Answer: \(h\nu = \phi_0 + \frac{1}{2}mv_{max}^2\); energy of photon \(\approx 4.97 \times 10^{-19}\) J (about 3.1 eV).
Einstein’s photoelectric equation:
\[h\nu = \phi_0 + \frac{1}{2}mv_{max}^2 \quad\text{or}\quad h\nu = h\nu_0 + K_{max}\]
Significance of terms:
- \(h\nu\): energy of one incident photon (\(h\) is Planck’s constant, \(\nu\) the frequency of the incident radiation). It is absorbed completely by a single electron.
- \(\phi_0 = h\nu_0\): work function of the metal, the minimum energy needed to free an electron from the metal surface; \(\nu_0\) is the threshold frequency.
- \(\frac{1}{2}mv_{max}^2\): maximum kinetic energy of the emitted photoelectron (the remaining energy after overcoming the work function). It equals \(eV_0\), where \(V_0\) is the stopping potential.
The equation explains why there is no emission below \(\nu_0\) and why \(K_{max}\) depends linearly on frequency but not on intensity.
Numerical: \(\lambda = 4000\) Å \(= 4 \times 10^{-7}\) m.
\[E = \frac{hc}{\lambda} = \frac{6.63 \times 10^{-34} \times 3 \times 10^8}{4 \times 10^{-7}} = 4.97 \times 10^{-19} \text{ J}\]\[E = \frac{4.97 \times 10^{-19}}{1.6 \times 10^{-19}} \approx 3.1 \text{ eV}\]