Open AccessActive phase correction of high resolution silicon photonic arrayed waveguide gratings
Author(s) -
Michael Gehl,
Douglas C. Trotter,
Andrew Starbuck,
Andrew Pomerene,
Anthony L. Lentine,
Christopher T. DeRose
Publication year - 2017
Publication title -
optics express
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.394
H-Index - 271
ISSN - 1094-4087
DOI - 10.1364/oe.25.006320
Subject(s) - optics , photonics , waveguide , silicon on insulator , silicon photonics , materials science , optical path , optoelectronics , wafer , photonic integrated circuit , refractive index , refractive index contrast , fabrication , optical path length , phase (matter) , silicon , physics , medicine , alternative medicine , pathology , quantum mechanics
Arrayed waveguide gratings provide flexible spectral filtering functionality for integrated photonic applications. Achieving narrow channel spacing requires long optical path lengths which can greatly increase the footprint of devices. High index contrast waveguides, such as those fabricated in silicon-on-insulator wafers, allow tight waveguide bends which can be used to create much more compact designs. Both the long optical path lengths and the high index contrast contribute to significant optical phase error as light propagates through the device. Therefore, silicon photonic arrayed waveguide gratings require active or passive phase correction following fabrication. Here we present the design and fabrication of compact silicon photonic arrayed waveguide gratings with channel spacings of 50, 10 and 1 GHz. The largest device, with 11 channels of 1 GHz spacing, has a footprint of only 1.1 cm 2 . Using integrated thermo-optic phase shifters, the phase error is actively corrected. We present two methods of phase error correction and demonstrate state-of-the-art cross-talk performance for high index contrast arrayed waveguide gratings. As a demonstration of possible applications, we perform RF channelization with 1 GHz resolution. Additionally, we generate unique spectral filters by applying non-zero phase offsets calculated by the Gerchberg Saxton algorithm.