Energy of photon emitted can be calculated by the formula
\(E = 13.6\left[\frac{1}{n_1^{2}} - \frac{1}{n_2^{2}}\right]\)
The first Balmer spectral line (of minimum energy) emission could be due to the transition between
n1 = 2 and n2 = 3
The energy of this photon
\(= 13.6[\frac{1}{2^2} - \frac{1}{3^2}] = 1.9\ eV\)
As the energy of an incident photon is greater than the work function of metal X but less than the work function of metal Y, this photon can result in photoelectric emission in only metal X.
The second Balmer spectral line (of maximum energy) emission corresponds to the transition:
n1 = 2 and n2 = infinity
The energy of this photon
\(=13.6[\frac{1}{2^2} - \frac{1}{\infty^2}] = 3.4\ eV\)
As the energy of the incident photon exceeds the work functions of both the metal X & Y, this photon can result in photoelectric emission in both metals X and Y.