Photoelectric Effect and Stopping Potential:
The photoelectric equation, which describes the energy conservation for the photoelectric effect, is given by:
\[
E_{\text{photon}} = E_{\text{kinetic}} + E_{\text{work}},
\]
where:
- \( E_{\text{photon}} \) is the energy of the incident photon,
- \( E_{\text{kinetic}} \) is the kinetic energy of the emitted electron, and
- \( E_{\text{work}} \) is the work function, which is the minimum energy required to release an electron from the surface.
The energy of a photon is given by:
\[
E_{\text{photon}} = h\nu = \frac{hc}{\lambda},
\]
where:
- \( h \) is Planck's constant,
- \( \nu \) is the frequency of the incident light, and
- \( \lambda \) is the wavelength of the incident light.
The stopping potential \(V\) is related to the kinetic energy of the emitted electron:
\[
E_{\text{kinetic}} = eV,
\]
where \( e \) is the charge of the electron, and \( V \) is the stopping potential. The work function is \( W = h\nu_0 \), where \( \nu_0 \) is the threshold frequency for the photoelectric effect.
For the incident light of wavelength \( \lambda \), the stopping potential is 4V, so we can write:
\[
h\left( \frac{c}{\lambda} \right) = e . 4 + h\nu_0.
\]
For the light of wavelength \( 2\lambda \), the stopping potential becomes \( V \), so we have:
\[
h\left( \frac{c}{2\lambda} \right) = eV + h\nu_0.
\]
By subtracting these two equations, we get:
\[
h \left( \frac{c}{\lambda} - \frac{c}{2\lambda} \right) = e(4 - V).
\]
Simplifying the left-hand side:
\[
h . \frac{c}{2\lambda} = e(4 - V),
\]
and solving for \( V \), we get:
\[
V = 4 - \frac{hc}{2e\lambda}.
\]
Now, for the threshold wavelength \( \lambda_0 \), the stopping potential \( V = 0 \). At this point, the photon energy is equal to the work function:
\[
h . \frac{c}{\lambda_0} = h . \nu_0.
\]
Thus, the formula for the threshold wavelength \( \lambda_0 \) in terms of \( \lambda \) is:
\[
\lambda_0 = 2 \lambda.
\]
This shows that the threshold wavelength is twice the wavelength for which the stopping potential is 4V.