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26 February 2010Challenges of developing resonant cavity photon-counting detectors at 1064 nm
Deep Space Optical Communications (DSOC)) impose challenging requirements on detector sensitivity and bandwidth
[1]. The current state-of-the art of high-repetition rate, high-power lasers recommends using near-infrared (NIR) 1064nm
wavelengths for specific DSOC tasks [2]. Large photonic arrays with integrated beam acquisition, tracking and/or
communication capabilities, and smart pixel architecture should allow the implementation of more reliable and robust
DSOC systems. Integration of smart pixel technology for parallel data read, acquisition and processing is currently
available in silicon. Therefore it would be desirable to monolithically integrate the photodetectors with the electronics.
However, silicon has a weak absorption at 1064nm. One elegant approach to increase its absorption efficiency is to trap
the photons inside the silicon using the cavity resonance effect (resonant cavity enhancement or RCE).
We present in this paper the challenges of developing resonant cavity single-photon detector arrays for applications to
DSOC. The metrics of the main process parameters to fabricate resonant cavity detectors is analyzed and critical process
steps are developed and evaluated.
We conclude that such detector arrays are feasible using current state-of-the-art CMOS technology, provided that
suitable process control protocols are developed. We report a 10X performance enhancement at NIR wavelengths for the
first generation of resonant cavity single-photon detector prototypes, less than 150ps timing performance in photonstarved
mode and 20-30ps for multi-photon hits.
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Stefan Vasile, M. Selim Ünlü, Jerold Lipson, "Challenges of developing resonant cavity photon-counting detectors at 1064 nm," Proc. SPIE 7587, Free-Space Laser Communication Technologies XXII, 75870T (26 February 2010); https://doi.org/10.1117/12.845260