We examine the potential of ultra-thin metallic layers for broadband wave-impedance matching in the terahertz frequency range. The metallic layer is modeled using Fresnel formulae for stratified optical medium. Experimental data for chromium and indium-tin-oxide layers, measured using time-domain terahertz spectroscopy over the frequency range 0.4 – 4.5 THz, are compared with theoretical results.
©2007 Optical Society of America
In recent years developments in terahertz technology have established time-domain terahertz spectroscopy (THz-TDS) as an important state-of-the-art tool in physics, chemistry, and even medical applications . The unique, otherwise hidden, features and characteristics of many materials become observable in the terahertz frequency range. The inherently large bandwidth of THz-TDS systems requires that equally broadband optical components are available to manipulate the terahertz beam. Here, efficient wave-impedance matching layers are needed to minimize the reflections of free-space propagating THz waves from refractive optic elements and beam splitters used in the THz beam path. Since the standard λ 0/4 dielectric antireflection layer is not suitable for THz systems due to its inherently small bandwidth , we examine the potential of semi-metallic and metallic films to serve as effective antireflection coatings for broadband THz signals.
The optical properties and performance of thin metallic films in the far-infrared frequency region have already been studied theoretically and experimentally [3,4]. It has been shown that a free-standing metallic mirror with a reflectivity varying from zero to almost one can be built due to the finite value of the conductivity of a metallic film . A behavior related to this fact, the disappearance of Fabry-Perot resonances probed by far-infrared continuous waves, was reported by Gorshunov et al. for superconducting NbN film  and by Dressel for VO2 layers  deposited on a sapphire substrate. In this contribution, we show theoretically and demonstrate experimentally that ultra-thin metallic films work as efficient wave-impedance matching layers in the terahertz and mid-infrared frequency regions.
2. Model of optical wave-impedance matching layer
We examine the case when a sub-10 nm metallic film is placed at the interface between two different optical materials with the complex refractive indices n 1 and n 2 (Fig. 1). The metallic layer thickness is chosen such that the penetration depth (known as skin depth) of the electromagnetic radiation is larger than the layer thickness. In this instance the reflection and transmission of electromagnetic radiation can be described using a standard model . The metallic layer is thus considered an ordinary optical layer, whose frequency response is described by the Drude model . The electric field ER of the reflected radiation is then given by
where E1 is the electric field of the incident radiation; rxy and txy are the Fresnel reflection and transmission coefficients (in general complex values) for an interface consisting of materials x and y; tM is the transmission coefficient through the metallic layer, and includes a phase shift as well as the attenuation losses of the electromagnetic wave as it propagates through the metal, i.e. tM = exp[i ∙ d ∙ 2π/λ 0 ∙(n + i ∙ k)∙ cosθM ] where n and k are the real and imaginary parts of the metal’s complex refractive index; d is the effective metal layer thickness; and finally θM is the angle satisfying the Snell’s law of refraction, n 1 ∙ sin θ 1 =(n + i ∙ k) ∙ sin θM=n 2 ∙sin θ 2. The reflection at the interface is suppressed when the nominator of Eq. (1) is equal to zero, i.e.
Several possible solutions of Eq. (2) exist. Assuming a lossless dielectric layer (k = 0), with r1M = rM2 the ideal refractive index of the matching dielectric layer is given by . In this instance dielectric layer thickness d should be set to d = (2m+1)*λ0/(4*n)*cosθM (m = 0,1,2, …) as is discussed in Ref. .
An alternative non-trivial solution exists that satisfies Eq. (2) for an absorptive layer (nonzero k). Assuming normal incidence, i.e. θM = 0, the following conditions for amplitude and phase arguments of the reflections coefficients hold
where ϕ1M and λM2 are the phases of reflection coefficients r1M and rM2. For an ultra-thin conductive layer (d ~ 1 - 10 nm) at terahertz frequencies (λ0 ~ 30 - 3000 μm or ν = 0.1 - 10 THz) we can easily satisfy (d * k/λ0)2 ≪1 and (d * n/λ0)2 ≪1, hence Eq. (3a) can be Taylor expanded to the first order of Exp argument to give
and phase arguments in (3b) have to satisfy an equation
Equation (4a) indicates that r1M has to be slightly smaller than rM2. This occurs when n1 > n2, i.e. for electromagnetic waves propagating from the optically denser material to the less dense one. For a particular metal, with given optical parameters, the difference in the reflections from the n1/metal and metal/n2 interfaces can be compensated for by varying the thickness of the metal film according to Eqs. (4a) and (4b). In Fig. 2(a) the total reflection coefficient, (calculated for 1.5 THz using our model) is plotted as a function of the conductance of the metal film for different refractive index ratios n1/n2. For these calculations we have chosen an arbitrary metal satisfying the Hagen-Rubens regime  at 1.5 THz, i.e. the real part of the metal conductivity σr is frequency independent and σr ≫ σi. The electric field of the reflected radiation changes amplitude and phase shifts by π as the sheet conductance and thus the thickness of the metallic layer increases. The position of the zero total reflection crossing point (ER=0) depends on the mismatch between the optical materials. Generally, if this mismatch is large, the conductance of the matching layer must also be made large to ensure proper matching between the materials.
One drawback of metallic wave-impedance matching layers is the energy loss due to absorption in the metal. This loss scales with the wave-impedance difference between optical materials. If the wave impedance difference between the optical materials is large then the matching conditions are more severe, requiring that a thicker metallic layer, with a correspondingly higher sheet conductance [see Fig. 2(b)], has to be used. This in turn leads to the larger absorption losses. This is illustrated clearly in Fig. 2(c) where the absorption loss in the impedance matching metallic layer is plotted as a function of the refractive index mismatch. We note that these losses are about twice the reflection losses incurred at the dielectric interface n1/n2 without an impedance matching layer.
The main advantage that the metallic wave-impedance matching film has over the standard λ0/4 dielectric antireflection layers is its superior frequency performance. The phase shift in the case of the λ0/4 dielectric antireflection layer scales as λ -1 0 . Since the metal plasma frequency is generally high (λplasma ~ 0.1 – 10 μm) [7–9], at THz frequencies we are in fact in the Hagen-Rubens regime  which implies n,k ~ λ 0 1/2 . That means that the frequency dependence of matching performance of the metallic layer is by principle weaker in comparison to the standard λ0/4 dielectric antireflection layer and the bandwidth is in fact √2 wider (see Fig. 3). The bandwidth in this case is defined as a frequency range where the total reflection coefficient is < 0.01.
The bandwidth of the metallic wave-impedance matching layer can be further increased if we assume that the left-hand side of Eq. (2) is equal to a small number, e.g. 10-2, instead of the somewhat stricter requirement that it be equal to zero. In this case the reflected power is four orders of magnitude smaller than the transmitted one which is satisfactory for most applications.Due to the magnitude of optical parameters (n,k ≫1) of metal in the Hagen-Rubens regime the phases of the reflection coefficients r1M and rM2 are very similar but of opposite sign. This situation is completely different from the case of the standard λ o/4 dielectric antireflection layers, in which the phase shift of individual reflections is zero. Therefore, the additional phase shift acquired by wave traveling in the metal layer, and necessary to achieve π phase difference of the waves reflected at individual interfaces n1/metal and metal/n2 is very small, usually several milliradians in the contrast to the standard antireflection layer. The frequency dependent phase argument in Eq. (4b) holds (4 ∙ d ∙ n/λ 0)≪ 1 in the case of thin metallic layer, while for the standard λ 0/4 dielectric antireflection layer it is of (4 ∙ d ∙ n/λ 0 ≈ 1. In practice this means that tolerating a small non-zero reflection coefficient allows the use of a metallic wave-impedance matching layer over frequency range orders of magnitude wider than the standard λ0/4 dielectric antireflection layer. The frequency dependence of the reflection coefficient shown in Fig. 3 (model details are in the figure caption) clearly demonstrates this fact. We call an ultra-thin metallic layer that reduced significantly the reflection of the electromagnetic waves at interface of two optically different materials as Metallic AntiReflection Coating (MARC).
At somewhat higher frequencies (in the relaxation regime of the metal response) k scales as λ 0 and n as λ 2 0. Therefore, the term in the parenthesis on right-hand side of Eq. (4a) is frequency independent in the relaxation regime. The phase of the reflection changes [Eq. (4b)] stays frequency dependent, but if [4∙d∙n/λ 0)≪1 still hold and the metallic layer could be used as a broadband antireflection coating also at frequencies within the relaxation regime of the metal response.
3. Experimental results
The effect of an ultra-thin metallic layer on the reflection coefficient at an interface of two different optical materials was studied for two different material systems: First, a series of the highly resistive (resistivity > 3000 Ocm) silicon plates were coated on one side with a chromium film with thicknesses ranging from 2 to 20 nm. The high resistive silicon is used because at THz frequencies it is transparent and has negligible dispersion. Chromium was chosen due to its excellent coating capability, allowing the thickness and the sheet resistance to be accurately controlled. The second chosen material system is highly resistive GaAs coated with indium-tin-oxide (ITO). Undoped GaAs is exhibits low absorption and dispersion at THz frequencies. Indium-tin-oxide is a material with a metal-like conductivity, but is transparent in the visible and near-infrared wavelength unlike the most metals. Recently, ITO was used for dichroic near-infrared/THz mirrors .
The THz performance of the chromium and ITO layers was measured using a transmission THz-TDS system with a photo-conductive gallium-arsenide emitter and a 300-μm thick gallium-phosphide electro-optic electric field sensor. This THz setup enables spectral sensing range 0.1 to 7 THz with an SNR>1.
The time-domain signal measured with this type of experimental setup typically consists of several THz pulses; the main pulse transmitted through sample and followed by a train of successive pulses of decreasing amplitude. Each of these successive pulses is delayed from main pulse by a multiple of the round-trip time within the sample. In Fig. 4(a) the amplitudes of the main and the first reflected THz pulses are shown. Amplitudes of both pulses are normalized with respect to the amplitude of the main THz pulse transmitted through the uncoated silicon plate. As expected, the amplitude of the main transmitted THz pulse decreases as thickness of the chromium and ITO film increases due to absorption losses in the metal film. The amplitude of the reflected THz pulse also decreases, goes through zero, and after a change of polarity it raises again in coherence with the theoretical predictions shown in Fig. 2. For a chromium layer thickness of about 8.3 nm the reflection of THz pulse from the system silicon/chromium/air vanishes. The same behavior was observed for the material system GaAs/indium-tin-oxide. Since the conductivity of the ITO is smaller than that of chromium, the optimal thickness of ITO for the reflection cancellation is relatively large ~ 44 nm [Fig. 4(b)].
We have compared our experimental data with the results predicted from the model and we found good agreement between them. We attribute any recognized differences to the limited validity of the Drude model [6, 8] at the THz frequencies, especially when the input model parameters (scattering rate, carrier density at Fermi surface) that we used, were obtained from measurements of DC conductivity of the chromium and ITO layers. In addition, deviation of the optical parameters of a metal from the Drude model is usually observed for the transition metals like chromium . Therefore, the optimal thickness of metal film for a given sample material almost always has to be estimated experimentally.
The measured THz signal, transmitted through both a coated and uncoated silicon plate, is presented in Fig. 5(a) (see caption for details). For the uncoated sample (red line) a secondary pulse can be seen approximately 9 ps after the initial pulse. However when the silicon plate is coated with a 8.3 nm of chromium, which corresponds to the optimized thickness, the secondary pulse is completely suppressed (black line).
Similarly in Fig. 5(c) we present the measured THz signal for a coated (44 nm thick ITO layer) and uncoated GaAs sample. By comparing the coated (red) and uncoated (black) traces in Fig. 5(c) it is evident that the second reflected pulse has also disappeared. These experimental results clearly demonstrate the effectiveness of our wave-impedance matching technique.
In Figs. 5(b) and 5(d) we demonstrate the effect of our coatings on the spectral characteristics of the THz signal. The spectral response for the coated sample is normalized with respect to the spectral response for the uncoated sample and presented as a spectral “ratio”. This spectral ratio stays approximately constant over a 4 THz range (0.4 to 4.5 THz) proving frequency independent behavior of the metallic coating. We note that analysis of measurement data at frequencies below 0.4 and above 4.5 THz is limited by the SNR of data.
The effectiveness of the ITO based MARC is also demonstrated for an electro-optic GaP crystal. This non-linear optical material can be used as a broadband detector of the coherent terahertz radiation by exploiting the Pockel effect [11, 12]. To ensure operation over a large bandwidth, the GaP crystal has to be thin . This however reduces the quality of the time-domain signal due to reflections of THz radiation from the crystal/air interfaces. Recently, we proposed a solution to this problem using an ultra-thin chromium film . One major drawback to this solution is the loss of about 45% of the near-infrared (λ=800 nm) probe power due to the chromium film. By replacing the chromium film with an ITO based MARC this 45% loss can be avoided, improving the detector performance. In Fig. 6 the time-domain response of the THz pulse detected at 300 μm thick GaP, with and without an applied ITO based MARC, is shown.
Finally, we demonstrate how the MARC can be used effectively for Fourier transform infrared spectroscopy (FTIR) in the mid infrared frequency range. The spectral characteristics of 370 μm thick GaAs wafer used as a beam splitter were estimated over the range 5 – 20 μm using FTIR. The measured spectrum, shown in Fig. 7, is strongly modulated by Fabry-Perot oscillations that arise due to interferences within the wafer. In the uncoated sample (red line) the absorption line of CO2 molecule at 14.978 μm is barely visible, inhibiting standard quantitative analysis of the CO2 concentration . If the same GaAs beam splitter is now coated with a MARC, the overall signal strength drops, but the Fabry-Perot oscillations are completely removed and good quality spectrum is obtained.
In summary, we have shown that the amplitude and phase of few-cycle THz pulses reflected at dielectric interfaces covered with a metal film can be efficiently minimized by controlling the film thickness. We modeled this behavior using Fresnel formulae applied to the stratified medium. We demonstrated experimentally that ultra-thin chromium and ITO films can be used as an efficient broadband antireflection coating for optical components in the terahertz frequency range.
The authors acknowledge financial support from the European commission (IST-511415 “Teranova”), the Austrian “Fonds zur Förderung der Wissenschaftlichen Forschung” (project SFB-ADLIS) and the “Gesellschaft für Mikroelektronik”.
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