2.1. Selecting the Material and Geometry
Traditional nonlinear materials are generally classified into organic and inorganic categories. Inorganic nonlinear materials can be further categorized into dielectric materials, including LNB, BBO, and barium titanate (BTO), as well as Group III–V and Group II–VI semiconductors, such as InP, CdTe, and gallium arsenide (GaAs). Some of the traditional nonlinear materials and their main properties are listed in
Table 1 [
8].
In addition to traditional χ(2) materials, which typically exhibit relatively low nonlinearities, there are engineered quantum well heterostructures, such as JRD1 in polymethylmethacrylate, demonstrating nonlinearities that are 10–100 times greater than those of traditional χ(2) materials [
9]. However, these specific, engineered, quantum well heterostructured materials were not considered in this study.
The optimum geometry of a MZM is varied by the selected material. For example, a model optimized for LNB is not optimized for other EO materials. No matter what geometry is selected, it must be optimized for the maximum transmission and minimum loss in the guiding mode.
Figure 1 compares the geometry of a conventional MZM with that of the MZM used in the model developed in this study.
Figure 2 shows the other geometries of the light modulators based on BTO, PZT, organic EO materials, and LNB, as presented by other researchers [
9,
10,
11,
12].
2.2. Selecting the Type and Architecture of the Modulator
Generally, the traditional light modulator has a bandwidth of around 35 GHz. In contrast and in theory, integrated CMOS-compatible light modulators can have a bandwidth of greater than 100 GHz, and their voltage length parameter (V.l) is between 1 to 3 V·cm, depending on its type, geometry, material, and electrode type [
13].
Optical modulators manipulate the output amplitude or phase of light waves as they pass through the device. Waveguide-based modulators are used in communication applications to reduce the size and required driving voltage. An EO effect, such as the Pockels effect, is utilized to control the refractive index of the waveguide with an external electric signal, where the crystal’s birefringence changes with the applied electric field. This change in the refractive index alters the phase of the wave passing through the crystal. An amplitude modulation can be achieved through interference by combining waves with different phases.
Figure 3 shows the architecture of a light phase modulator, an intensity modulator, and a combined phase and intensity modulator. The intensity modulator is more complicated because it consists of a phase modulator on one arm.
A CMOS-compatible Mach-Zehnder intensity modulator (MZM) was considered in this design and simulation model.
Figure 4 illustrates the configuration of the MZM pursued in this study. Initially, the input optical wave is directed to a directional coupler, where its intensity is evenly split between the two output waveguides. These waveguides constitute the two arms of a Mach-Zehnder interferometer. One of the arms allows for the application of an electric field, enabling the modification of the refractive index in the material and consequently altering the wave’s phase propagating through that specific arm. The two waves are subsequently merged using another 50/50 directional coupler. By adjusting the applied voltage, precise control over the amount of light exiting from the two output waveguides can be achieved.
As mentioned, six traditional χ(2) materials, including LNB, KNB, LTO, BBO, CdTe, and InP, were considered for this waveguide modulator. In the MZM, a confined mode propagates through one of those six types of EO crystal, and the cladding comprises a doped crystal with a lower index. The optical wavelength (λ) is considered to be 1.55 µm. In order to achieve a state where the field of confined modes exhibits zero magnitude at the exterior boundaries, it is imperative to employ a cladding radius of adequate size. As boundary conditions, it is vital to ensure a rapid decay of the electric field amplitude with respect to the cladding radius coupled with an absolute zero electric field outside the cladding region. These conditions have been implemented to maintain adherence to the prescribed theoretical framework and uphold the integrity of the system under analysis.
In a confined mode, there is no energy flow in the radial direction, making the wave evanescent in the radial direction within the cladding. This condition holds true only if the effective index (
) is greater than the index of the cladding (
). Conversely, the wave cannot be radially evanescent in the core region. Therefore, the effective index must be between the index of the core and that of the cladding (
). It is important to note that a higher effective index results in a more confined optical wave, with the fundamental mode having the highest effective index. The effective refractive index of a confined mode is calculated in Equation (1):
where
is the vacuum wavenumber, and
is the propagation constant. The
is a function of the frequency. The normalized frequency of a waveguide or the V-number is calculated in Equation (2):
where
a is the radius of the core. The mode analysis is conducted on a cross-sectional plane (xy-plane) of the fiber, specifically examining the behavior of the optical wave in the z-direction. The optical wave can be characterized by the following expression:
Within the provided context,
w is defined as 2πν, representing the frequency of the optical wave denoted by ν. In order to determine the eigenvalues for the electric field, the Helmholtz equation (Equation (4)) is solved, yielding the eigenvalues of (−iβ).
In order to model the MZM, the interface for the optical waves’ beam envelopes is formulated by assuming that the electric field can be represented as the product of a slowly varying envelope function and a rapidly varying phase function, as per Equation (5).
In Equation (5), the envelope function,
, represents the electric field, where
k denotes the wave vector, and
r represents the position. When the wave vector
k is appropriately chosen for the specific problem, the envelope function,
, exhibits spatial variation on a larger length scale compared to the wavelength. In this application, it is reasonable to assume that the wave can be accurately approximated in straight domains by utilizing the wave vector corresponding to the incident mode of β. However, in waveguide bends, assuming α is the bend angle from the x-axis and
and
are unit vectors in the x and y-directions, the wave vector can be expressed as
. Therefore, the wave vector difference in the bent waveguide will be the following:
determines the phase variation for the envelope electric field. The splitting and recombining of light in a guiding mode inside the waveguide is the most complicated task in the model. Steering the incoming photonic intensity toward unusual directions, which is not predicted by Snell’s laws of reflection and refraction in various wavefront engineering applications, can be described with the integral equation formulation presented by Tsitsas and Valagiannopoulos (2020) [
14].
The initial step in the model developed in this study is to optimize the waveguide’s bending ratio. This is based on the wavelength, the waveguide’s core, and a width that ensures a 50–50 light split in a guiding mode using a numerical model created in COMSOL multiphysics [
15]. This COMSOL model calculates the phase modulation from the optical path difference (OPD) resulting from the change in the index (n) of the EO medium with an appropriate EO coefficient of
due to the imposition of an external electric field and the length of propagation (l) through the EO medium under the voltage (V), as per Equation (7) [
16].
where D is the distance between the electrodes surrounding the EO medium. The COMSOL model defines the intensity modulation after recombining the two arms if the transmission at the outlet port drops to zero.
The OPD required for modulation in the MZM is expressed as the voltage-length product (Vπ·L) [
17]. This value was calculated for each EO material studied based on the assumed geometry. Note that both the choice of EO material and the geometry affect the half-wave voltage (Vπ), causing variations in the voltage-length product for the EO materials examined in this paper.
2.3. Selecting the Type of Electrodes
The lumped or traveling wave (TW) electrodes can be used in the MZM. Lumped MZMs have a smaller length than the wavelength of the modulation field due to the low modulation frequency (
f). This results in a longer modulation period (1/
f) than the transit time (
, which is the duration for the optical wave to propagate through the MZM.
Generally, the 3 dB modulation bandwidth (
) of an MZM depends on both transit time (
) and the RC time constant (
). Since the RC time is much longer than the transit time in a lumped MZM, the modulation bandwidth is defined by the RC time constant as
For a fixed resistance, the gets longer by increasing the length (l) of the electrodes due to increasing the capacitance by length (). Therefore, . On the other hand, the optical path delay (OPD) increases by length (l) for a given index change, as per Equation (7). Thus, the length of the electrode would be a trade-off between the modulation bandwidth, the required OPD for phase modulation, and the voltage to impose the index change in a lumped MZM; hence, the modulation bandwidth of a lumped MZM cannot be greater than a few gigahertz.
As seen, to achieve higher bandwidth modulation, the lumped modulator’s frequency response is limited by its RC characteristics at high modulation frequencies. In order to overcome this limitation, a traveling wave configuration is used for the MZM. This involves matching the phase velocity of the microwave modulation field or radio frequency (RF) wave with that of the optical wave in the MZM. The MZM with traveling wave-type electrodes is called TW-MZM [
18]. This type of electrode was selected for the MZM in this study.
In order to enable effective interaction between the microwave field and optical wave in a TW-MZM, the high-frequency modulation signal is injected and propagates in the same direction as the optical wave, terminating at the end of the electrode transmission line [
19].
The modulation bandwidth
of a TW-MZM depends on the mismatch between the phase-velocity of the optical wave propagating in the waveguide and the RF wave propagating in the transmission line, as well as the loss of RF signal along the transmission line depending on the frequency of the RF wave. The velocity mismatch and the RF attenuation also depend on the materials and geometry of the waveguide and the transmission line [
4]. Considering Z as the impedance of the transmission line (
,
L as inductance,
C as capacitance per unit of length of transmission line,
as the index for the RF wave, and
as the effective index of the optical wave, the phase velocity of the RF (
) and the optical wave in the guided mode (
) can be calculated as
Considering the frequency-dependent absorption coefficient of α for the RF wave in the transmission line, the voltage attenuation coefficient will be 0.5 α, and therefore, the traveling voltage throughout the electrode as a function of time and space will be
where
is the peak of the modulation voltage, and
is the angular modulation frequency. That variation in voltage in time and space will impose a variable change in the propagation in time, space, and also frequency due to the dependence of the phase velocity of RF on frequency (
). The
would impose the maximum electric field to the EO medium and achieve the maximum index change (
) and, therefore, the maximum change in the propagation constant (
).
The max change in the propagation constant results in the max phase shift (
):
The optical wave entering the entrance port at the time of
t will get to the point of
z at
, where the voltage at that point is
Therefore, the change in the propagation constant will be
Therefore, the phase modulation will be
In order to estimate the maximum modulation bandwidth of TW-MZM, two limitation cases can be considered: having a velocity mismatch between the RF and optical waves () but a very low loss transmission line (α ≈ 0), as in Case 1, and having minimum velocity mismatch () but a lossy transmission line (), as in Case 2.
- i.
Case 1: The phase modulation in this case is
After conducting a lengthy analytical calculation, one can demonstrate that the modulation bandwidth of the TW-MZM, in this case, is calculated as follows:
The equation above shows that achieving velocity matching between RF and optical waves in a TW-MZM using a low-loss transmission line can significantly increase modulation bandwidth. Employing low-loss RF transmission methods, such as radio-over-fiber (RoF) [
20] techniques, in such systems further enhances this effect, leading to exceptionally high modulation bandwidth.
- ii.
Case 2: The phase modulation in this case is
Therefore, in this case, the modulation bandwidth of the TW-MZM will be inversely proportional to the square of the length.
Therefore, if the phase velocity of the RF and optical waves in a TW-MZM are matched, the modulation bandwidth will be limited solely by the square of the length of the transmission line.
However, the transmission line cannot be too short due to the necessary OPD for phase modulation. In order to meet the OPD requirements while reducing the transmission line length, exhibiting a medium with a higher index change will be advantageous.
2.4. Velocity Matching between the RF and Optical Wave
As mentioned, the optical wave’s group velocity and the microwave’s phase velocity must be matched to increase the modulation bandwidth. The maximum bandwidth of the TW-MZM will be the frequency of the RF wave, which has a phase velocity matched to the group velocity of the optical wave [
7].
The velocity of the optical wave is defined by the optical wave’s effective index in the waveguide, which is defined by wavelength(s), the propagation mode, the core size, and the refractive index of the core and cladding, which can be calculated independently of RF propagation. On the other hand, the RF phase velocity is a function of substrate thickness and the type and size of the electrodes, cladding sizes, and refractive indices, which can be modeled after calculating the optical wave propagation. Therefore, the materials and the thickness of the SiO
2 can be controlled to get the velocity of the RF and optical waves matched together, as schematically shown in
Figure 5.
The thickness of the SiO
2 layer in a TW-MZM, as depicted in
Figure 1a, does not impact the optical wave’s propagation constant. However, it does affect the phase velocity of the RF wave. Adjusting the SiO
2 layer’s thickness makes it possible to achieve velocity matching between the optical and RF waves to optimize the modulation bandwidth.
As shown in
Figure 1a, it is essential to note that the SiO
2 layer in the TW-MZM considered in this study is not positioned on top of the nonlinear layer, unlike conventional MZMs. Therefore, altering the SiO
2 thickness does not affect the propagation constant of the optical wave; instead, it solely controls the propagation constant of the RF wave (
Figure 5).
Wang et al. (2018) and Pascher et al. (2003) [
7,
13] conducted similar studies, where they optimized the SiO
2 layer thickness in a thin-film TW-MZM to attain velocity matching between the RF and optical waves to maximize the modulation bandwidth. Wang et al. (2018) [
13] focused on a TW-MZM with an assumed geometry and LNB as the EO medium, while Pascher et al. (2003) [
7] explored a different geometry using InP as the EO medium.
2.5. The Loss Estimation Method for the RF and Optical Waves in the TW-MZM
In the TW-MZM depicted in
Figure 4, the input optical wave, characterized by a known intensity, is introduced through one of the inlet ports. The COMSOL model can compute the intensity of the outgoing light from both outlet ports. Consequently, the optical loss can be determined as the disparity between the input and output intensities. This variation can be visually presented by plotting the optical loss along the length of the directional coupler waveguide.
Although the calculation of optical loss, as described earlier, appears straightforward, determining the loss of the radio frequency (RF) wave is more complex and requires evaluating the RF propagation constant following velocity matching. Assuming the complex RF propagation constant is
, the RF field will be
As the intensity of the radio frequency (RF) wave is directly proportional to the square of the field, the RF intensity follows an exponential decay as per the Beer–Lambert law.
Therefore, the RF absorption coefficient will be and is reported in terms of dB/mm.
In this model developed in COMSOL multiphysics, the loss associated with the RF wave is computed as described above for the six EO crystals under investigation. The calculations involve optimizing the shape and adjusting the thickness of the silicon dioxide layer (or the silicon layer in the case of CdTe) to achieve a velocity matching between the RF and optical waves, and the results will be compared.