Noise equivalent power (NEP)
The optical input power that produces a signal equal to the detector's noise in a 1 Hz bandwidth. The standard figure of merit for photodetector sensitivity.
NEP is the input optical power that produces a photocurrent equal to the detector's noise current in a 1 Hz electrical bandwidth:
where is the RMS noise current per and is the responsivity.
Total noise current sums contributions from shot noise on dark current and the amplifier:
where is dark current, is the load (or transimpedance) resistance, is the amplifier input-referred current noise, is APD gain ( for PIN), is the APD excess noise factor, and is the multiplied portion of the dark current.
At low light levels, NEP is dominated by dark current and amplifier noise (independent of signal). At high light levels, signal shot noise dominates and NEP is meaningless — the signal is well above noise by definition.
Typical NEP values at 1550 nm:
| Detector | NEP |
|---|---|
| InGaAs PIN, 50 μm, transimpedance amp | W/ |
| InGaAs PIN, 1 mm, large-area, low-noise amp | W/ |
| InGaAs APD, | W/ |
| Single-photon InGaAs APD (Geiger mode) | quantum-limited; quoted as dark count rate instead |
| Cooled superconducting nanowire (SNSPD) | W/ effective |
| Si PIN, large-area, °C | W/ |
NEP scales with for a measurement bandwidth : minimum detectable power . A receiver with W/ at 10 GHz bandwidth has minimum detectable power W = dBm.
For telecom receivers, the relevant figure is usually input-referred sensitivity at a target bit error rate — typically to dBm for direct-detection 10–25 Gb/s — rather than NEP directly. NEP remains the standard metric for instrumentation photodetectors (lock-in amplifiers, FTIR spectrometers, low-light imaging).