(Digital Presentation) Ge-on-insulator Platform for Mid-infrared Photonic Integrated Circuits
Authors: Takenaka Mitsuru , Zhao Ziqiang , Ho Chong Pei , Fujigaki Takumi , Piyapatarakul Tipat , Miyatake Yuto , Tang Rui , Toprasertpong Kasidit , Takagi Shinichi 
Published: November 2022

Since mid-infrared (MIR) wavelengths have a great potential for optical communication, sensing, and quantum information, Si-based MIR photonic integrated circuits (PICs) have been developed by leveraging Si photonics technology for near-infrared wavelengths. However, the transparency wavelength window of Si is from 1.2 µm to 8 µm, limiting the available wavelengths in the MIR spectrum. Ge is emerging as a waveguide material to overcome this difficulty because Ge is transparent in the entire MIR spectrum. A Ge-on-Si waveguide is one of the promising platform for a MIR PICs. We have also proposed a Ge-on-insulator (GeOI) platform for MIR integrated photonics [1]. The strong optical confinement in a GeOI waveguide enables an ultracompact MIR PIC. Using wafer bonding and smart-cut, a GeOI wafer was successfully fabricated [2]. As a result, we have demonstrated various Ge passive devices, thermo-optic phase shifters, and modulators on a GeOI platform [3][4].
The propagation loss of a GeOI waveguide is one of the issues. The crystal defects induced by hydrogen implantation for smart-cut generates holes in a Ge film. As a result, evening using an n-type Ge donor wafer for smart-cut, a final Ge layer tends to be p-type. Since free-hole absorption in Ge is significant, the propagation loss of a p-type GeOI becomes large. To suppress hole generation, the optimization of the hydrogen implantation conditions was conducted. We found that the higher the implantation energy was, the deeper the center of the defect position was from a Ge surface [5]. When the implantation energy increases from 80 keV to 160 keV, the defects can be removed from a 300-nm-thick Ge device layer, enabling an n-type GeOI wafer. As a result, a low-loss GeOI waveguide with a propagation loss of 2.3 dB/cm was demonstrated.
The monolithic integration of Ge passive waveguides and photodetectors (PDs) is also essential for a MIR PIC. We examined the defect-assist photodetection mechanism in a GeOI waveguide with a lateral PIN junction. When a reverse voltage was applied to the PIN junction, the substantial photocurrent was observed at a wavelength of 2 µm for which Ge is transparent. The defect-assist photodetection is expected to be enhanced due to the large intrinsic carrier density in Ge. As a result, the responsivity of 0.25 A/W was obtained at -5 V.
In conclusion, we have developed a GeOI photonics platform for MIR wavelengths. We have achieved a low-loss Ge waveguide, PDs, and optical modulators, the indispensable building blocks for large-scale MIR PICs. The functionality of a GeOI platform can be extended with emerging materials including graphene and phase change materials.
This work was partly based on the results from the project JPNP13004, commissioned by the New Energy and Industrial Technology Development Organization (NEDO) and supported by JST-Mirai Program Grant Number JPMJMI20A1, JSPS KAKENHI Grant Number JP20H02198, and the Canon Foundation.
Reference
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[5] Z. Zhao et al., “Low-loss Ge waveguide at the 2-µm band on an n-type Ge-on-insulator wafer,” Opt. Mater. Express, OME, vol. 11, no. 12, pp. 4097–4106, Dec. 2021.
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