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Broadband high reflectivity in subwavelength-grating slab waveguides

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Abstract

We computationally study a subwavelength dielectric grating structure, show that slab waveguide modes can be used to obtain broadband high reflectivity, and analyze how slab waveguide modes influence reflection. A structure showing interference between Fabry-Perot modes, slab waveguide modes, and waveguide array modes is designed with ultra-broadband high reflectivity. Owing to the coupling of guided modes, the region with reflectivity R > 0.99 has an ultra-high bandwidth (Δf / ̅f > 30%). The incident-angle region with R > 0.99 extends over a range greater than 40°. Moreover, an asymmetric waveguide structure with a semiconductor substrate is studied.

© 2015 Optical Society of America

1. Introduction

Subwavelength structures are of interest in a wide range of theoretical fields and applications, including cavity quantum electrodynamics, polariton lasers, filters, splitters, and couplers. Recently, high-contrast subwavelength gratings (HCGs) have been used as reflectors in quantum cavities [1], vertical-cavity surface-emitting lasers (VCSELs) [2], and optomechanical nanoresonators [3], replacing the conventional distributed Bragg reflectors because of its remarkable performance in terms of dispersion, reflectivity, and bandwidth [4]. HCG reflectors can introduce ultra-high dispersion to quantum cavities, which can be engineered to control the cavity performance by, for example, modifying phase and group velocities [5], controlling the density of states (DOS) of the photonic modes [6], and creating synthetic magnetic fields [7]. In addition, for tunable etalon-type device applications, such as lasers, filters, and detectors, the tuning range is significantly extended using HCG broadband reflectors. However, HCG reflectors need a sacrifice layer [8] (generally an air gap), which complicates the fabrication of an integrated device, and HCG can hardly be made into a membrane owing to its discontinuous structure.

Recently, a numerical algorithm was developed to simulate rectangular gratings based on the choice of propagation mode-set [9], which converges much faster than the Rigorous Coupled Wave Analysis (RCWA) does for HCG. The results demonstrated that the interference of the first two propagation modes in the grating, which are called waveguide-array (WGA) modes [1, 9], causes the broadband reflection of HCGs. The WGA modes are coupled between grating bars and gaps and have a similar dispersion relation with slab waveguide modes. In this Letter, we develop a subwavelength-grating slab waveguide structure. Ultra-broadband high reflectivity is realized through the interference between Fabry-Perot modes,WGA modes and guided modes. The structure is much easier to fabricate and integrate into optoelectronic components. Also, the incident-angle range with high reflectivity is significantly extended.

In the following, we first investigate the similarity between guided modes and WGA modes, and show that high-Q resonances and high-reflectivity bands exist, owing to the interference between Fabry-Perot modes and guided modes. Furthermore, as the thickness of the grating layer increases, an ultra-broadband reflectivity with large incident-angle region is obtained through the coupling between guided modes, WGA modes, and Fabry-Perot modes. Moreover, the structure is easy to fabricate and to integrate into optical system. Last, we integrate our structure on a GaAs substrate. The broadband reflection is realized due to the coupling of asymmetric-slab-waveguide modes.

2. Effect of slab waveguide modes

A schematic of our proposed structure is shown in Fig. 1(a). All length units are normalized by the grating period (Λ) with the following parameters: grating-layer thickness h1, and slab-waveguide-layer thickness h2. Figure 1(b) shows the reflectivity contour map against the normalized frequency (by 2πc/Λ) and slab-layer thickness for a surface-normal TM-plane wave incident onto the free-standing structure using RCWA [10]. The permittivity εr of both grating and slab material is 11.9 (Si), grating thickness h1/Λ is 0.167, and a duty cycle η is 0.5 (in this paper, η=0.5 is always true unless otherwise mentioned). Three regions can be clearly identified with different wave vectors in the propagation direction kz, which is defined as

kz2=(2πni/λ)2(2πm/Λ)2.
where λ is the wavelength, m is the diffraction order, and niis the refraction index of the material in each layer, which is unity in air. For λ>Λneff (the left region in Fig. 1(b), where neff is the effective refractive index of the structure), kz is always imaginary when m>0. The reflection shows classical Fabry-Perot dispersion. The curve for reflectivity versus frequency and slab thickness displays an approximate 1/f line shape. For λ<Λ (the right region in Fig. 1(b)), kz can be real in air when m>0. Thus, high-order diffraction exists in the transmission, which reduces the total contrast of the peaks and dips. For Λ<λ<Λneff, kz is imaginary in the transmission region (air below), but it can be real in the slab layer when m>0. Therefore, a real kx (or k//) is introduced into the slab layer. The imaginary kz in the transmission region ensures that the wave power is entirely confined in the zero-order diffraction. The real kz and kx in the slab layer lead to the coupling of guided modes, resulting in intricate transmission properties.

 figure: Fig. 1

Fig. 1 (a) Schematic of the free-standing grating slab waveguide structure. (b) Reflectivity contour of the structure as a function of frequency and slab-layer thickness simulated using RCWA, with TM-polarized, surface-normal incident waves and the parameters h1=0.167Λ, εr=11.9, and η=0.5. The contour map shows a dispersion shape of guided modes but with some cut-off frequencies (dashed lines), which has affinities with the dispersion of WGA modes. Intricate transmission properties occur in the Λ<λ<Λneff range owing to interference.

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The guided modes introduced by the slab layer have a similar dispersion with WGA modes [1]. The WGA modes supported by the high refractive index grating bars are essential to transmission properties of HCGs [9]. For HCG reflectors, the broadband high reflectivity range results from the interference between the zeroth and first order of WGA modes, which is called “dual mode” regime. The dispersion curves shown in Fig. 1(b) illustrate a clear line shape of guided modes with different cut-off frequencies for each curve group, compared to WGA modes. These three cut-off lines in the region represent m = 1, 2, 3 (k//=2πm/Λ). In each m-order diffraction group, different order waveguide modes exist and have the same cut-off lines, similar to the dispersion of ordinary guided modes. The detailed reflection characteristics resemble those of WGA dispersion. Characteristics common with the WGA modes include (1) the cut-off frequency mentioned above; (2) the existence of a so-called “dual mode” regime, in which high reflectivity occurs; and (3) the occurrence of crossings (when m = 1, 3 or 0, 2 intersect) and anti-crossings (when m = 0, 1; 1, 2; or 2, 3 intersect) when different m-order mode curves intersect [11]. Anti-crossings are usually known to be indicators of strong coupling, which results in broadband high reflectivity or high-Q resonances.

In the present study, the grating-layer thickness is set to 0.167Λ. Thus, the grating layer can be simply considered to provide the parallel wave vector in the structure via diffraction, which is demonstrated by the dispersion curves of classical guided modes. In this case, the so-called “dual mode” interference occurs between Fabry-Perot modes (m = 0) and the guided modes of high order diffraction (m > 0). The dispersion relation shown in Fig. 1(b) illustrates that when the curve of the Fabry-Perot modes (the dark blue region in the contour map) encounters the first-order diffraction mode, anti-crossings occur [11]. Moreover, when these two curves show similar slopes, broadband high reflectivity occurs at the intersection; otherwise, high-Q resonances occur. Fabry-Perot modes are weak-coupling resonances, and when the waveguide-mode curves cross the curves of the Fabry-Perot modes with different slopes, they play the role of discrete resonance, as in Fano resonances [12]. On the other hand, when two types of modes have similar dispersion slopes, the reflected wave phases of two different orders interfere with each other, attenuating the transmission power in a large frequency range. Therefore, dispersion relations can be engineered for various applications by modifying the parameters of the structure.

3. Interference between WGA modes and slab waveguide modes

In the case above, the grating layer mainly has two effects: (1) introducing the parallel wave vector through diffraction and (2) modifying the effective index of the entire structure. Because of the small thickness of the grating layer, the wave phase produced by the grating layer is not considerable. With increasing grating-layer thickness, the wave phase introduced by the grating cannot be neglected, which will introduce mode coupling in the grating bars (WGA modes). Moreover, the grating layer influences the effective index, which determines the Fabry-Perot dispersion curves. The interference between WGA modes and Fabry-Perot modes can yield broadband high reflectivity, and this interference has been utilized as mirrors in quantum wells [13] and VCSELs. The additional slab layer on the HCG, which introduces the coupling of guided modes, not only modifies the dispersion relation but also improves the reflector performance. The simulation result in Fig. 2(a) shows the reflectivity contour map versus the normalized frequency (2πc/Λ) and slab-layer thickness h2 for a surface-normal incident TM-plane wave, with the material permittivity εr = 11.9 (Si) and grating-layer thickness h1 = 0.685Λ. Two cut-off lines (λ = Λneff and λ = Λ) are observed, which divide the contour map into three parts. As mentioned above, an increasing grating thickness modifies the dispersion curves. Thus, the position and slope of the curves of the Fabry-Perot modes have significantly changed. Moreover, as the grating thickness increases, the WGA modes, which exist in the high-refractive-index bars and air gaps, provide more complicated coupling. As shown in the contour map, when the slab layer is thin (in the bottom area), a high-reflectivity region due to the WGA exists. As the slab-layer thickness increases, guided modes emerge, couple with WGA modes, and significantly expand the high-reflectivity range. In this case, the reflection is determined by interference among the Fabry-Perot modes (m = 0), waveguide modes (m > 0), and WGA modes (grating contribution). We cannot distinguish guided modes from WGA modes in Fig. 2(a) because of their similar dispersion relations. These three modes affect the wave phase together and lead to ultra-broadband high reflectivity.

 figure: Fig. 2

Fig. 2 (a) Reflectivity contour as a function of frequency and grating-layer thickness with h1 = 0.685Λ. The thick grating layer can sustain WGA modes, which are essential for HCGs. The interference among guided modes, WGA modes, and Fabry-Perot modes leads to the broadband high reflection (dark red area). (b) Reflectivity with the parameters described in (a) for three different configurations: h2 = 0.45Λ and η = 0.5(black line), h2 = 0.5Λ and η = 0.5 (red dashed line), and h2 = 0.45Λ and η = 0.55 (blue dash-dotted line).

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Owing to the guided modes, the high-reflectivity range is larger than those attained with only WGA modes as traditional HCG gratings. The black curve in Fig. 2(b) shows the reflectivity at a fixed slab-layer thickness (h2 = 0.45Λ). The high-reflectivity (R > 0.99) bandwidth (Δf/f¯) is greater than 30%. In addition, all the simulations are performed with normalized units. Therefore, the structure can be easily designed by adjusting Λ for a certain frequency. For example, for the traditional optical communication range, we set the central wavelength as 1.55 μm; then, the high-reflection range is from 1.31 μm to 1.79 μm, with the structure parameters Λ = 0.698 μm, h1 = 0.478 μm, h2 = 0.314 μm, and εr = 11.9. We consider variations of up to 10% in the slab thickness h2 and grating duty circle η. The red dashed line and blue dash-dotted line show the influence of h2 and η, respectively. Owing to the complicated interference, there still remains a large range of high reflectivity. In fact, the fabrication technology could control the error within 5% in the parameters for a central wavelength of 1.55 μm. The permittivity here is chosen as that of silicon. Moreover, silicon and many other semiconductor materials have a high refractive index (2.8~3.5) and show little dispersion from the infrared region to the terahertz region. Thus, by modifying Λ (about 100 times that at 1.55 μm), this structure can also be used in the terahertz region.

The waveguide modes introduce rather intricate phase interference to the reflection, some of which significantly benefits the structure as a reflector. Figure 3(a) and Fig. 3(b) show contour maps of the reflectivity as a function of frequency and incident angle at the high-reflectivity frequency region with h1 = 0.685Λ, h2 = 0.45Λ and h1 = 0.685Λ, h2 = 0, respectively. The contour maps indicate that the angle tolerance greatly increases with the aid of the slab layer, compared to the case of only a WGA (HCGs), owing to the coupling of guided modes. At a frequency of approximately 0.5 × 2πc/Λ with the structure parameters in Fig. 3(a), the angle tolerance is up to 40°, as shown in Fig. 3(c). This huge incident-angle redundancy provides flexibility in integrating components. In addition, the large phase shift produced by the large angle introduces more dispersion properties of cavity quantum electrodynamics systems using this reflector.

 figure: Fig. 3

Fig. 3 (a) Reflectivity contour as a function of frequency and incident angle with the parameters h1 = 0.685Λ and h2 = 0.45Λ. (b) Reflectivity contour as a function of frequency and incident angle with the parameters h1 = 0.685Λ and h2 = 0 (HCGs). (c) Reflectivity as a function of incident angle at a frequency of 0.5×2πc/Λ. The high reflection angle region is significantly expanded because of the slab waveguide modes.

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The transmission properties of the free-standing structure benefit from the symmetric slab waveguide modes. In addition, the gratings fabricated on a substrate, shown in Fig. 4(a), can be regarded as an asymmetric waveguide, which has similar influence on the properties of reflection. Figure 4(b) shows the reflectivity contour with a substrate of permittivity εr = 10.8 (GaAs) as a function of frequency for a grating with parameters h1 = 0.685Λ and h2 = 0.45Λ. The normally incident electromagnetic wave propagates from the substrate material to the structure and into air. As shown in Fig. 4(b), there also exist several high-reflectivity areas and the same cut-off lines in the contour map, which implies that the asymmetric waveguide modes can be exploited to design a reflector. Moreover, this structure with a slab-waveguide layer and substrate layer can be easily used for integrated components through electron-beam deposition, molecular-beam epitaxy, or some other modern membrane-growth technology.

 figure: Fig. 4

Fig. 4 (a) Schematic of the asymmetric waveguide structure. (b) Reflectivity contour of the structure with a substrate (εr = 10.8) as a function of frequency and grating thickness with h2 = 0.45Λ.

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4. Conclusion

In summary, we proposed a subwavelength-grating slab waveguide structure, calculated its reflection properties, and analyzed the effect of slab waveguide modes. The interference between guided modes and Fabry-Perot modes lead to complicated reflection properties including broadband high reflectivity. An ultra-broadband (Δf/f¯>30% with R > 0.99) high reflectivity was observed with phase interference among the guided modes, Fabry-Perot modes, and WGA modes. On introducing the guided modes, the angle tolerance significantly increased, which implies that R > 0.99 is maintained at incident angles greater than 40°. Moreover, we simulated an asymmetric waveguide setup and observed high-reflectivity areas. Because of the guided modes introduced by the slab-waveguide layer, a feasible dispersion can be realized; thus, our structure is promising for use in quantum cavities and integrated components.

Acknowledgments

This work was supported by the National Natural Science Foundation of China (Grant Nos. 50902034 and 11074059), the Science Fund for Distinguished Young Scholars of Heilongjiang Province (Grant No. JC200710), and the Program for Innovation Research of Science in Harbin Institute of Technology. The authors thank the Laboratory of Micro-Optics and Photonic Technology of Heilongjiang Province for help in the calculation.

References and links

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Figures (4)

Fig. 1
Fig. 1 (a) Schematic of the free-standing grating slab waveguide structure. (b) Reflectivity contour of the structure as a function of frequency and slab-layer thickness simulated using RCWA, with TM-polarized, surface-normal incident waves and the parameters h 1 =0.167Λ , ε r =11.9 , and η=0.5 . The contour map shows a dispersion shape of guided modes but with some cut-off frequencies (dashed lines), which has affinities with the dispersion of WGA modes. Intricate transmission properties occur in the Λ<λ<Λ n eff range owing to interference.
Fig. 2
Fig. 2 (a) Reflectivity contour as a function of frequency and grating-layer thickness with h1 = 0.685Λ. The thick grating layer can sustain WGA modes, which are essential for HCGs. The interference among guided modes, WGA modes, and Fabry-Perot modes leads to the broadband high reflection (dark red area). (b) Reflectivity with the parameters described in (a) for three different configurations: h2 = 0.45Λ and η = 0.5(black line), h2 = 0.5Λ and η = 0.5 (red dashed line), and h2 = 0.45Λ and η = 0.55 (blue dash-dotted line).
Fig. 3
Fig. 3 (a) Reflectivity contour as a function of frequency and incident angle with the parameters h1 = 0.685Λ and h2 = 0.45Λ. (b) Reflectivity contour as a function of frequency and incident angle with the parameters h1 = 0.685Λ and h2 = 0 (HCGs). (c) Reflectivity as a function of incident angle at a frequency of 0.5×2πc/Λ . The high reflection angle region is significantly expanded because of the slab waveguide modes.
Fig. 4
Fig. 4 (a) Schematic of the asymmetric waveguide structure. (b) Reflectivity contour of the structure with a substrate (εr = 10.8) as a function of frequency and grating thickness with h2 = 0.45Λ.

Equations (1)

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k z 2 = (2π n i /λ) 2 (2πm/Λ) 2 .
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