Optisystem Simulation of Cost-Effective PIN-TIA Design for 1 GBPS Achieving Near-APD BER
DOI:
https://doi.org/10.66411/jer.v41i2.422Keywords:
APD, PIN photodiode, transimpedance amplifier (TIA), free-space optics (FSO), BER, Q-factor, receiver sensitivity, shot noise, excess noise factor, thermal noise, OptiSystemAbstract
Selecting the right photodetector front-end is one of the most consequential engineering decisions in free-space optical (FSO) system design. Avalanche photodiodes (APDs) deliver substantial sensitivity improvements through internal multiplication gain, yet their demanding high-voltage bias requirements and temperature-dependent gain introduce cost and complexity that are often difficult to justify in moderate-distance links. PIN photodiodes occupy the opposite extreme—simple, inexpensive, and entirely free of excess multiplication noise—but their performance degrades sharply as received power falls and thermal noise begins to dominate. This paper investigates whether a PIN photodiode paired with a transimpedance amplifier (PIN–TIA) can bridge that gap: recovering much of the APD's sensitivity advantage while preserving the simplicity and low cost of a PIN-based front-end. Three receiver topologies are compared for a 1 Gbps FSO link—APD, standalone PIN, and PIN–TIA—using a rigorous noise-budget derivation and a controlled OptiSystem simulation in which all three branches share the same received optical signal through an identical-loss optical coupler. Bit error rate (BER) is evaluated over a link-distance sweep from 6 km to 12 km at 1 dB/km and over a responsivity sweep at fixed 6 dB attenuation. Across both sweep dimensions, the PIN–TIA tracks the APD BER curve closely and outperforms the standalone PIN by a substantial margin, establishing it as a compelling cost-effective alternative for near-APD performance in practical 1 Gbps FSO deployments.
References
[1] M. A. Khalighi and M. Uysal, "Survey on free space optical communication: A communication theory perspective," IEEE Commun. Surveys Tuts., vol. 16, no. 4, pp. 2231–2258, 4th Qtr., 2014. DOI: https://doi.org/10.1109/COMST.2014.2329501
[2] A. Trichili, M. A. Cox, B. S. Ooi, and M.-S. Alouini, "Roadmap to free space optics," J. Opt. Soc. Am. B, vol. 37, no. 11, pp. A184–A201, Nov. 2020. DOI: https://doi.org/10.1364/JOSAB.399168
[3] Z. Ghassemlooy, W. Popoola, and S. Rajbhandari, Optical Wireless Communications: System and Channel Modelling with MATLAB. Boca Raton, FL, USA: CRC Press, 2012.
[4] A. U. Chaudhry and H. Yanikomeroglu, "Free space optics for next-generation satellite networks," IEEE Consum. Electron. Mag., vol. 10, no. 6, pp. 21–31, Nov. 2021. DOI: https://doi.org/10.1109/MCE.2020.3029772
[5] J. Liang, A. U. Chaudhry, E. Erdogan, H. Yanikomeroglu, G. K. Kurt, P. Hu, K. Ahmed, and S. Martel, "Free-space optical satellite networks performance analysis: Transmission power, latency, and outage probability," IEEE Open J. Veh. Technol., vol. 5, pp. 244–261, 2024. DOI: https://doi.org/10.1109/OJVT.2023.3341409
[6] L. C. Andrews and R. L. Phillips, Laser Beam Propagation Through Random Media, 2nd ed. Bellingham, WA, USA: SPIE Press, 2005. DOI: https://doi.org/10.1117/3.626196
[7] M. A. Esmail, H. Fathallah, and M.-S. Alouini, "Outdoor FSO communications under fog: Attenuation modeling and performance evaluation," IEEE Photonics J., vol. 8, no. 4, Art. no. 7905622, Aug. 2016. DOI: https://doi.org/10.1109/JPHOT.2016.2592705
[8] R. J. McIntyre, "Multiplication noise in uniform avalanche diodes," IEEE Trans. Electron Devices, vol. 13, no. 1, pp. 164–168, Jan. 1966. DOI: https://doi.org/10.1109/T-ED.1966.15651
[9] F. Capasso, "Physics of avalanche photodiodes," in Semiconductors and Semimetals, vol. 22, New York, NY, USA: Academic, 1985, pp. 1–172. DOI: https://doi.org/10.1016/S0080-8784(08)62952-X
[10] X. Jiang et al., "InGaAs/InAlAs avalanche photodiodes for high speed optical communications," J. Lightw. Technol., vol. 38, no. 12, pp. 3365–3373, Jun. 2020.
[11] B. E. A. Saleh and M. C. Teich, Fundamentals of Photonics, 2nd ed. Hoboken, NJ, USA: Wiley, 2007.
[12] G. P. Agrawal, Fiber-Optic Communication Systems, 4th ed. New York, NY, USA: Wiley, 2010. DOI: https://doi.org/10.1002/9780470918524
[13] B. Razavi, "The transimpedance amplifier," IEEE Solid-State Circuits Mag., vol. 11, no. 1, pp. 10–15, Winter 2019. DOI: https://doi.org/10.1109/MSSC.2017.2771102
[14] A. A. Abidi, "On the choice of optimum FET size in wide-band transimpedance amplifiers," J. Lightw. Technol., vol. LT-6, no. 1, pp. 64–66, Jan. 1988. DOI: https://doi.org/10.1109/50.3965
[15] F. Xu, M.-A. Khalighi, and S. Bourennane, "Impact of different noise sources on the performance of PIN- and APD-based FSO receivers," in Proc. 11th Int. Conf. Telecommun. (ConTEL), Graz, Austria, Jun. 2011, pp. 211–218.
[16] O. Kharraz and D. Forsyth, "Performance comparisons between PIN and APD photodetectors for use in optical communication systems," Optik, vol. 124, no. 13, pp. 1493–1498, Jul. 2013. DOI: https://doi.org/10.1016/j.ijleo.2012.04.008
[17] Optiwave Systems Inc., OptiSystem User Reference and Component Models. Ottawa, ON, Canada: Optiwave, 2020.
[18] S. D. Personick, "Receiver design for digital fiber optic communication systems, Parts I and II," Bell Syst. Tech. J., vol. 52, no. 6, pp. 843–886, Jul.–Aug. 1973. DOI: https://doi.org/10.1002/j.1538-7305.1973.tb01994.x
[19] P. P. Webb, R. J. McIntyre, and J. Conradi, "Properties of avalanche photodiodes," RCA Rev., vol. 35, pp. 234–278, Jun. 1974.
[20] G. P. Agrawal, Fiber-Optic Communication Systems, 5th ed. Hoboken, NJ, USA: Wiley, 2021. DOI: https://doi.org/10.1002/9781119737391
[21] R. Wu et al., "A 40-Gb/s transimpedance amplifier in 0.18-µm CMOS for optical communications," IEEE J. Solid-State Circuits, vol. 39, no. 6, pp. 925–931, Jun. 2004.
[22] Y. Huang et al., "A broadband transimpedance amplifier with bandwidth enhancement for optical receivers," IEEE Trans. Microw. Theory Tech., vol. 69, no. 1, pp. 352–362, Jan. 2021.
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