High-performance silicon-graphene hybrid plasmonic waveguide photodetectors beyond 1.55 μm.

Graphene has attracted much attention for the realization of high-speed photodetection for silicon photonics over a wide wavelength range. However, the reported fast graphene photodetectors mainly operate in the 1.55 μm wavelength band. In this work, we propose and realize high-performance waveguide photodetectors based on bolometric/photoconductive effects by introducing an ultrathin wide silicon-graphene hybrid plasmonic waveguide, which enables efficient light absorption in graphene at 1.55 μm and beyond. When operating at 2 μm, the present photodetector has a responsivity of ~70 mA/W and a setup-limited 3 dB bandwidth of >20 GHz. When operating at 1.55 μm, the present photodetector also works very well with a broad 3 dB bandwidth of >40 GHz (setup-limited) and a high responsivity of ~0.4 A/W even with a low bias voltage of -0.3 V. This work paves the way for achieving high-responsivity and high-speed silicon-graphene waveguide photodetection in the near/mid-infrared ranges, which has applications in optical communications, nonlinear photonics, and on-chip sensing.

Introduction

Currently, it is desirable to extend the wavelength band of silicon photonics[1] beyond 1.55 μm, e.g., 2 μm, for many important applications in optical communications[2,3], nonlinear photonics[4], and on-chip sensing[5-7]. However, the realization of high-performance silicon-based waveguide photodetectors beyond 1.55 μm still faces challenges. For example, the reported GeSn[8] and ion-implanted silicon[9] photodetectors still operate in the limited wavelength band of <2.5 μm, while III−V photodetectors[10] are unsuitable for monolithic integration on silicon. As an alternative, two-dimensional materials[11,12] (e.g., graphene[13,14] and black phosphorus[15]) provide a promising solution because of their broad operation wavelength band and advantage of avoiding material and structure mismatch in the design and fabrication. At present, black-phosphorus photodetectors have limited bandwidths of ~3 GHz[16-18], and their fabrication is not easy. In contrast, large-size graphene sheets are commercially available and can be transferred/patterned easily in the wafer process line[19]. Recently, several fast silicon−graphene waveguide photodetectors at 1.31/1.55 μm have been reported with a high bandwidth of ~100 GHz[20,21]. Among these photodetectors, the metal−graphene−metal (MGM) configuration is widely used, since the high mobility of graphene facilitates high-speed operation. However, MGM graphene photodetectors[19-32] usually have limited responsivities when operating at low bias voltages. For example, in ref. [20], the reported responsivities are <170 mA/W at −0.4 V and <400 mA/W at −0.6 V for mono-layer and bi-layer graphene photodetectors, respectively. In addition, for the 40 GHz graphene-semiconductor heterostructure (GSH) photodetector reported recently[33], the responsivity is also very low (~11 mA/W). More recently, a graphene-insulator-graphene (GIG) photodetector was reported with an improved responsivity of 0.24 A/W and an estimated 3 dB bandwidth of 56 GHz. Unfortunately, the working bias voltage is as high as 10 V[34]. Therefore, high-speed and high-responsivity graphene photodetectors with low bias voltages are still highly desired. Notably, very few results have been reported for the realization of graphene waveguide photodetectors beyond 1.55 μm, even though light absorption in graphene is present in this range. For the reported surface-illuminated mid-IR graphene photodetectors[35-40], the responsivity is low due to the limited light absorption, which is well known. For the mid-IR graphene waveguide photodetectors reported in recent years[41-43], the measured bandwidths are very limited (e.g., several hundreds of kHz or less). To the best of our knowledge, currently, high-speed (e.g., >10 GHz) silicon−graphene waveguide photodetectors have not been reported for the mid-IR range beyond the wavelength band of 1.55 μm.

In this paper, we propose and demonstrate high-speed and high-responsivity silicon−graphene waveguide photodetectors beyond 1.55 μm by utilizing a hybrid plasmonic waveguide with an ultrathin wide silicon ridge. With this novel design, the light absorption in graphene is enhanced while the metal absorption loss is reduced simultaneously, which helps to greatly improve the responsivity. Here, the wide metal cap in the middle and the MGM sandwiched structures are introduced as the signal electrode and the ground electrodes, respectively, so that one can achieve reduced graphene-metal contact resistances (e.g., several tens of ohms) and a large 3 dB bandwidth. A mechanism analysis confirms that the photothermoelectric (PTE) effect dominates the photoresponse under zero bias, while the bolometric (BOL)/photoconductive (PC) effects become dominant when a bias voltage is applied. When operating at 2 μm, the present graphene photodetector has a responsivity of ~70 mA/W and a measured 3 dB bandwidth of >20 GHz (which is setup-limited). Meanwhile, the present photodetectors also work very well at 1.55 μm. The measured responsivity is approximately 0.4 A/W for a bias voltage of −0.3 V and an optical power of 0.16 mW, while the 3 dB bandwidth is over 40 GHz (setup-limited).

Results

Structure and design

Figure 1a, b shows the configuration of the present silicon−graphene hybrid plasmonic waveguide photodetector, which consists of a passive input section based on a silicon-on-insulator (SOI) strip waveguide and an active region based on a silicon−graphene hybrid plasmonic waveguide. These two parts are connected through a mode converter based on a lateral taper structure. As shown in Fig. 1c, the present hybrid plasmonic waveguide has a silicon ridge core region, an ultrathin Al2O3 insulator layer, a graphene sheet, and a metal cap. The metal cap in the middle is used as the signal electrode, while the ground electrodes are placed far away from the silicon ridge to avoid high metal absorption loss. In particular, here, we introduce the MGM sandwiched structure for the ground electrodes in order to achieve reduced graphene-metal contact resistances, which helps achieve a large 3 dB bandwidth[44]. For previous silicon−graphene hybrid plasmonic waveguide photodetectors, the center metal strip exhibits high absorption of light even though the light−graphene interaction can be enhanced[24,27], in which case the undesired metal absorption without any contribution to the photocurrent generation is even higher than the desired graphene absorption. As a result, the responsivity is usually limited[24,27]. This problem can be alleviated partially by reducing the width of the center metal strip (e.g., 70 nm[27]). However, this reduction in width introduces a high graphene-contact resistance, which consequently leads to a reduction in the responsivity and the bandwidth. In this paper, a silicon−graphene hybrid plasmonic waveguide is proposed with a wide silicon ridge, as shown in Fig. 1d. For the present waveguide, the silicon core layer is chosen to be as thin as 100 nm instead of the regular thickness of 220 nm[19,28,29] so that the light absorption in graphene is enhanced due to the weak mode field confinement in the vertical direction[45]. Furthermore, for the hybrid photonic-plasmonic mode[46] supported in the present waveguide, the metal absorption loss is low even when a relatively wide metal strip is chosen to achieve a low metal−graphene-contact resistance. Meanwhile, the center metal strip (the signal electrode) on top of the silicon ridge still helps improve the light absorption in graphene due to the strong localized field. In this way, the present hybrid plasmonic waveguide can simultaneously realize low metal loss and high absorption in graphene. In addition, the silicon ridge height is chosen to be as small as 50 nm, which helps to avoid damage to the graphene sheet during the fabrication processes. As shown in Fig. 1, an Al gate electrode is integrated on top of the silicon slab region; thus, the silicon ridge acts as a global gate electrode. In this way, one can manipulate the graphene chemical potential by applying a gate bias voltage, as proposed in ref. [24] and demonstrated in refs. [29,30].

Fig. 1

Structures of the present silicon−graphene hybrid plasmonic waveguide photodetector.

a Schematic configuration. b Optical microscopy image. c SEM images. d Cross-section of the present silicon−graphene hybrid plasmonic waveguide with the signal electrode in the middle and the ground electrodes on both sides (here, the metal−graphene−metal sandwich structure is utilized). Vb bias voltage, VG gate voltage

Note that the thin-silicon photonic waveguide and the silicon−graphene hybrid plasmonic waveguide are polarization-sensitive. Here, we consider the case of TE polarization; thus, a TE-type grating coupler is used to achieve efficient fiber-to-chip coupling. The input light is coupled to the TE0 mode of the thin-silicon photonic waveguide and then coupled to the quasi-TE0 mode of the silicon−graphene hybrid plasmonic waveguide[46] with a low coupling loss. Figure 2a, b shows the calculation results of evaluating the light absorption induced by the graphene sheet and the metal strip for the quasi-TE0 mode in the present silicon−graphene hybrid plasmonic waveguide as the waveguide dimensions vary. Here, a finite-element method mode-solver tool (COMSOL) is used (see more details in Supplementary Note 1). The graphene absorptance is given by η(L) = ηg(1 − 10−0.1), where L is the propagation distance, α is the mode absorption coefficient in dB/μm, ηg is the ratio of the graphene absorption to the total absorption, i.e., (here, αg and αm are the absorption coefficients of the graphene sheet and the metal strip, respectively). Since only the graphene absorption contributes to the photocurrent, one should maximize the ratio ηg so that the graphene absorption is more dominant than the metal absorption to improve the responsivity. Figure 2a shows the absorption ratio ηg and the results for the absorption coefficients (αg, αm) as the ridge width wsi varies from 0.5 to 4.0 μm. Here, the width and height of the metal strip are chosen as wm = 200 nm and hm = 50 nm, respectively. As shown in Fig. 2a, the graphene absorption ratio ηg increases when choosing a wider ridge. When the ridge width wsi is chosen to be larger than 3 μm, the ratio ηg is higher than 70%. Meanwhile, it is noted that the absorption coefficients (αg, αm) decrease when choosing a wider ridge, which is simply due to more optical confinement in the silicon region and weaker light−matter interaction in the absorption regions. As a result, one needs to choose a longer absorption length to achieve sufficient absorption in the photodetector, which prevents fast responses due to the RC-constant limitation. Fortunately, the light absorption can be enhanced greatly by reducing the silicon core height hsi, as shown in Fig. 2a, where the absorption coefficients (αg, αm) for the cases with different silicon core heights of hsi = 220, 160, and 100 nm are given. From this figure, one sees that the absorption coefficients αg and αm increase by more than 100% when the core height hsi is reduced from 220 to 100 nm. This result is attributed to the stronger evanescent field for the case with a thinner silicon core. Meanwhile, the graphene absorption ratio ηg increases slightly as the core height hsi decreases. As a result, an ultrathin silicon core is preferred to achieve strong light absorption so that one can use a short absorption section. Here, we choose hsi = 100 nm for our devices based on the feasibility of the fabrication processes. To avoid a long carrier transit time between the electrodes, the ridge width is chosen as wsi = 3 μm. With this design, the absorption coefficients are (αg, αm) = (0.230, 0.098) dB/μm, and the graphene absorption ratio ηg is approximately 70%.

Fig. 2

Mode properties of the present silicon−graphene hybrid plasmonic waveguide when operating at λ = 2 μm.

a Calculated absorption coefficients (αg, αm) and the graphene absorption ratio ηg as the silicon ridge width wsi varies for cases with different silicon ridge heights hsi. Here, wm = 200 nm, and hm = 50 nm. b Calculated absorption coefficients (αg, αm) and the graphene absorption ratio ηg as the metal strip width wm varies for cases with different metal heights hm. Here, wsi = 3 μm, and hsi = 100 nm. c The electric field component distribution of the quasi-TE0 mode for the optimized silicon−graphene hybrid plasmonic waveguide. d Calculated graphene absorptance η as the propagation length L varies for cases with different metal widths of wm = 100, 200, and 300 nm. Here, hm = 50 nm, wsi = 3 μm, and hsi = 100 nm

Figure 2b shows the dependence of the ratio ηg and the absorption coefficients (αg, αm) on the width wm and height hm of the metal strip. Here, the dimensions of the silicon ridge are wsi = 3 μm and hsi = 100 nm. It can be seen that a high ratio ηg can be achieved by choosing a narrow metal strip, which is simply due to a significant reduction in the metal absorption. For example, when choosing wm = 100 nm, the metal absorption coefficient is as small as αm = 0.019 dB/μm, while the ratio ηg is as high as ~90%. However, the graphene absorption coefficient αg also decreases to some degree when the metal strip becomes narrow. Therefore, to have a sufficiently high graphene absorption coefficient and a high absorption ratio ηg, we choose wm = 200 nm in our design, which also makes the fabrication relatively easy and guarantees a low graphene-metal contact resistance for the middle electrode. The absorption coefficients (αg, αm) can also be further enhanced by reducing the metal thickness, as shown in Fig. 2b. However, the graphene absorption ratio ηg also decreases. Therefore, we choose hm = 50 nm as a trade-off.

For the designed silicon−graphene hybrid plasmonic waveguide with wm = 200 nm, hm = 50 nm, wsi = 3 μm, and hsi = 100 nm, the calculated electric field distribution of the quasi-TE0 mode is shown in Fig. 2c. It can be seen that there is strong field localization and enhancement in the area around the metal strip. For example, the electric field component along the graphene layer at the metal corners reaches up to 1.0 × 107 V/m for 1 mW optical power, which helps enhance the light absorption in graphene. For the present design, we calculate the total graphene absorption η(L) as the propagation distance L varies from 0 to 50 μm, as shown in Fig. 2d. It can be seen that the total graphene absorptance is almost saturated at approximately 68.6% for the case of wm = 200 nm when the length L is 50 μm. For a metal width of wm = 300 nm, the total graphene absorptance is close to a saturated value of 51.4% when the length L is 20 μm, which occurs because the metal absorption increases. In contrast, when wm = 100 nm, the total graphene absorption increases to 78.7% (not yet saturated) when the length L increases to 50 μm, which is due to the relatively low absorption coefficients (αg, αm). With such a design, the present silicon−graphene hybrid plasmonic waveguide achieves the best result among the results of the reported silicon−graphene hybrid waveguides (which were developed for 1.55 μm). For a direct comparison, the silicon−graphene hybrid plasmonic waveguide is also designed optimally for 1.55 μm (see Supplementary Note 1), and the graphene absorptance at 1.55 μm is approximately 54.3% for the optimal design with wm = 200 nm when the length L = 20 μm. In contrast, in ref. [24], the graphene absorptance is 44% only for the bi-layer-graphene hybrid plasmonic waveguide with wm = 180 nm and L = 22 μm. For the Si3N4-graphene hybrid plasmonic waveguide with wm = 70 nm in ref. [27], the graphene absorptance η is 42% when the length is L = 40 μm. More recently, a plasmonic-enhanced graphene waveguide with bowtie-shaped metallic structures was reported with a short device length of 6 μm; however, the graphene absorptance is saturated at ~34%[20].

Measurement results and analyses

The designed waveguide photodetectors were fabricated with a series of steps (see Methods), including the processes of electron-beam lithography, ICP etching, Al2O3 atom-layer deposition, graphene transfer, and metal deposition. For the fabricated devices, the I−V characteristics were characterized by varying the gate voltage (see Supplementary Note 2). The contact resistance and the graphene properties were obtained by fitting the measured resistance data with a simple capacitance model[29]. The typical value for the graphene mobility is ~500 cm2/V s, which is not as high as the best results reported by some other groups[28,29]. This might be due to the defects introduced during the fabrication processes; the graphene mobility could possibly be enhanced further by improving the fabrication processes in the future. For all of the devices, the total contact resistances are typically several tens of Ohms, depending on the sizes of the contact regions and some random variations introduced in the fabrication processes. As an example, the total contact resistance is approximately 45 Ω for Device A, which is characterized in more detail in the following sections.

The photocurrents were measured by using a lock-in amplifier (see Methods and Supplementary Note 7). The gate voltage VG is set to less than 4.0 V to avoid the breakdown of the Al2O3 nanolayer. Figure 3a shows the measured photocurrent map for one of the representative devices (Device A) operating with different gate voltages VG and bias voltages Vb. For Device A, the Dirac voltage VDirac is approximately 3.2 V (see the measurement in Supplementary Note 2). The photocurrent map has a fourfold pattern, which is similar to the measured results for the device reported in ref. [28], even though the structural designs of the devices are different. From this figure, it can be seen that the photocurrent strongly depends on the gate voltage VG and the bias voltage Vb. To see more details, the dependence of the photocurrent at zero bias for the gate voltage VG is shown in Fig. 3b, which shows that there is a transition from a positive photocurrent to a negative photocurrent when the gate voltage VG is approximately 2.7 V. It is well known that such behavior for the dependence of the photocurrent on the gate voltage VG is very typical for the PTE photocurrent[47,48]. Our photocurrent modeling in Supplementary Note 6 (see Supplementary Fig. S7d) further confirms that the PTE effect is the dominant mechanism for the zero-bias photocurrent. As shown by the fourfold pattern in Fig. 3a, when the bias voltage Vb is applied, the photocurrent increases greatly, which indicates that the PTE effect is no longer the dominant mechanism. The reason is that the PTE photocurrent is generally not sensitive to the bias voltage Vb, as observed previously[29]. This result is also predicted by the theoretical modeling in Supplementary Note 6. Instead, the dominant mechanisms for generating the photocurrent are very likely to be the BOL effect or the PC effect when Vb ≠ 0. As shown in Fig. 3a, the fourfold photocurrent map has two subparts, i.e., the left and right regions divided by the dotted line located around VG = 2.3−3 V. On the left side, the signs for the measured photocurrent and the bias voltage are opposite, which indicates that the dominant mechanism is the BOL effect[49]. In contrast, on the right side, the signs for the photocurrent and the bias voltage are consistent, which indicates that the dominant mechanism is the PC effect[29].

Fig. 3

Static characterization of the present silicon−graphene hybrid plasmonic waveguide photodetector (Device A).

a Measured photocurrent map as the gate voltage VG and the bias voltage Vb vary. b Dependence of the photocurrent at zero bias for the gate voltage VG. c−f Calculated energy band diagrams for the cases of (VG, Vb) = (2.3, 0.3), (1.9, −0.3), (3.4, 0.3), and (3.2, −0.3) V. g Measured responsivities with different input optical powers Pin. Here, Vb = −0.3 V and VG = ~1.9 V (for the BOL effect), or VG = ~3.2 V (for the PC effect)

In order to better understand the mechanisms of the photodetectors, we also provide theoretical calculations for the Fermi level EF, the Dirac-point energy Φ, and the chemical potential μc along the graphene channel between the signal electrode and the right ground electrode (see the details in Supplementary Note 5), as shown in Fig. 3c–f. In this calculation, the bias voltage is chosen to be Vb = ±0.3 V, while the gate voltage is chosen as VG = ~2.0 and ~3.2 V, located on the left and right sides of the photocurrent map (see the labels in Fig. 3a). Here, the chemical potential for the graphene sheet underneath the gold electrodes is estimated to be approximately −0.1 eV due to the pinning effect[50]. In contrast, the chemical potential of the graphene sheet in the channel center is fully gate-controllable, and there is a transition region gradually varying from the pinning region and the fully gate-controllable region. As shown in Fig. 3c, d, which correspond to the cases with (VG, Vb) = (2.3, 0.3) V and (1.9, −0.3) V, respectively, the graphene sheet is highly doped. As a result, the bolometric coefficient β is large[11,49]; thus, the BOL effect becomes the dominant mechanism. In Fig. 3e, f, which correspond to the cases with (VG, Vb) = (3.4, 0.3) V and (3.2, −0.3) V, respectively, the graphene sheet is lightly doped. As a result, the bolometric coefficient β is small[11,49]; thus, the BOL effect is suppressed. Meanwhile, the lifetime of the photogenerated carriers in graphene becomes long because of the low doping level[49]. In this case, the density of the photogenerated carriers is sufficiently high, and the PC effect becomes the dominant mechanism for the photoresponse.

In summary, when the bias voltage |Vb| increases from 0 to 0.3 V, the dominant mechanism for the photoresponse changes from the PTE effect to the BOL effect or the PC effect, depending on the applied gate voltage. Meanwhile, the responsivity increases significantly if the gate voltage is controlled well. Figure 3g shows the measured responsivity for Device A operating with Vb = −0.3 V when choosing VG = ~1.9 V (the BOL effect) and ~3.2 V (the PC effect). The responsivities for the BOL and PC modes are 35.0 and 25.5 mA/W, respectively, when the input optical power Pin is ~2.2 mW. When the input optical power Pin decreases to 0.28 mW, the responsivities increase to approximately 52.1 and 30.0 mA/W for the BOL mode (VG = ~1.9 V) and the PC mode (VG = ~3.2 V), respectively. Since MGM-type graphene photodetectors often have a high dark current (see the I−V curves in Supplementary Fig. S9a), the signal-to-dark-current ratio is usually relatively low[19-30,43,49] in the absence of photoconductive gain. As shown by the noise analysis presented in Supplementary Note 8, the noise equivalent powers (NEPs) of Device A are 6.68−9.92 × 102 pW/Hz1/2 and 61.7−72.7 pW/Hz1/2 for the BOL and PC modes, respectively, when Pin = 0.28−2.2 mW. It can be seen that the PC mode achieves a better sensitivity than the BOL mode because of the lower dark current and similar responsivity. In the future, the dark current could be reduced by introducing some junction structures[14].

The frequency responses of the devices were measured by using a setup combining a commercial 10 GHz optical modulator and a vector network analyzer (VNA, 40 GHz bandwidth), as shown in Fig. 4a, b. The gate voltages were chosen as VG = 2.1 and 3.4 V, corresponding to the BOL effect and the PC effect, respectively. Because the output optical power of the optical modulator at 2 μm is limited and there is no 2 μm optical amplifier available in the lab, the input optical power to the photodetectors is limited to 0.5 mW. In this case, the small-signal photocurrent (on the scale of μA) is much lower than the dark current (~3 mA). Thus, some notable noise was observed at high frequencies in the measurement, as shown in Fig. 4a, b. From this figure, no notable decay is observed in the frequency range of 1.5−20 GHz for both cases with the BOL effect and the PC effect. Here, the maximal frequency fmax in the measurement is up to 20 GHz, which is limited by the 2 μm optical modulator (with a 3 dB bandwidth of 10 GHz) available in the lab.

Fig. 4

Measured frequency responses of Device A operating at different gate voltages.

a VG = 2.1 V (the BOL mode). b VG = 3.4 V (the PC mode)

Figure 5a, b shows the measured responsivity and the frequency response for another photodetector (Device B) on the same chip. For Device B, the graphene is highly p-doped with a Dirac voltage VDirac larger than 4.0 V (see Supplementary Fig. S3a), which is the maximal gate voltage used in our experiment regarding the breakdown condition of the 10-nm-thick Al2O3 layer. In this case, Device B operates based on the BOL effect. As shown in Fig. 5a, the responsivity is up to 70 mA/W when Vb = −0.3 V and Pin = 0.28 mW. From the measured frequency response shown in Fig. 5b, there is no notable decay in the measured frequency range despite the noise, which shows that the 3 dB bandwidth BW3 dB is also more than 20 GHz.

Fig. 5

Experimental results for Device B operating at λ = 2 μm.

a Measured responsivities with different input powers Pin (Vb = −0.3 V). b Measured frequency response (Vb = −0.5 V and VG = 2.9 V)

To verify the high bandwidth of the present waveguide photodetector, we characterized the third device (Device C) on the same chip, as shown in Fig. 6a. Device C is very similar to Devices A and B and has a grating coupler for 1.55 μm, so that the high-speed measurement setup for 1.55 μm available in the lab can be used. For Device C with a 20-μm-long absorption length, the Dirac voltage VDirac is higher than 4 V (see Supplementary Fig. S3a), and the BOL effect is the dominant mechanism. From Fig. 6a, Device C has a responsivity of 396 mA/W when Vb = −0.3 V and Pin = 0.16 mW. The high responsivity of Device C is attributed to the high light absorption in graphene and thus the high light-induced temperature increase (which is beneficial for achieving a high bolometric photoresponse). Figure 6b shows the measured frequency response of Device C operating at Vb = 0.6 V, which was characterized with the help of an erbium-doped fiber amplifier at 1.55 μm. The measured 3 dB bandwidth is higher than 40 GHz (which is the maximal bandwidth of our VNA). This device was further used to receive high-bit-rate data with the setup shown in Supplementary Fig. S8d. Figure 6c shows the measured eye diagram for the photodetector operating at 30 Gbit/s when Vb = 0.6 V and VG = 2.8 V. It can be seen that the eye diagram is open with a bit rate as high as 30 Gbit/s. More details are provided in Supplementary Note 7.

Fig. 6

Experimental results for Device C when operating at 1.55 μm.

a Measured responsivities with different input powers Pin (Vb = −0.3 V). b Measured frequency response (Vb = 0.6 V and VG = 2.8 V). c Measured eye diagram for a 30 Gbps PRBS data stream when Vb = −1 V and VG = 0.3 V

Comparisons

Here, we provide a comprehensive comparison of the performances of the reported silicon−graphene photodetectors beyond 1.55 μm, as shown in Table 1. Several surface-illuminated silicon−graphene photodetectors with broad operation wavelength bands have been reported. In ref. [35], a silicon−graphene photodetector was demonstrated with a responsivity of 6.25 mA/W at 10 μm and an estimated 3 dB bandwidth of >1 GHz at 1.03 μm. In ref. [36], a silicon−graphene photodetector was reported with responsivities of 0.6−0.076 A/W for an input optical power of 2.5−50 μW. For the device in ref. [36], the measured 3 dB bandwidth was higher than 50 GHz at 0.8 μm, and the responsivity was 2−11.5 A/W for an ultralow optical power in the wavelength range of 3−20 μm. For the waveguide photodetector reported recently[35,41-43], the measured 3 dB bandwidths were on the scale of kHz or not given. In contrast, the present photodetectors (e.g., Device B) have a responsivity of 70 mA/W (at −0.3 V and 0.28 mW) and a setup-limited 3 dB bandwidth of >20 GHz.

Table 1

Performances of graphene photodetectors in the mid-infrared range beyond the 1.55 μm wavelength band

Reference	Type	Mechanism	λ (μm)	(External) Responsivity	Pin (μW)	Vbias (V)	BW3 dB
[35]	GSH, surface-illuminated	IPE	2	0.16 mA/W	~0.5	0	~kHz
[36]a	MGM, surface-illuminated	PV	3	2 A/W	2.5	0.02	–
[37]b	MGM, surface-illuminated (at T = 10 K)	BOL	10	6.25 mA/W	0.8	2.4 × 10−5	–
[38]	GIG, surface-illuminated	Photogating	Up to 3.2	>1 A/W	~6	1	~Hz
[41]	GSH, waveguide-type	IPE	2.75	130 mA/W	<1	1.5	~11 kHz
[42]	GSH, waveguide-type	IPE	2.75	4.5 mA/W	10	−1	–
[43]	MGM, waveguide-type	–	3.8	2 mA/W	~300	−1	–
This work: Device A	MGM, waveguide-type	BOL	2	52 mA/W	280	−0.3	>20 GHzc
This work: Device B				70 mA/W			>20 GHzc

aThe operation wavelength ranges from 0.8 to 20 μm, and the 3 dB bandwidth of 50 GHz is measured at λ = 0.8 μm

bThe operation wavelengths are 0.658, 1.03, 2, and 10 μm. The external responsivity is evaluated from an internal responsivity of 2 × 105 V/W, while the graphene absorptance is 0.5%. The 3 dB bandwidth of >1 GHz is measured at 1.03 μm

cThe 3 dB bandwidths are setup-limited

We further compare the reported silicon−graphene photodetectors in a wavelength band of 1.55 μm, because abundant measurement results are reported in this band, as shown in Fig. 7. Here, only devices with a monolayer graphene sheet and a 3 dB bandwidth of >1 GHz are included. It can be seen that a number of results with high bandwidths of >40 GHz were reported[19-21,26,28,29,31-33]. More recently, the device demonstrated in ref. [20] showed a 3 dB bandwidth of over 110 GHz and 100 Gbps data reception. Similarly, the present silicon−graphene hybrid waveguide photodetector also demonstrates a high 3 dB bandwidth of >40 GHz, which is setup-limited.

Fig. 7

Comprehensive comparisons of previously reported GHz graphene photodetectors at 1.55 μm.

The data are for |Vb | = 0.3 V unless indicated. In refs. [20,21,28,30], the responsivities at |Vb | = 0.3 V are estimated according to the data given in the literature

On the other hand, most of the reported graphene photodetectors have a responsivity of less than 100 mA/W[19,21,25-29,31-33] when operating at a low bias voltage, e.g., |Vb| < 0.3 V. It is well known that, for MGM photodetectors, the responsivities are usually positively correlated with the bias voltages Vb[19-21,23,25-30,35,36,43,49] and negatively correlated with the input optical powers Pin[20,35,36]. Meanwhile, it is usually desirable to be able to detect a low optical power with a low bias voltage because this helps to reduce the dark currents and suppress the shot noise. In Fig. 7, the device responsivities are shown for bias voltages of Vb = ±0.3 V unless no data are provided in the literature. Three graphene photodetectors with a responsivity of >100 mA/W have been reported recently[20,28,30]. For the photodetector reported in ref. [28], the responsivity is estimated to be ~150 mA/W (at 0.3 V) with Pin = 0.025 mW according to the responsivities given for the cases of Vb = 0 and 1.2 V. The other photodetector in ref. [30] has a responsivity of ~140 mA/W (at 0.3 V) with Pin = 0.56 mW, which is estimated from the responsivities given for the cases of Vb = 0 and 0.4 V. In ref. [20], the responsivities are proportional to the bias voltage and are ~375 mA/W and ~150 mA/W when operating with Vb = −0.3 V for Pin of 0.08 and 0.6 mW, respectively. For the present photodetector (Device C) operating at a low bias voltage Vb = −0.3 V, the responsivity at 1.55 μm is as high as ~0.4 A/W with Pin = 0.16 mW, which is the highest value among the results of the various reported high-speed graphene photodetectors. In addition, the tunneling photodiode in ref. [34] with an estimated bandwidth of 56 GHz is not included in Fig. 7, since it operates with a very large bias voltage of ~10 V while the dark current can be kept on the nA scale; therefore, it can realize a high on−off current ratio with a responsivity of 240 mA/W at Pin = 0.42 mW. However, a high bias voltage results in large power consumption and cannot be supported by low-voltage CMOS drivers. In summary, the present silicon−graphene waveguide photodetector works well with a high responsivity and a high bandwidth.

Discussion

In this paper, we have proposed and demonstrated novel silicon−graphene hybrid plasmonic waveguide photodetectors beyond 1.55 μm, which are realized by introducing an ultrathin wide silicon ridge core region with a metal cap at the top. With this design, the light absorption in graphene is enhanced while the metal absorption loss is reduced simultaneously. This design greatly facilitates effective optical absorption in graphene over a short length. Metal−graphene−metal sandwiched electrodes have also been introduced to reduce the metal−graphene-contact resistance, which helps improve the response speed. For the fabricated photodetectors, the mechanism has been revealed from the IV characteristics operating at different gate voltages. It has been shown that the dominant mechanism for the present photodetectors is the PTE effect at zero bias voltage and the BOL or PC effect at nonzero bias voltages, which help achieve high-speed responses. For the fabricated photodetector operating at 2 μm, the measured 3 dB bandwidth is >20 GHz (which is limited by the experimental setup), while the responsivity is ~70 mA/W at Vb = −0.3 V for Pin = 0.28 mW. In order to verify the ultrafast photodetection capability, we have also measured the frequency responses of the present waveguide photodetector operating at 1.55 μm. It is shown that the measured 3 dB bandwidth is >40 GHz (which is still limited by the setup). Meanwhile, the measured responsivity is approximately 0.4 A/W at Vb = −0.3 V for Pin = 0.16 mW, which has some advantages over other photodetectors[19-21,25-33]. It is well known that MGM graphene photodetectors usually suffer from a low signal-to-noise ratio due to the high intrinsic large dark current. Fortunately, this issue can be alleviated partially for the present device, which has relatively high responsivities at low bias voltages. In this paper, Device A at 2 μm has an NEP of 61.7−72.7 pW/Hz1/2, which is slightly better than that of commercial infrared photoconductive PbSe detectors (80 pW/Hz1/2)[51]. For the present 2 μm waveguide photodetectors with large bandwidths, there are some important application scenarios, e.g., 2 μm optical communications[2,3], monitoring of a 2 μm pulsed laser system in mid-infrared time resolved spectroscopy[52], nonlinear photonics[4], and lab-on-chip sensing[5-7]. In short, the present work paves the way for achieving high-responsivity and high-speed near/mid-infrared waveguide photodetectors on silicon, which will play an important role in various applications. In future works, more efforts should be dedicated to introduce special junction structures to reduce the dark current and further extend the operation wavelength band.

Materials and methods

Device fabrication

The ultrathin silicon core layer was obtained from a standard 220-nm-thick SOI wafer. A thermal oxidation process was used to obtain an ~100-nm-thick silicon top layer from a standard 220-nm-thick lightly p-doped SOI wafer. EBL and ICP processes were used for the fabrication of the silicon ridge waveguide with a silicon thickness of hsi = ~100 nm, an etching depth of het = ~50 nm, and a ridge width of wsi = 3 μm. A 90-nm-thick aluminum gate electrode (with an ohmic contact) was fabricated by utilizing lift-off processes. A 10-nm-thick Al2O3 layer was deposited on the SOI ridge waveguide by using an atomic-layer deposition (ALD) process. The bottom layer of the side ground electrodes was made of 15/50-nm-thick Ti/Au hybrid thin films. Then, a single-layer graphene sheet was transferred onto the chip and patterned by EBL and ICP etching processes. Finally, a 50-nm-thick Au layer was deposited and patterned to form the narrow signal electrode and the top layer of the side ground electrodes.

Transfer process of graphene

The CVD-grown graphene was obtained from ACS material LLC (single layer, on copper foil). A 300-nm-thick film of PMMA was spin-coated on the graphene/copper film at 4000 rpm. The PMMA/graphene/copper film was floated on aqueous ammonium persulfate (60 mg/mL) to remove the copper and rinsed in deionized water. Then, the film was transferred onto the chip. The graphene-covered chip was dried, baked, soaked in acetone and rinsed with isopropanol.

Device measurement

The responsivities of the photodetectors were characterized by using low-frequency measurements. Continuous-wave light from a fiber laser was modulated with a frequency of 0.2 kHz by a chopper and then coupled to the optical waveguide by using an on-chip grating coupler. The photocurrent was then amplified and recorded by using a preamplifier and a lock-in amplifier (see Supplementary Fig. S8a, b). The input optical power Pin was estimated according to the measured coupling efficiency of the grating coupler (~10.5 dB at 2 μm) and the power splitting ratio of the directional coupler (~1 dB at 2 μm). More details on the optical power analysis are provided in Supplementary Note 4.

Supplementary Material