from anisotropic, randomly rough, perfectly conducting surfaces,” Comput. Phys. Commun. 182, 1904–1908 (2011). [CrossRef]  

14. T. Kawanishi, H. Ogura, and Z. L. Wang, “Scattering of an electromagnetic wave from a slightly random dielectric surface: Yoneda peak and Brewster angle in incoherent scattering,” Wave. Random Media 7, 351–384 (1997). [CrossRef]  

15. A. Soubret, G. Berginc, and C. Bourrely, “Backscattering enhancement of an electromagnetic wave scattered by two-dimensional rough layers,” J. Opt. Soc. Am. A 18, 2778–2788 (2001). [CrossRef]  

16. E. R. Méndez, E. I. Chaikina, and H. M. Escamilla, “Observation of satellite peaks and dips in the scattering of light in a double-pass geometry,” Opt. Lett. 24, 705–707 (1999). [CrossRef]  

17. T. Nordam, P. A. Letnes, and I. Simonsen, “Numerical simulations of scattering of light from two-dimensional surfaces using the reduced Rayleigh equation,” http://arxiv.org/abs/1204.4984.

18. T. A. Leskova, P. A. Letnes, A. A. Maradudin, T. Nordam, and I. Simonsen, “The scattering of light from two-dimensional randomly rough surfaces,” Proc. SPIE 8172, 817209 (2011). [CrossRef]  

19. T. A. Leskova, Department of Physics and Astronomy, University of California, Irvine CA 92697, U.S.A. (personal communication, 2010).

20. J. T. Johnson, “Third-order small-perturbation method for scattering from dielectric rough surfaces,” J. Opt. Soc. Am. A 16, 2720–2736 (1999). [CrossRef]  

21. A. Maradudin, T. Michel, A. McGurn, and E. Méndez, “Enhanced backscattering of light from a random grating,” Ann. Phys. 203, 255–307 (1990). [CrossRef]  

22. W. Press, B. Flannery, S. Teukolsky, and W. Vetterling, Numerical recipes, 3rd ed. (Cambridge Univ Press, 2007).

23. P. B. Johnson, “Optical constants of the noble metals,” Phys. Rev. 6, 4370–4379 (1972). [CrossRef]  

24. C. S. West and K. A. O’Donnell, “Observations of backscattering enhancement from polaritons on a rough metal surface,” J. Opt. Soc. Am. A 12, 390–397 (1995). [CrossRef]  

25. A. Madrazo and A. Maradudin, “Numerical solutions of the reduced Rayleigh equation for the scattering of electromagnetic waves from rough dielectric films on perfectly conducting substrates,” Opt. Commun. 134, 251–263 (1997). [CrossRef]  

26. I. Simonsen and A. Maradudin, “Numerical simulation of electromagnetic wave scattering from planar dielectric films deposited on rough perfectly conducting substrates,” Opt. Commun. 162, 99–111 (1999). [CrossRef]  

Cited By

Optica participates in Crossref's Cited-By Linking service. Citing articles from Optica Publishing Group journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (4)

Fig. 1
Fig. 1 (a) The contributions to the mean differential reflection coefficient as functions of the polar scattering angle θs from the in-plane (ϕs = ϕ0) co-polarized (p→p, s→s) and cross-polarized (p→s, s→p) scattering of light incident on the two-dimensional randomly rough surface of a dielectric film deposited on the planar surface of silver, whose dielectric constant is ε3 = −18.28 + 0.481i. The wavelength of the incident light is λ = 633 nm, the angles of incidence are (θ0,ϕ0) = (0.74°, 45°). The dielectric constant of the film is ε2 = 2.6896+ 0.01i, and its mean thickness is d = 478.5 nm. The roughness of the surface is characterized by the power spectrum in Eq. (13), with k = 0.82(ω/c), k+ = 1.97(ω/c), and its rms height is δ = λ/40 = 15.82 nm. (b) The same as (a) for out-of-plane (ϕs = ϕ0 + 90°) scattering.
Fig. 2
Fig. 2 The complete angular distribution of the mean differential reflection coefficient 〈∂Rαβ/Ωsincoh for the light scattered incoherently from the film structure. The material and experimental parameters assumed here are those used in obtaining the plots presented in Fig. 1. Light of either p (left column) or s (right column) polarization is incident on the structure. In (a) and (d) all (diffusely) scattered light is recorded. In (b) and (e) only the p-polarized scattered light is recorded, while in (c) and (f) only the s-polarized scattered light is recorded. The dark dot in each panel indicates the enhanced backscattering peak. Note that the gray scale bar is cut at both ends in order to enhance the satellite rings. Also note that the contribution from single scattering is suppressed, i.e. the differential reflection coefficient is artificially set to 0 for | q k | > k .
Fig. 3
Fig. 3 The same as Fig. 1, but for angles of incidence given by (θ0,ϕ0) = (5.19°, 45°).
Fig. 4
Fig. 4 The same as Fig. 2, but for angles of incidence given by (θ0,ϕ0) = (5.19°, 45°). Note that the color bar is cut at both ends in order to enhance the satellite rings. Also note that the contribution from single scattering is suppressed, i.e. the differential reflection coefficient is artificially set to 0 for | q k | > k .

Equations (30)

Equations on this page are rendered with MathJax. Learn more.

ζ ( x ) ζ ( x ) = δ 2 W ( | x x | ) .
E ( x | ω ) inc = { c ω [ k ^ α 1 ( k ) + x ^ 3 k ] B p ( k ) + ( x ^ 3 × k ^ ) B s ( k ) } × exp ( i k x i α 1 ( k ) x 3 )
E ( x | ω ) sc = d 2 q ( 2 π ) 2 { c ω [ q ^ α 1 ( q ) x ^ 3 q ] A p ( q ) + ( x ^ 3 × q ^ ) A s ( q ) } × exp ( i q x + i α 1 ( q ) x 3 ) ,
α i ( q ) = [ ɛ i ( ω c ) 2 q 2 ] 1 / 2 , Re α i ( q ) > 0 , Im α i ( q ) > 0 .
A α ( q ) = β R α β ( q | k ) B β ( k )
R ( q | k ) = ( R pp ( q | k ) R ps ( q | k ) R sp ( q | k ) R ss ( q | k ) ) .
d 2 q ( 2 π ) 2 M ( p | q ) R ( q | k ) = N ( p | k ) ,
M pp ( p | q ) = [ p q + α 2 ( p ) ( p ^ q ^ ) α 1 ( q ) ] × Γ p ( p ) exp ( i [ α 2 ( p ) α 1 ( q ) ] d ) I ( α 2 ( p ) α 1 ( q ) | p q ) α 2 ( p ) α 1 ( q ) + [ p q α 2 ( p ) ( p ^ q ^ ) α 1 ( q ) ] × Δ p ( p ) exp ( i [ α 2 ( p ) + α 1 ( q ) ] d ) I ( [ α 2 ( p ) + α 1 ( q ) ] | p q ) α 2 ( p ) + α 1 ( q )
M ps ( p | q ) = ω c α 2 ( p ) ( p ^ × q ^ ) 3 ( Γ p ( p ) exp ( i [ α 2 ( p ) α 1 ( q ) ] d ) I ( α 2 ( p ) α 1 ( q ) | p q ) α 2 ( p ) α 1 ( q ) Δ p ( p ) exp ( i [ α 2 ( p ) + α 1 ( q ) ] d ) I ( [ α 2 ( p ) + α 1 ( q ) ] | p q ) α 2 ( p ) + α 1 ( q ) )
M sp ( p | q ) = ω c ( p ^ × q ^ ) 3 α 1 ( q ) ( Γ s ( p ) exp ( i [ α 2 ( p ) α 1 ( q ) ] d ) I ( α 2 ( p ) α 1 ( q ) | p q ) α 2 ( p ) α 1 ( q ) + Δ s ( p ) exp ( i [ α 2 ( p ) + α 1 ( q ) ] d ) I ( [ α 2 ( p ) + α 1 ( q ) ] | p q ) α 2 ( p ) + α 1 ( q ) )
M ss ( p | q ) = ω 2 c 2 ( p ^ q ^ ) ( Γ s ( p ) exp ( i [ α 2 ( p ) α 1 ( q ) ] d ) I ( α 2 ( p ) α 1 ( q ) | p q ) α 2 ( p ) α 1 ( q ) + Δ s ( p ) exp ( i [ α 2 ( p ) + α 1 ( q ) ] d ) I ( [ α 2 ( p ) + α 1 ( q ) ] | p q ) α 2 ( p ) + α 1 ( q ) ) ,
N pp ( p | k ) = [ p k α 2 ( p ) ( p ^ k ^ ) α 1 ( k ) ] × Γ p ( p ) exp ( i [ α 2 ( p ) + α 1 ( k ) ] d ) I ( α 2 ( p ) + α 1 ( k ) | p k ) α 2 ( p ) + α 1 ( k ) [ p k + α 2 ( p ) ( p ^ k ^ ) α 1 ( k ) ] × Δ p ( p ) exp ( i [ α 2 ( p ) α 1 ( k ) ] d ) I ( [ α 2 ( p ) α 1 ( k ) ] | p k ) α 2 ( p ) α 1 ( k )
N ps ( p | k ) = ω c α 2 ( p ) ( p ^ × k ^ ) 3 × ( Γ p ( p ) exp ( i [ α 2 ( p ) + α 1 ( k ) ] d ) I ( α 2 ( p ) + α 1 ( k ) | p k ) α 2 ( p ) + α 1 ( k ) Δ p ( p ) exp ( i [ α 2 ( p ) α 1 ( k ) ] d ) I ( [ α 2 ( p ) α 1 ( k ) ] | p k ) α 2 ( p ) α 1 ( k ) )
N sp ( p | k ) = ω c ( p ^ × k ^ ) 3 α 1 ( k ) × ( Γ s ( p ) exp ( i [ α 2 ( p ) + α 1 ( k ) ] d ) I ( α 2 ( p ) + α 1 ( k ) | p k ) α 2 ( p ) + α 1 ( k ) + Δ s ( p ) exp ( i [ α 2 ( p ) α 1 ( k ) ] d ) I ( [ α 2 ( p ) α 1 ( k ) ] | p k ) α 2 ( p ) α 1 ( k ) )
N ss ( p | k ) = ω 2 c 2 ( p ^ k ^ ) × ( Γ s ( p ) exp ( i [ α 2 ( p ) + α 1 ( k ) ] d ) I ( α 2 ( p ) + α 1 ( k ) | p k ) α 2 ( p ) + α 1 ( k ) + Δ s ( p ) exp ( i [ α 2 ( p ) α 1 ( k ) ] d ) I ( [ α 2 ( p ) α 1 ( k ) ] | p k ) α 2 ( p ) α 1 ( k ) ) .
Γ p ( p ) = ɛ 2 α 3 ( p , ω ) + ɛ 3 α 2 ( p , ω )
Δ p ( p ) = ɛ 2 α 3 ( p , ω ) ɛ 3 α 2 ( p , ω )
Γ s ( p ) = α 3 ( p , ω ) + α 2 ( p , ω )
Δ s ( p ) = α 3 ( p , ω ) α 2 ( p , ω ) ,
I ( γ | Q ) = d 2 x exp ( i Q x ) exp [ i γ ζ ( x ) ] .
R pp Ω s incoh = 1 S ɛ 1 4 π 2 ω c α 1 2 ( q ) α 1 ( k ) [ | R pp ( q | k ) | 2 | R pp ( q | k ) | 2 ]
R ps Ω s incoh = 1 S ɛ 1 3 / 2 4 π 2 ω c α 1 2 ( q ) α 1 ( k ) [ | R ps ( q | k ) | 2 | R ps ( q | k ) | 2 ]
R sp Ω s incoh = 1 S 1 4 π 2 ɛ 1 ω c α 1 2 ( q ) α 1 ( k ) [ | R sp ( q | k ) | 2 | R sp ( q | k ) | 2 ]
R ss Ω s incoh = 1 S ɛ 1 4 π 2 ω c α 1 2 ( q ) α 1 ( k ) [ | R ss ( q | k ) | 2 | R ss ( q | k ) | 2 ] ,
g ( | k | ) = 4 π k + 2 k 2 θ ( | k | k ) θ ( k + | k | ) ,
sin θ s ( m , n ) = sin θ 0 ± c ω ɛ 1 [ q m ( ω ) q n ( ω ) ] .
α 2 ( q , ω ) = 1 2 ɛ 1 ɛ 3 ( ɛ 2 [ ɛ 1 β 3 ( q , ω ) + ɛ 3 β 1 ( q , ω ) ] cot [ α 2 ( q , ω ) d ] ± { ɛ 2 2 [ ɛ 1 β 3 ( q , ω ) + ɛ 3 β 1 ( q , ω ) ] 2 cot 2 [ α 2 ( q , ω ) d ] + 4 ɛ 1 ɛ 2 2 ɛ 3 β 1 ( q , ω ) β 3 ( q , ω ) } 1 / 2 )
α 2 ( q , ω ) = 1 2 ( [ β 1 ( q , ω ) + β 3 ( q , ω ) ] cot [ α 2 ( q , ω ) d ] ± { [ β 1 ( q , ω ) + β 3 ( q , ω ) ] 2 cot 2 [ α 2 ( q , ω ) d ] + 4 β 1 ( q , ω ) + β 3 ( q , ω ) } 1 / 2 )
q 1 ( ω ) = 1.4391 ( ω / c ) , q 2 ( ω ) = 1.0119 ( ω / c ) ,
q 1 ( ω ) = 1.5467 ( ω / c ) , q 2 ( ω ) = 1.2432 ( ω / c ) .
Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.