Photoelectrons are emitted from various depths within the metal. Those originating from deeper layers expend energy to overcome internal resistance and collide with atoms before reaching the surface.
Consequently, the kinetic energy of photoelectrons is calculated as:
\( K.E. = hu - \phi - \text{energy lost inside the metal} \)
This energy loss results in varying kinetic energies among the emitted photoelectrons.
Saturation current signifies the maximum photocurrent, achieved when all emitted electrons are collected. An increase in light intensity leads to a greater number of photons striking the metal per unit time, thus increasing the emission rate of photoelectrons.
As current is directly proportional to the number of charge carriers, the saturation current rises with increasing light intensity.
The energy of a photon is defined by:
\( E = \frac{hc}{\lambda} \)
As the wavelength \( \lambda \) increases, the photon energy \( E \) diminishes. When \( \lambda \) reaches a point where \( E \) is less than the metal's work function (\( \phi \)), photons lack sufficient energy to eject electrons.
Therefore, photoemission ceases beyond a specific cut-off wavelength \( \lambda_0 \), determined by:
\( \lambda_0 = \frac{hc}{\phi} \)