1.6:1 bandwidth two-layer antireflection structure for silicon matched to the 190–310 GHz atmospheric window
Abstract
Although high-resistivity, low-loss silicon is an excellent material for terahertz transmission optics, its high refractive index necessitates an antireflection treatment. We fabricated a wide-bandwidth, two-layer antireflection treatment by cutting subwavelength structures into the silicon surface using multi-depth deep reactive-ion etching (DRIE). A wafer with this treatment on both sides has <−20 dB<−20 dB (<1%<1%) reflectance over 187–317 GHz at a 15° angle of incidence in TE polarization. We also demonstrated that bonding wafers introduce no reflection features above the −20 dB−20 dB level (also in TE at 15°), reproducing previous work. Together these developments immediately enable construction of wide-bandwidth silicon vacuum windows and represent two important steps toward gradient-index silicon optics with integral broadband antireflection treatment.
Additional Information
© 2018 Optical Society of America. Received 16 March 2018; revised 17 May 2018; accepted 22 May 2018; posted 22 May 2018 (Doc. ID 326119); published 19 June 2018. We performed this work at the California Institute of Technology, the Caltech Submillimeter Observatory Hilo office, the Harvard-Smithsonian Center for Astrophysics, and the MicroDevices Laboratory of the Jet Propulsion Laboratory (operated by the California Institute of Technology under a contract with the National Aeronautics and Space Administration). The authors thank A. Bose for early, pathfinding HFSS simulation work, K. McClure for contributions to the HFSS tolerancing simulations, K. Yee for performing the wafer-bonding steps, J. Wong for contributions to the test setup control code, E. Padilla for undertaking preparatory measurements of the two-layer structures, C.-Y. E. Tong for participation in the Fig. 14 alternate technique measurements, and T. Macioce for contributions to the text of the paper. C. de Young acknowledges support from an SAO Internship. D. Bisel, K. Deniston, and S. Stoll provided able administrative support. Funding: National Aeronautics and Space Administration (NASA) (NNX15AE01G).Attached Files
Accepted Version - 1803.05168
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Additional details
- Eprint ID
- 87565
- DOI
- 10.1364/AO.57.005196
- Resolver ID
- CaltechAUTHORS:20180705-143644278
- NNX15AE01G
- NASA
- NASA/JPL/Caltech
- Smithsonian Astrophysical Observatory
- Created
-
2018-07-06Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department