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OPA855 Datasheet(PDF) 24 Page - Texas Instruments |
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OPA855 Datasheet(HTML) 24 Page - Texas Instruments |
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24 / 41 page ![]() OPA855 offers 8 GHz of gain bandwidth, high slew-rate, and low noise which makes this device an excellent for a wide range of photodetectors. Figure 9-5 shows the OPA855 configured as a transimpedance amplifier (TIA) in a wide-bandwidth, optical front-end system. Various types of optical sensors can be used as an optical input to the amplifier: photodiode (PD), avalanche photodiode (APD), photomultiplier tube (PMT), and multipixel photon counter (MPPC) or known as solid-state photomultiplier (SiPM). Optical detection applications have commonly used APDs, but ultra-low light source detection has been a challenge in past options. With technologies such as PMTs and MPPCs, the high intrinsic gain, while maintaining a fast output, requires a low noise, high-speed interface. The OPA855 can accommodate for these optical challenges and can work equally as well in these applications. + – RF CF VBIAS VOUT Geiger-Mode APD RQ Cathode Anode GND Anode PMT PIN/ APD SiPM/MPPC Photoelectron Dynode Dynode Figure 9-5. Transimpedance Amplifier With APD or SiPM/MPPC or PMT Inputs Transimpedance applications require low voltage and current noise for an excellent system performance. As a result of the high input impedance structure, the OPA855 has a great balance between low input-referred voltage noise and current noise that is consistent over frequency. Overall, the amplifier noise must have minimal impact to the total noise of the application. Examine the total input referred noise to the optical sensor. Noise sources in optical sensors vary especially when introducing gain and photon paralleling. Optical power, gain, and applied reverse bias are the main characteristics that can affect signal to noise ratio. Standard photodiodes contribute the lowest noise at the highest quantum efficiency. Internal to photodiodes, noises sources include shot and thermal. Shot noise is a random occurrence of photodetection which arises in periods of both light and dark. Dark current is noise that occurs in the absence of an optical source which can be included with shot noise. And, thermal noise originates from the shunt resistance internal to the diode. At the lower signal levels, shot noise can dominate. Figure 9-6 shows an example of the noise sources present in a transimpedance amplifier circuit. The total TIA noise is the root sum square of each component within the system: photodiode noise, amplifier current noise, amplifier voltage noise, and feedback resistor noise. iN_Amp VN_Amp VOUT RF VN_R iN_D CD CF RD VBIAS + – * * * * Figure 9-6. Photodiode and TIA Noise Model OPA855 SBOS622D – JULY 2018 – REVISED MAY 2025 www.ti.com 24 Submit Document Feedback Copyright © 2025 Texas Instruments Incorporated Product Folder Links: OPA855 |
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