The Magic of Photodiodes
Imagine a device that can literally 'see' light and convert it into an electrical signal. That's exactly what a photodiode does! But to understand how it behaves when we tweak its settings, we need to dive into the physics of its operation.
The Reverse Bias Setup
A photodiode is essentially a p-n junction, but it is intentionally operated in reverse bias. Why? Because in reverse bias, the normal current (called dark current) is extremely small. This makes it much easier to detect the tiny additional current created when light shines on it. When we apply a reverse biasing voltage, the depletion region at the junction widens, creating a strong electric field.
The Birth of Photocurrent
When photons of light with sufficient energy hit the depletion region, they knock electrons loose, creating electron-hole pairs. The strong electric field immediately grabs these newly born carriers—sweeping electrons towards the n-side and holes towards the p-side. This flow of charges is what we call the photocurrent.
The Saturation Phase
Now, what happens if we keep increasing the reverse biasing voltage? Initially, a stronger voltage means a stronger electric field, which sweeps the carriers more efficiently before they have a chance to recombine. So, the photocurrent increases initially.
However, there is a limit. The number of electron-hole pairs generated per second depends entirely on the intensity of the incident light, not the voltage. Once the voltage is high enough to sweep all the generated carriers across the junction, the current cannot increase any further. It hits a ceiling. We say the photocurrent saturates finally.
Therefore, the correct behavior of the photocurrent magnitude with increasing biasing voltage is that it increases initially and then saturates.