Introduction

Global data traffic continues to grow at double-digit annual rates1, driven by cloud-based service delivery, video on demand, or Internet-of-Things (IoT) applications. To keep pace with this evolution, transceivers on all levels of optical networks are subject to the same challenge: To radically increase data rates, while maintaining acceptable technical complexity and energy consumption. In long-reach core and metropolitan networks, this challenge can be met by advanced modulation formats that exploit advances in high-speed digital signal processing (DSP) and advanced photonic integration. These approaches have led to transmission demonstrations at data rates in excess of 500 Gbit/s on a single polarization, using, e.g., 64-state quadrature amplitude modulation (64QAM) in conjunction with symbol rates up to 100 GBd2,3. When it comes to short-reach transmission over distances of a few kilometers or less in data centers or campus-area networks, however, higher-order modulation formats and the associated coherent reception techniques are prohibitive in terms of technical complexity and power consumption of the DSP. As a consequence, short-reach transmission largely relies on simple on-off-keying (OOK) as a modulation format that can be directly detected with a single high-speed photodiode. Such schemes are at the heart of current transceivers, e.g., for 100 Gbit/s Ethernet interfaces, that usually exploit low-cost vertical-cavity surface emitting lasers (VCSEL) or silicon photonic modulators to generate four spatially or spectrally separated data streams of 25 Gbit/s4,5,6. For future interfaces operating at data rates of 400 Gbit/s, 800 Gbit/s or 1.6 Tbit/s, however, parallelization of 25 Gbit/s channels is not a sustainable option7. Instead, lane rates of 100 Gbit/s are considered indispensable to maintain further scalability of throughput in campus-area and data-center networks. In this context, the key challenge is to build transmitters that can generate 100 Gbit/s OOK data streams at lowest possible power consumption, and such transceivers have even been identified as the “Holy Grail” of the Ethernet ecosystem by the Ethernet Alliance7. In fact, while a wide variety of compact high-speed optical modulators has been demonstrated over the last years8,9,10,11,12,13,14,15,16,17,18, only a few10,11,14,18 are at all capable of providing OOK data rates of 100 Gbit/s, and these often feature comparatively high operating voltages. When it comes to high-speed Mach-Zehnder modulators (MZM), the most efficient 100 Gbit/s device demonstrated so far is based on 2.5 mm-long phase shifters and features a π-voltage of 2 V11.

In this paper we show that these limitations can be overcome by silicon-organic hybrid (SOH) modulators19,20,21,22,23,24,25,26,27,28,29,30,31,32,33 that combine the advantages of large-scale silicon photonic integration with the extraordinarily high electro-optic (EO) coefficients obtained by molecular engineering of organic materials34,35. We demonstrate generation of OOK signals up to 100 Gbit/s using a 1.1 mm-long SOH MZM which features a π-voltage of only 0.9 V. The associated switching energy amounts to less than 98 fJ/bit – a record-low value for transmission at 100 Gbit/s OOK using semiconductor-based modulators. In our experiments, we operate the device at a peak-to-peak voltage of 1.4 V, thereby exploiting the nonlinear transfer characteristic of the MZM to mitigate impairments by limited bandwidth of the modulator and of the transceiver circuitry, which leads to an estimated BER down to 6.6 × 10−6. We support our experiments by a theoretical analysis that takes into account the measured transfer function of the modulator and of the driver circuits. Besides signal generation, we transmit a 100 Gbit/s OOK stream over a dispersion-compensated 10 km standard single-mode fiber (SMF) link. This is the first transmission experiment of a 100 Gbit/s OOK signal generated by a semiconductor-based modulator. Unlike previous implementations20,21 and competing device concepts18,36,37,38 fabricated by high-resolution electron beam lithography, our modulators were processed in a commercial silicon photonics line together with the full portfolio of silicon photonic devices and Ge photodiodes using standard 248 nm deep-UV lithography. In contrast to earlier demonstrations of SOH electro-optic modulators20,21,26,32, this work focusses on high-speed serial transmission using simple on-off-keying and direct detection techniques rather than technically demanding quadrature amplitude modulation (QAM), thereby considerably reducing hardware complexity and avoiding energy-intensive signal processing. When combined with highly efficient CMOS drivers, SOH modulators have the potential to open a technically and commercially superior avenue towards short-reach transceivers with unprecedented energy efficiency that will be key for future Ethernet interfaces at Tbit/s data rates.

Materials and Methods

Principle of a silicon-organic hybrid (SOH) electro-optic (EO) phase modulator

SOH modulators combine silicon-on-insulator (SOI) slot waveguides and electro-optic (EO) cladding materials19. A schematic of an SOH Mach-Zehnder modulator (MZM) and its cross-section are depicted in Fig. 1(a) and (b), respectively. The phase shifters consist of a silicon slot waveguide which is formed by two silicon rails19. Due to the discontinuity of the normal electric field component at the interface to the silicon rails, the dominant field component \({\underline{ {\mathcal E} }}_{0,x}\) for the quasi-TE polarization in the slot is strongly enhanced, Fig. 1(b), Inset (1). The slot is filled with an organic EO material which provides a high χ(2)-nonlinearity (Pockels effect). The silicon rails are connected to aluminum (Al) electrodes via thin n-doped silicon slabs and aluminum vias (not depicted). A modulation voltage applied to the Al electrodes drops completely across the narrow slot and leads to a strong electric field Ex,RF which is well confined to the silicon slot region, Fig. 1(b), Inset (2). The strong electric field interacts with the EO organic cladding and leads to a pronounced change of the refractive index, and consequently to a phase modulation of the optical wave. For estimating the phase shift ΔΦ in an SOH waveguide, we may assume that the modulating radio-frequency RF field features only an x-component which has a constant value of Ex,RF = Udrive/wslot in the slot region Aslot, see Fig. 1(b), and which is negligible outside. This leads to the relation19

$${\rm{\Delta }}{\Phi }=\frac{1}{2}{n}_{{\rm{EO}}}^{3}{r}_{33}{E}_{{\rm{x}},{\rm{RF}}}\Gamma {k}_{0}L,$$
(1)

where k0 = 2π/λ is the optical wavenumber at a vacuum wavelength λ, Γ is the field interaction factor, nEO is the refractive index of the organic cladding material in the slot if no voltage is applied, r33 is the EO coefficient and L describes the length of the phase shifter. The field interaction factor Γ can be calculated in terms of the vectorial mode fields \({\underline{ {\mathcal E} }}_{0}(x,y)\) and \({\underline{ {\mathcal H} }}_{0}(x,y)\) of the fundamental waveguide modes19,

$${\Gamma }=\frac{{c{\rm{\varepsilon }}}_{0}{n}_{{\rm{EO}}}\mathop{{\int }^{}\,{\int }^{}}\limits_{{A}_{{\rm{slot}}}}|{\underline{ {\mathcal E} }}_{0,x}(x,y){|}^{2}{\rm{d}}x{\rm{dy}}}{{\iint }^{}{\rm{Re}}\{{\underline{ {\mathcal E} }}_{0}(x,y)\times {{\underline{ {\mathcal H} }}^{\ast }}_{0}(x,y)\}{{\rm{e}}}_{z}{\rm{d}}x{\rm{dy}}}$$
(2)

where c is the vacuum speed of light, and ε0 is the vacuum dielectric constant.

Figure 1
figure 1

Schematic of an SOH Mach-Zehnder modulator (MZM). (a) Top view of an MZM with two SOH phase shifters, a coplanar ground-signal-ground (GSG) transmission line, and a pair of multi-mode interference (MMI) couplers. (b) Cross-sectional view of the phase shifter section of the SOH MZM fabricated on a silicon-on-isolator substrate with a 2 µm thick buried oxide (BOX) layer. The slot waveguide (wSlot = 160 nm, wRail = 240 nm, hSlab = 70 nm) is formed by two silicon rails and is embedded into an organic electro-optic (EO) cladding material. The slot is connected to the aluminum (Al) transmission lines by thin n-doped silicon slabs and aluminum vias (not depicted). A poling voltage Upol applied across the (floating) ground electrodes at an elevated temperature close to the material’s glass transition point aligns the EO chromophores in the slot (green arrows). An electric field generated from a modulation signal Udrive applied to the GSG electrodes (red arrows) is oriented parallel (anti-parallel) with respect to the chromophores orientation in the left (right) slots. This leads to a phase shift of equal magnitude but opposite sign in the two slots, resulting in chirp-free push-pull operation. The electronic bandwidth of an SOH MZM is limited by the inherent RC lowpass characteristic resulting from the limited conductivity of the n-doped silicon slabs and the capacitance of the slot. Inset (1): Dominant x-component of the optical electric field \(\underline{ {\mathcal E} }\)x,opt in the slot waveguide with slot area Aslot. Inset (2): Field component \({E}_{0,x}\) of the electrical RF drive signal. Both the optical and the electrical field are well confined to the slot and overlap strongly for an efficient modulation. Inset (3): Electron accumulation layer. The modulator bandwidth is increased by a decreased resistance (R) of the slabs, induced by a charge accumulation layer that can be generated by a “gate voltage” Ugate between the bulk silicon and the ground electrodes. (c) DC characteristic of a 1.1 mm long SOH MZM with a π-voltage of 0.9 V measured at a voltage offset slightly more than 2 V. Using this offset avoids screening effects of the applied electric field by free charges in the organic cladding19.

The dynamic behavior of an SOH device can be understood by considering a lumped-circuit model as indicated in Fig. 1(b). It consists of a capacitor C representing the SOH slot waveguide, and of two resistors R which describe the finite conductivity of the n-doped silicon slabs. The resulting RC low-pass characteristic as well as the RF propagation loss lead to bandwidth limitations22. The conductivity of the silicon slabs and hence the device bandwidth can be increased by, e.g., applying a voltage between the device layer and the bulk silicon, which leads to an electron accumulation layer and hence to a reduced resistivity of the slabs22,39, see Fig. 1(b), Inset (3). Using this approach, bandwidths in excess of 100 GHz have been demonstrated22. The necessary gate voltage can be diminished by using thin oxide and doped poly-silicon gates deposited on top of the slab regions28.

Note that the SOH approach maintains the full advantages of silicon photonics, exploiting highly mature CMOS processes for fabrication of the slot-waveguide base structures, onto which EO materials are deposited in a highly scalable post-processing step. In particular, SOH devices can be seamlessly integrated into complex photonic integrated circuits (PIC) that exploit the full range of devices available on the silicon photonic platform.

Design, fabrication, and operation of SOH Mach-Zehnder modulators

In this work we use a 1.1 mm long SOH Mach-Zehnder modulator (MZM) formed by two SOH phase shifter sections. The phase shifters comprise 240 nm wide rails and 160 nm wide slots and are covered by the organic EO material SEO10040, which has a refractive index of nEO = 1.73. This leads to a field interaction factor Γ ≈ 0.16. Our experiments build upon a series of technological advances in comparison to earlier publications21,24,26. These advances relate, e.g., to fabrication techniques, to the materials, for which stability has been improved greatly21, and to the underlying poling procedures. In particular, the silicon photonic base structures in this work are fabricated in a 248 nm deep ultra-violet (DUV) optical lithography process at A*Star IME in Singapore – unlike previous generations of SOH modulators, for which electron-beam lithography was used20,21. Fabrication on a standard platform allows co-integration with the full portfolio of silicon photonic devices. In order to comply with the design rules of the foundry, some adaptations of the modulator and the transmission line were required. As an example, the slots had to be defined on a dedicated mask layer to enable better control of the slot width. Regarding electrical wiring, our current chips comprise two metal layers, rather than a single layer as used in previous devices. The additional wiring layer is embedded into a 2 µm-thick layer of oxide (not depicted in Fig. 1(b)). In addition, our current devices rely on a dedicated process to locally remove the top oxide layer in the slot regions, such that the EO material can be deposited onto the pre-fabricated chips in a separate process. The deposition of the EO material is completely independent from the processing in the fab. Note that, besides opening of the top oxide, there is no need to further adapt the fabrication workflow of the silicon photonic base structure. The approach should also be compatible with on-chip integration of driver electronics, and we do not expect fundamental technology-related roadblocks when it comes mass production of SOH base structures in silicon foundries.

The EO material has a high EO coefficient of 166 pm/V as measured in bulk material for a wavelength of 1550 nm41. After spin coating, the macroscopic EO activity of the cladding is activated by poling23 at an elevated temperature close to the material’s glass transition temperature. To this end, a DC poling voltage is applied across the (floating) ground electrodes to align the EO chromophores in the two slots. The direction of alignment is defined by the direction of the electric DC poling field and is the same direction in both slots, indicated by green arrows in Fig. 1(b). The poling voltage remains applied while cooling the device to room temperature in order to freeze the chromophores in their state of orientation. Applying a modulation voltage to the signal electrode after poling leads to modulating fields oriented in opposite directions with respect to the chromophore alignment in the two slots. The modulating field is indicated by red arrows in Fig. 1(b). This leads to phase shifts of equal magnitudes but opposite signs in the two slots. This results in an efficient push-pull operation19 and leads to chirp-free amplitude modulation provided that the device is perfectly balanced; see Supplementary Information for a more detailed discussion of chirp properties and of the impact of imbalance.

In general, SOH EO modulators stand out due to their high modulation efficiency, which can be expressed by the π-voltage-length product UπL, where Uπ is the voltage required to achieve a phase difference of π in the two arms of the MZM, and where L denotes the phase shifter length. SOH MZM have been demonstrated with UπL products down to 0.5 Vmm23,24 – more than an order of magnitude below that of conventional pn-depletion type devices42,43. Using SOH modulators, we have demonstrated optical signal generation with drive voltages down to 80 mVpp and energy consumptions of the order of 1 fJ/bit using OOK modulation24. In contrast to plasmonic-organic hybrid (POH) electro-optic modulators36,37,38, which adapt the concept to plasmonic waveguides, SOH devices stand out due to significantly lower propagation losses, which enable larger lengths of phase shifters, and hence lower drive voltages19. As a quantitative measure, the product of the π-voltage Uπ and the achievable insertion loss aL can be used, where a denotes the propagation loss in the phase shifter in dB/mm and where L is the phase shifter length. For POH modulators, this figure is usually above 10 dBV, whereas values of 1 dBV can be achieved by SOH devices19. The capabilities of the SOH platform can further be extended to highly efficient phase shifters based on liquid crystals27, or to hybrid lasers that exploit light-emitting cladding materials44.

While the present work concentrates on SOH MZM for high-speed OOK, the SOH modulator concept has also been proven to be perfectly suited for generation of advanced modulation formats such as 4-state pulse-amplitude modulation (4PAM, 120 Gbit/s)30, 8-state amplitude shift keying31 (8ASK, 84 Gbit/s), quadrature phase shift keying (QPSK), or 16-state quadrature amplitude modulation20,25,26,32 (16QAM). For 16QAM signaling, we have recently demonstrated line rates of up to 400 Gbit/s20,32. At the same time, the efficiency of SOH modulators is accentuated by the ability for operation without external drive amplifiers, even for generation of higher-order modulation formats25,26, where an electrical energy consumption of down to 18 fJ/bit has been demonstrated for 16QAM signaling. While these modulation formats lead to larger spectral efficiency and consequently to higher data rates, they considerably increase the complexity of transmitter and receiver and are hence not well suited for short-reach transmission in data centers or campus-area networks. This is particularly true for coherent communications where the receiver requires a dedicated photonic integrated circuit with two balanced detectors per polarization, a local oscillator laser, and extended DSP rather than just a simple photodiode.

The MZM used in our experiment features a π-voltage of 0.9 V at a wavelength of 1550 nm, see Fig. 1(c), which, for a device phase shifter length of 1.1 mm, corresponds to a UπL-product of 1 Vmm. Note that the π-voltage was measured at DC bias voltages above 2 V. For smaller bias voltages, we observe slightly increased spacings of the transmission dips and hence slightly increased π-voltages, which is attributed to free ions in the cladding that lead to a partial screening of the applied fields at small bias voltages19. However, this effect is only observable for low frequencies and does not impede RF operation23.

The slight increase of UπL in comparison to the value reported in references23,24 is caused by a reduced r33-coefficient of the presently used EO material, which was selected for high thermal stability rather than for highest EO activity. The EO coefficient r33 can be estimated from the measured UπL-product of the MZM operated in push-pull, the calculated field interaction factor Γ and from the slot width wslot,

$${U}_{\pi }L=\frac{{w}_{{\rm{s}}{\rm{l}}{\rm{o}}{\rm{t}}}\lambda }{2{n}_{{\rm{E}}{\rm{O}}}^{3}{r}_{33}{\rm{\Gamma }}},{r}_{33}=\frac{{w}_{{\rm{s}}{\rm{l}}{\rm{o}}{\rm{t}}}\lambda }{2{U}_{\pi }L{n}_{{\rm{E}}{\rm{O}}}^{3}{\rm{\Gamma }}}.$$
(3)

In this relation, λ is the carrier wavelength, and nEO is the refractive index of the organic cladding material19. The factor of 2 in the denominator results from the push-pull operation. For our device, we find an r33 coefficient of 147 pm/V, which compares well to values of 166 pm/V reported for bulk SEO100, see reference41. Note that SEO100 was chosen due to its temperature stability40. Using specially optimized material systems, we have previously demonstrated even higher EO coefficients in excess of 230 pm/V24,33, but these materials did not yet feature thermal stability for extended operation at 85 °C. The modulator structure as well as the organic material are well suited to operate over a large range of infrared telecommunication wavelengths comprising all relevant transmission bands between 1260 nm and 1675 nm, see Supplementary Information for details.

For the special SOH devices used in our experiments, rather high optical losses were observed with fiber-to-fiber attenuations of 20 dB or more. These high losses were caused by a fabrication problem, which led to contamination of the slot waveguides with Germanium residuals  – this problem was fixed in newer device generations by adapting the process flow. In the presented experiments, the losses of the devices comprise approximately 4.5 dB of fiber-chip coupling loss for each of the grating coupler interfaces (9 dB in total), around 1 dB of excess loss for a pair of strip-to-slot converters, approximately 1 dB of excess loss for a pair of multi-mode interference couplers, and an additional approximately 1 dB for on-chip waveguides. This leaves approximately 8 dB for the 1.1 mm-long slot-waveguide section, corresponding to rather high propagation losses of 7.3 dB/mm for this specific device generation. These losses lead to aUπL products of 8 dBV, which is clearly above the 2.8 dBV that were previously demonstrated for SOH devices24, but still well below the approximately 25 dBV found for POH modulators45.

Another important performance parameter of MZM is the static extinction ratio δ(stat), which is defined by the squared sum of the superimposed optical field strengths of both arms at the output of the MZM, related to the squared difference of the field strengths,

$${\delta }^{(stat)}=\frac{{({E}_{1}+{E}_{2})}^{2}}{{({E}_{1}-{E}_{2})}^{2}}.$$
(4)

If the splitting and combining ratios are not exactly 50/50 or if the loss in one arm is different from the loss in the other arm, then the amplitudes of the superimposed fields are different, and the extinction ratio (ER) is finite. This may lead to a chirped output signal, even if the modulator is operated in push-pull mode, see Section “Results and Discussion” and Supplementary Information for details. The (static) ER can be determined by measuring the transmission of the MZM as a function of the applied DC voltage, see Fig. 1(c). For the device used in the transmission experiments, the ER is rather low and amounts to approximately 14 dB. We attribute this to deviations of the MMI coupler from the ideal splitting ratio and to unequal propagation losses in the two arms of the MZM caused by the Germanium contaminations of the slot waveguides. Note that, due to the specific chip design, ports 2 and 4 of the MZM were inaccessible, see Fig. 1(a). Using ports 1 and 4 or ports 2 and 3 instead would eliminate the problem of non-ideal MMI couplers. In general, SOH devices can provide ER which are much better than the 14 dB obtained here – for other devices with similar device layouts we typically measure ER of δ(stat) = (20 … 32) dB, see Supplementary Information and reference23. Note that the “dynamic” extinction ratio δ(dyn) of the data signal is not only dictated by the static extinction ratio δ(stat) of the modulator itself, but also by other effects such as inter-symbol interference, see Section “Generation and transmission of 100 Gbit/s OOK” below.

Results and Discussion

Setup for signal generation

The experimental setup for data signal generation is depicted in Fig. 2(a). An external cavity laser (ECL) provides the optical carrier at a wavelength of approximately 1550 nm. The light is coupled to and from the SOH MZM via grating couplers. While these couplers are perfectly suited for testing, they introduce limitations of the operating wavelength range. In advanced device implementations, these grating couplers might be replaced by edge coupling, e.g., based on free-space assemblies of micro-lenses and prisms46, or with 3D free-form waveguides or lenses printed by two-photon polymerization47,48,49,50,51. After modulation, the optical signal is fed into an erbium-doped fiber amplifier (EDFA) with a gain of 35 dB, an optional 10 km long fiber, and a 2 nm wide optical band-pass filter to remove out-of-band noise, before being detected by a 100 Gbit/s photodiode. At the transmitter, an arbitrary waveform generator (AWG, Keysight M8195A) is used to synthesize the electrical drive signals, using two independent pseudo-random binary sequences (PRBS) of length 29-1. These signals enter a 2:1 electrical multiplexer (MUX, SHF 603A), the output of which is a non-return-to-zero (NRZ) signal with a peak-to-peak voltage swing of 0.4 Vpp and double the symbol rate of the inputs. A radio-frequency (RF) amplifier (SHF 827) with a nominal bandwidth of 70 GHz is used to boost the signal at the MUX output to a peak-to-peak voltage of 1.4 Vpp. This signal is then coupled to the ground-signal-ground (GSG) transmission line of the MZM via microwave probes having a nominal bandwidth of 67 GHz. A DC bias voltage is applied via the same microwave probe to set the operating point of the MZM to the quadrature (3 dB) point. An external 50 Ω termination resistor connected to the end of the transmission line via a second microwave probe prevents back-reflections. Because de-multiplexers operating at 100 Gbit/s are commercially not yet available, we could not analyze the data stream in real-time, and it was hence impossible to measure the bit error ratio (BER) directly. Instead, the received electrical signal is analyzed using an Agilent 86100C digital communications analyzer (DCA) with a 70 GHz equivalent-time sampling module (Agilent 86118A). We record the electrical eye diagrams and extract the quality factor (Q-factor) which is defined by the signal’s mean levels u1 and u0 for the logical ‘1’ and the logical ‘0’, and by the corresponding standard deviations σ1 and σ0,

$$Q=\frac{{u}_{1}-{u}_{0}}{{\sigma }_{1}+{\sigma }_{0}}.$$
(5)

The BER of the data signal can be estimated from the measured Q-factor52

$${{\rm{BER}}}_{{\rm{e}}}=\frac{1}{2}{\rm{erfc}}(\frac{Q}{\sqrt{2}})$$
(6)

The complementary error function is defined by \({\rm{erfc}}(z)=(2/\sqrt{\pi }){\int }_{z}^{\infty }\exp (-{t}^{2}){\rm{d}}t\).

Figure 2
figure 2

Experimental setup and measured eye diagrams. (a) Setup for 100 Gbit/s OOK data generation. An external cavity laser (ECL) provides the optical carrier. Optical power is coupled to and off the 1.1 mm long SOH MZM chip via grating couplers (GC). An erbium-doped fiber amplifier (EDFA) with a 2 nm optical bandpass filter (BPF) compensates chip losses. An optional dispersion-compensated 10 km fiber link is used for transmission experiments. A 100 Gbit/s photodiode detects the signal and feeds it to a 70 GHz equivalent-time sampling module of a digital communications analyzer (DCA). The electrical drive signal is derived from two independent pseudo-random binary sequences (PRBS) generated in an arbitrary waveform generator (AWG, Keysight M8195A). These sequences are fed to a multiplexer (MUX, SHF 603 A), combined to a single binary NRZ sequence (≤100 Gbit/s), amplified with a radio-frequency (RF) amplifier, and coupled to the chip using microwave probes. A bias-T adds a DC voltage Ubias to set the MZM to the quadrature (3 dB) operating point. The ground-signal-ground (GSG) transmission line is terminated with a 50 Ω resistor. (b) Eye diagrams of MUX output (voltage swing 400 mVpp) for data rates 60 Gbit/s, 70 Gbit/s, 80 Gbit/s, and 100 Gbit/s. (c) Eye diagrams of RF amplifier output (voltage swing 1.4 Vpp). The amplifier transfer function causes signal distortions. (d) Eye diagrams, measured Q-factor and estimated BERe after detection (back-to-back, b2b) and (e) after transmission over the dispersion-compensated 10 km long link. In the b2b measurement, a gate field was applied for the 100 Gbit/s signal only. For the transmission, a gate field was applied for both the 80 Gbit/s and 100 Gbit/s signal.

Generation and transmission of 100 Gbit/s OOK

The NRZ eye diagrams of the OOK drive signals for different data rates are depicted in Fig. 2(b),(c). The clearly open eyes of the MUX output are shown in the first column, Fig. 2(b), while the eye diagrams of the RF drive amplifier output are depicted in the second column, Fig. 2(c). Up to data rates of 60 Gbit/s, the eyes are well open, while at 80 Gbit/s the signal starts deteriorating. This is due to the bandwidth limitations of the amplifier, which predominantly affect its phase response and lead to significant group delay dispersion, see Section “Theoretical analysis of bandwidth limitations” for details.

In a back-to-back measurement without the 10 km long transmission fiber, we record the eye diagrams of the optical signals after direct detection of data signals from 60 Gbit/s to 100 Gbit/s, Fig. 2(d). For data rates of 60 Gbit/s and 70 Gbit/s, we measure open eyes and Q-factors of Q = 5.7 and 4.8, respectively. Following Eq. (6), we estimate BERe of 6.7 × 10−9 and 7.9 × 10−7. At 80 Gbit/s and 100 Gbit/s, the measured Q-factors of 4.2 and 3.4 correspond to an estimated BERe of 1.3 × 10−5 and 3.2 × 10−4, respectively. All of these BERe values are below the threshold of 4.5 × 10−3 for hard-decision forward error correction (FEC) with 7% overhead53. A gate field was applied for the 100 Gbit/s signal only. The 100 Gbit/s achieved in our experiment corresponds to the highest OOK data rate generated by a silicon-based modulator so far, see Section “Competitive benchmarking and application potential” for a more detailed comparison to other experiments. Note that in our as well as in competing high-speed OOK demonstrations10,11,18, the data rate of 100 Gbit/s does not refer to the net data rate, but to the line rate and hence includes the 7% FEC overhead.

The rather low static extinction ratio (ER) of approximately 14 dB of our MZM leads to a residual chirp of the generated data signal, which would not occur for perfectly balanced devices. For quantifying the chirp of the data signal, we use the chirp parameter α that is essentially defined by the ratio of the phase modulation to the amplitude modulation54,55,

$$\alpha =2P\frac{{\rm{d}}\varphi /{\rm{d}}t}{{\rm{d}}P/{\rm{d}}t}$$
(7)

In this relation, ϕ denotes the phase and P the time-dependent power of the optical signal averaged over a few optical cycles. In SOH devices, imbalance of the MZM arms is the dominant source of chirp, see Supplementary Information for a more detailed discussion and an experimental verification. The magnitude of the chirp parameter α can thus be directly related to the ratio γ = E2/E1 of the fields in the two MZM arms54.

$$|\alpha |=\frac{1}{{\rm{\gamma }}}\frac{{\phi }_{1}+{\gamma }^{2}{\phi }_{2}}{{\phi }_{1}-{\phi }_{2}}.$$
(8)

In this relation, ϕ1 and ϕ2 denote the phases shifts in the individual MZM – for push-pull modulation we can assume ϕ2 = −ϕ1. The field amplitude ratio γ can be derived from a measurement of the (static) extinction ratio δ(stat) defined in Eq. (4),

$$\gamma =\frac{\sqrt{{\delta }^{(stat)}}-1}{\sqrt{{\delta }^{(stat)}}+1.}$$
(9)

Note that the electric fields are chosen such that E1 > E2 and hence 0 ≤ γ ≤ 1. As a consequence, Eq. (8) only allows determining the magnitude of α, but not its sign – this would require knowing whether the stronger optical amplitude is associated with the MZM arm having a positive or a negative phase shift, which cannot be derived from a measurement of the static extinction ratio. Using Eqs (8) and (9), the static extinction ratio of 14 dB of our device translates into a magnitude of the chirp parameter of |α| ≈ 0.42, which is well below chirp parameters of |α| = 0.8 that are obtained for conventional pn-depletion type silicon modulators with comparable ER56.

We also measure the dynamic extinction ratios of our data signals. For 100 Gbit/s signaling, the measured dynamic ER amounts to 5 … 7 dB, which compares well to a measured extinction ratio of 6.1 dB that was observed for a conventional pn-depletion type silicon modulator15 at 70 Gbit/s. Note that the dynamic extinction ratio measured from the eye diagram of a data signal is generally worse than the static extinction ratio of the underlying modulator according to Eq. (4). This is due to inter-symbol interference and quadratically detected optical noise.

In addition to the back-to-back experiment, we transmit the data signals over a dispersion-compensated fiber link of 10 km standard single-mode fiber (SMF) having a negligible residual dispersion of 2.6 ps/nm. The eye diagrams of the data signals received after transmission are depicted in Fig. 2(e). For the 60 Gbit/s and 70 Gbit/s data, the Q-factors of 5.6 and 4.4 did not significantly deteriorate compared to the Q-factors of 5.7 and 4.8 in the back-to-back measurements. These Q-factors correspond to BERe = 7.9 × 10−7 and BERe = 4.9 × 10−6, respectively. For data rates of 80 Gbit/s and 100 Gbit/s, a gate field was applied and the measured Q-factors of 4.2 and 2.8 correspond to BERe values of 1.5 × 10−5 and 3.0 × 10−3. This experiment corresponds to the first 100 Gbit/s OOK transmission demonstration using a modulator on the silicon photonic platform. The transmission demonstration over the dispersion-compensated 10 km fiber link was performed with binary drive signals without further signal processing. Still, the results compare very well to recently published demonstrations of 100 Gbit/s OOK transmission over an uncompensated 1.8 km-link using InP based devices in combination with digital equalization at the receiver11.

Theoretical analysis of bandwidth limitations

To analyze the impact of bandwidth limitations on our experiments, we reproduce the results by simulations, see Fig. 3. To this end, we use a vector network analyzer (VNA) to measure the frequency response of a 1.1 mm long SOH MZM with a gate field of 0.1 V/nm, as used for the 100 Gbit/s transmission experiment. The VNA generates an input signal with varying frequency, which is coupled to the (terminated) modulator. The modulated optical power is received with a photodiode featuring a calibrated frequency response, which feeds its output back to the VNA for a characterization of the electro-optic-electric (EOE) bandwidth. The measured frequency response (by modulus and phase) is depicted in Fig. 3(c). The 6 dB point57 of the EOE frequency response is found to be about 25 GHz.

Figure 3
figure 3

Analysis of bandwidth limitations. (a) Simulated eye diagrams. Amplifier input: Cosine-shaped pulses with full-width-half-maximum (FWHM) duration equal to the symbol period. The amplifier is modeled by its measured frequency response, see (b). The modulator is represented by its measured small-signal transfer function, see (c), followed by a cosine-shaped intensity transfer characteristic as sketched in (d). Color map differs from Fig. 2. (b) Modulus and phase of measured S21 parameters of 70 GHz drive amplifier. (c) Modulus and phase of measured small-signal electro-optic frequency response of a 1.1 mm long SOH MZM. Note that the bandwidth of an EO modulator is usually specified by the modulation frequency which corresponds to a 6 dB drop of EOE response10,57. For the spectral component associated with the modulation frequency, this corresponds to a drop of the optical power and hence of the photocurrent amplitude by factor of two, which is measured as a four-fold (6 dB) decrease of the spectral power density by the VNA. For our device, the 6 dB bandwidth amounts 25 GHz. Organic cladding: SEO100. Gate field: 0.1 V/nm. (d) Intensity transfer function T of a MZM vs. normalized drive voltage U/U π .

At first sight, a 6 dB EOE bandwidth of 25 GHz seems rather small for generating a 100 Gbit/s NRZ signal. In general, considering a low-pass filter at the receiver, an optimum signal-to-noise power ratio is found for a 3 dB bandwidth of approximately 65% of the symbol rate58. This bandwidth leads to an ideal trade-off of noise power in the filter passband and inter-symbol interference (ISI) caused by the limited filter bandwidth. In our case, however, the situation is different: The bandwidth limitation is caused by a low-pass characteristic associated with the electrical part of the modulator, which is then followed by the nonlinear, cosine-shaped MZM intensity transmission characteristic, see Fig. 3(d). As a consequence, while low amplitudes of the drive signal translate linearly to optical output power, higher amplitudes are compressed, thereby mitigating ISI-related amplitude fluctuations of the drive signal. To illustrate this effect, we analyze our transmission system in MATLAB. To emulate the limited rise and fall times of the hardware in the simulation, we use cosine-shaped pulses in the time-domain (not to be confused with raised-cosine pulse shaping with a raised-cosine shaped spectrum) to approximate the measured output signal of the MUX, see Fig. 2(b). Details can be found in the Supplementary Information. In the simulation, this signal is then fed to the drive amplifier, which has a gain of 11 dB and which is modeled by the measured S21-parameter, Fig. 3(b). At the output of the amplifier, the drive signal features a peak-to-peak voltage swing of 1.4 Vpp, which is used as an input signal to the modulator. The modulator is modeled by the measured frequency response depicted in Fig. 3(c), followed by the cosine-shape time-domain power transfer function, for which we assume a π-voltage of 0.9 V. The frequency response was set to nearly zero (−200 dB) beyond the measured frequency range. The results of the simulation are depicted in the lower part of Fig. 3(a). Interestingly, the electrical eye diagrams at the amplifier output show already significant distortions, see left column of eye diagrams in Fig. 3(a), even though the magnitude of the frequency response of the device remains flat up to more than 70 GHz. It turns out that these distortions are not caused by the low-pass characteristic of the amplifier, but by its phase response, which starts dropping by approximately −200° between 40 GHz and 75 GHz, see Fig. 3(b). This can be confirmed by assuming a flat phase characteristic in the simulation, for which the distortions disappear. The low-pass modulator frequency response leads to further closure of the eye due to ISI, see center column of eye diagrams in Fig. 3(a), and it is only the compression of large amplitudes in the MZM that reproduces an open eye, see right column of eye diagrams in Fig. 3(a). Using this property allows the generation of high-speed NRZ signals with data rates well beyond the modulator’s small-signal 6 dB bandwidth. Note that, in contrast to other 100 Gbit/s OOK demonstrations11,18 or high symbol-rate coherent modulation experiments32, our demonstration does not require any digital pre-distortion or post-equalization and can rely on simple binary drive signals for the modulator at the transmitter and on a simple sampling oscilloscope for measuring the eye diagram at the receiver.

The compression of large amplitudes by the cosine-shaped transfer function is a general property of all MZM. The effect, however, can only be exploited if the available peak-to-peak drive voltage reaches the π-voltage of the device. It is a unique feature of our SOH MZM that this amplitude compression can be achieved at comparatively low drive voltages, which can be realistically generated by currently available driver circuits. The low operating voltage becomes particularly crucial at high data rates, where drive signals with high modulation amplitude are particularly difficult to generate. As an example, conventional pn-depletion-type modulators require peak-to-peak drive voltage swings in excess of 5 V to reach compression of the power transfer function, which would be hard to achieve with currently available electrical drivers for 100 Gbit/s, in particular when lower power consumption shall be maintained.

In our experiments, the length of the PRBS was limited to 29 − 1 due to the memory size and the memory granularity of the AWG, but does not represent a fundamental limit of the device. Using a longer PRBS sequence would lead to elongated sequences of subsequent logical “0” or “1” and hence to more low-frequency components in the signal spectrum. This should not affect the results – the lower cut-off frequency of our transmitter amounts to only 70 kHz, dictated by the AC-coupled drive amplifier. To confirm this expectation, we simulated PRBS sequences of lengths 29 − 1 and 218 − 1 – the maximum possible length that could be handled by our computer. We do not find any relevant change of the received eye diagram.

Signal generation using a 100 GSa/s digital-to-analog converter (DAC) and a real-time oscilloscope

In our previous experiments we were unable to measure the BER directly, since the eye diagram at the receiver was taken with equivalent-time sampling technique. For a more direct analysis of the BER, we improved our setup as follows: AWG and MUX were replaced by a programmable DAC with a sampling rate of 100 GSa/s (Micram DAC4) and analog bandwidth above 40 GHz, and the equivalent-time sampling oscilloscope was substituted by a real-time oscilloscope having a bandwidth of 63 GHz. For detection, we use a photodiode with a bandwidth of 70 GHz, similar to the one of our previous experiment. We record the time traces of the photodiode current and analyze it offline with MATLAB. We operate the MZM without a gate field. For a 100 Gbit/s OOK signal we measure a Q-factor of 2.4 and estimate a BERe = 8.2 × 10−3, Fig. 4(b). The Q-factor in the previous experiment was larger and the estimated BERe was smaller because the MUX acted as a limiter, and because the gate field increased the MZM bandwidth. When taking the directly measured BER from the DAC-based experiment, however, we find a value of only BERm = 4.2 × 10−3, which is smaller than the BERe estimated from the measured Q-factor and falls just within the limits of hard-decision (HD) FEC with 7% overhead. This illustrates the issues involved in estimating a BER from the Q-factor using Eq. (6).

Figure 4
figure 4

Experimental b2b setup and measured eye diagrams for a 100 Gbit/s OOK. (a) A programmable digital-to-analog converter (DAC, 100 GSa/s) serves as an AWG and drives the MZM (no gate field). The receiver Rx comprises a BPF, a photodiode, and a 63 GHz real-time oscilloscope. (b) Received eye diagram, measured Q-factor, estimated BERe, and measured BERm at 100 Gbit/s without post-equalization and (c) with post-equalization. Color map differs from Fig. 2.

Note that FEC is presently not used for short-reach optical interconnects because of the computational latency. However, the OpenOptics multi-source agreement (MSA)59 already describes the use of optimized, low-latency FEC codes that allow to trade coding gain for latency60 and therefore exhibit more stringent BER thresholds. With a post-equalization filter, we measure a BERm of 6.6 × 10−6, see Fig. 4(c), which is within the limits of low-latency FEC. On-chip equalizers are commonly used in state-of-the-art transmitter drive chips61.

Energy considerations

In data center networks, power dissipation is a severe aspect, and the driver electronics of EO modulators play an important role in the overall energy consumption of the transceiver. The design and therefore the power dissipation of the driver depends strongly on the specifications of the modulator. In the following, we analyze the modulator’s energy consumption per bit, which we regard as a figure of merit for the overall power dissipation of the transceiver. To this end, we assume that the GSG transmission line impedance is matched to the 50 Ω drive circuitry and to the terminating resistor R L  = 50 Ω, see Fig. 2(a). The modulator is driven with rectangular non-return-to-zero (NRZ) pulse sequences, for which logical “1” and “0” are equiprobable. The energy consumption per bit can then be calculated24 by dividing the electrical power associated with the drive voltage amplitude by the line rate r,

$${W}_{{\rm{bit}}}={(\frac{{U}_{{\rm{drive}}}}{2})}^{2}\frac{1}{{R}_{{\rm{L}}}r}.$$
(10)

For R L  = 50 Ω, a peak-to-peak voltage swing of Udrive = 1.4 V, and a line rate of 100 Gbit/s, we find an energy consumption of 98 fJ/bit. This is, to the best of our knowledge, the smallest power consumption ever reported for a semiconductor-based MZM at 100 Gbit/s OOK. Note that the biasing and the gate voltage do not involve any measureable DC current flow and hence do not contribute to the energy consumption.

Competitive benchmarking and application potential

The experiments presented in the previous sections demonstrate the unprecedented performance of SOH EO modulators to realize high-speed energy efficient OOK transceivers for data-center and campus area networks. A more detailed comparison to competing concepts of semiconductor-based devices is given in Fig. 5(a). The graph shows the required peak-to-peak drive voltages as a measure of the energy consumption in dependence of experimentally demonstrated OOK line rates. Energy-efficient and fast modulators are found in the lower right corner of the diagram. With our SOH MZM, we generate line rates of up to 100 Gbit/s at drive voltages as low as 1.4 Vpp (), corresponding to a switching energy of 98 fJ/bit. This marks the highest OOK line rate reported so far at the lowest drive voltage. A previous OOK data transmission24 experiment at 40 Gbit/s with a drive voltage of only 950 mV is also given as a reference.

Figure 5
figure 5

Comparison of OOK modulators fabricated on various material platforms. (a) Comparison of drive voltages and OOK line rates for different modulators types. Silicon germanium (SiGe) electro-absorption modulators (EAM), 28 Gbit/s @ 2.8 Vpp, 50 Gbit/s @ 2 Vpp, and 100 Gbit/s @ 2 Vpp12,13,14. Indium phosphide (InP) EAM, 80 Gbit/s @ 3 Vpp8. InP MZM, 60 Gbit/s @ 1.5 Vpp100 Gbit/s @ 2.3 Vpp9,10 and @ 1.5 Vpp11. All-silicon Mach-Zehnder modulators (Si MZM) 70 Gbit/s @ 5.3 Vpp, 80 Gbit/s @ 5 Vpp, and 90 Gbit/s @ 7 Vpp15,16,17. Plasmonic-organic hybrid (POH) MZM, 72 Gbit/s @ 6 Vpp38 and 100 Gbit/s @ 4 Vpp18. Present work: Silicon-organic hybrid (SOH) MZM, 100 Gbit/s @ 1.4 Vpp, corresponding to a switching energy of 98 fJ/bit. This corresponds to the by far lowest value demonstrated to date. Another experiment with SOH modulators24 was performed with drive voltages of 950 mV at a line rate of 40 Gbit/s. (b) Comparison of modulators in terms of OOK line rate and π-voltage. The SOH MZM for 40 Gbit/s and 100 Gbit/s exhibit π-voltages of 0.5 V24 and 0.9 V, respectively. These values are clearly below those achieved by other material platforms: InP MZM with π-voltages of 1.7 V and 2 V were operated at 60 Gbit/s8 and 100 Gbit/s9,10, respectively. For the 100 Gbit/s POH MZM18, we estimate a Uπ of 3 V. In the plot, EAM are not depicted since the π-voltage is not defined for these devices. For the Si MZM, the π-voltage is either not given or π-voltage of more than 20 V are estimated15, which are outside the plotted parameter range. Similarly, the π-voltage of approximately 10 V in the 72 Gbit/s POH experiment38 cannot be depicted.

The fastest and most energy-efficient competing devices are based on InP, where both electro-absorption modulators (EAM) and MZM have been shown. InP EAM enable line rates up to 80 Gbit/s at peak-to-peak drive voltages of 3 Vpp8. With an InP MZM, 60 Gbit/s OOK signaling was demonstrated at a comparatively low drive voltage of 1.5 V9. More recently 100 Gbit/s at drive voltages of 2.3 Vpp were shown10. This is clearly higher than the 1.4 Vpp demonstrated for our devices, and the associated switching energy of more than 250 fJ/bit is more than twice the value reported for our device. Further, 100 Gbit/s OOK was demonstrated11 with an InP MZM at a peak-to-peak drive voltage of 1.5 Vpp. This performance is on par with the results obtained by our experiment, however the device features a π-voltage of 2 V which is twice as high as the 0.9 V obtained for the SOH MZM. This allowed to drive the modulator in the linear regime for multi-level PAM signaling but sacrificed modulation depth. Moreover, SOH devices exploit the intrinsic scalability advantages associated with large-scale silicon photonic fabrication based on highly developed CMOS processes, potentially in combination with electrical circuits62,63. Regarding the silicon photonic platform, silicon-germanium (SiGe) EAM were realized and demonstrated at line rates of up to 50 Gbit/s, using drive voltages of at least 2 Vpp12,13. More recently, a 100 Gbit/s OOK signal was generated using a SiGe EAM14 at a drive voltage 2 Vpp. With all-silicon MZM (Si MZM), line rates up to 70 Gbit/s15, 80 Gbit/s16, and 90 Gbit/s17 were demonstrated, but at the expense of large drive voltages of 5 Vpp and beyond. Another interesting approach published recently relies on a silicon-based plasmonic-organic hybrid (POH) MZM, for which a line rate of 72 Gbit/s and 100 Gbit/s have been published18. It shall be noted that the 72 Gbit/s signal was detected by a coherent receiver and hence signal quality aspects cannot be directly compared to the other direct detection experiments. In general, the performance of these devices is fundamentally limited by an intrinsic trade-off between energy consumption and insertion loss19, leading to relatively large drive voltages of 6 Vpp38 and 4 Vpp18, respectively. In addition, fabrication of POH devices has so far relied on advanced electron-beam lithography, which is not readily amenable to large-scale low-cost production. Figure 5(b) takes the same MZM references but plots the π-voltages instead of the applied drive voltage. The plot nicely exhibits the extraordinary low π-voltages of less than 1 V as the unique feature of SOH modulators. For the InP MZM, the π-voltages amount to 1.7 V and 2 V for the devices demonstrating 60 Gbit/s and 100 Gbit/s, respectively. The π-voltage of the POH MZM is not specified in the paper, but estimated from the device length and from the UπL product that is referenced for POH modulators using the same EO material. Note that the EAM listed in Fig. 5(a) are not included in the comparison in Fig. 5(b), because the π-voltage is not defined for EAM. Moreover, Fig. 5(b) does not contain all MZM from Fig. 5(a), since some of the specified or estimated π-voltages would exceed the scale. As an example, the 70 Gbit/s Si MZM15 and the 72 Gbit/s POH MZM38 feature π-voltages of 20 V and around 10 V, respectively, which would be outside the depicted range. For VCSEL-based links, the highest OOK data rate demonstrated so far amounts to 70 Gbit/s5,64, but transmission distances are usually less than 100 m.

SOH devices can hence compare very well to competing device concepts, both in terms of performance and in terms of device scalability. The record-low drive voltage of 1.4 Vpp can be further reduced by using optimized poling techniques65 or advanced organic materials, for which EO coefficients in excess of 350 pm/V have been demonstrated33. This might pave the path towards SOH MZM with sub-500 mV drive voltages that can be directly operated25 by energy-efficient CMOS circuits without additional SiGe BiCMOS amplifier stages. Note that serializer/deserializer (SerDes) chips generating 100 Gbit/s NRZ drive signals have recently been realized on the BiCMOS platform61. SOH modulators are perfectly suited to complement these circuits on the optical side and to enable short-reach, high-speed transceivers with unprecedented energy efficiency that will be key for future Ethernet interfaces at data rates of 400 Gbit/s, 800 Gbit/s, or 1.6 Tbit/s. In the future, such devices might be co-integrated with light sources in compact chip-scale assemblies. This can be accomplished by hybrid integration approaches that rely, e.g., on flip-chip integration of direct-bandgap III-V dies on processed silicon photonic waveguides66, on mounting of readily processed III-V lasers onto silicon photonic dies67, or on photonic multi-chip integration concepts that exploit the concept of photonic wire bonding47,49,50.

Another important aspect of the SOH concept is the stability of the organic EO materials. Recent advances in material synthesis and molecular design have led to efficient and thermally stable organic EO materials. Meanwhile, tests have shown that organic EO materials40 such as SEO100 or side-chain polymers68 maintain more than 90% of their EO activity when stored at an elevated temperature of 85 °C for 500 hours. We have previously shown that SOH modulators with SEO100 are suited for operation at elevated temperatures of 80 °C under ambient atmospheric conditions21. More recently, polymer modulators withstanding temperatures of 105 °C for 2000 hours have been demonstrated69. We expect that even higher operating temperatures can be achieved in the future, e.g., by cross-linking techniques70, or by using materials with intrinsically higher glass transition temperatures such as side-chain EO polymers68. In addition to temperature, photo-oxidation might play an important role in the degradation of EO organic materials – this aspect is subject to ongoing research, and we expect that the associated life-time limitations can also be overcome by cross-linking, which reduces oxygen diffusion into the material71,72, or by encapsulation of the devices.

Conclusion

Using a silicon-organic hybrid (SOH) MZM we demonstrate for the first time the generation and transmission of a 100 Gbit/s OOK signal at record-low drive voltages of only 1.4 Vpp and energy consumptions of only 98 fJ/bit. We confirm our experimental results by simulations using the measured frequency characteristic of our SOH modulator and its associated drive circuitry. The moderate EOE modulator bandwidth of 25 GHz leads to an eye opening, which is much improved by the nonlinear modulator transfer characteristic. In the experiments, we achieve BER below the threshold for hard-decision forward error correction. Post-equalization helps in improving the eye opening so that low-power and low-latency FEC codes can be employed. The efficiency of our modulator and the possibility to exploit large-scale silicon photonic integration allows the realization of compact and technically simple high-speed transceivers that meet the stringent cost targets of medium-reach interconnects.