The de-Broglie wavelength \(\lambda_e\) of emitted electrons from a photo-emissive substance is determined using the photoelectric effect and energy conservation. The incident photon energy is \( E_{\text{incident}} = \frac{hc}{\lambda_i} \), where \( \lambda_i \) is the incident radiation wavelength, \( h \) is Planck's constant, and \( c \) is the speed of light.
In the photoelectric effect, incident photon energy equals the work function \(\phi\) plus the kinetic energy of the emitted electron: \(\frac{hc}{\lambda_i} = \phi + \frac{1}{2}mv^2\), where \( \frac{1}{2}mv^2 \) is the kinetic energy of an electron with velocity \( v \) and mass \( m \).
The threshold wavelength \(\lambda_0\) corresponds to the work function: \(\phi = \frac{hc}{\lambda_0}\).
Substituting \(\phi\) into the incident energy equation yields: \(\frac{hc}{\lambda_i} = \frac{hc}{\lambda_0} + \frac{1}{2}mv^2\).
Rearranging for kinetic energy: \(\frac{1}{2}mv^2 = \frac{hc}{\lambda_i} - \frac{hc}{\lambda_0}\).
The de-Broglie wavelength \(\lambda_e\) of the electron is given by: \(\lambda_e = \frac{h}{mv}\).
From the kinetic energy equation: \(\frac{1}{2}mv^2 = \frac{h \cdot c}{\lambda_i} - \frac{h \cdot c}{\lambda_0}\).
Solving for \( v \): \( v = \sqrt{\frac{2hc}{m} \left(\frac{1}{\lambda_i} - \frac{1}{\lambda_0} \right)} \).
Substituting \( v \) into the de-Broglie wavelength formula: \(\lambda_e = \frac{h}{\sqrt{2mc \left(\frac{h}{\lambda_i} - \frac{h}{\lambda_0} \right)}} \).
The correct expression is: \(<\lambda_e = \frac{h}{\sqrt{2mc \left(\frac{h}{\lambda_i} - \frac{h}{\lambda_0} \right)}}\).