For this, we use the equation for the Bohr's model:
\[E = E_0 \left(\frac{1}{n_2^2} - \frac{1}{n_1^2}\right)\]
where \(E\) is the photon energy, \(E_0\) is the energy of the first energy shell (-13.6 eV), \(n_1\) is the quantum number of the starting level, and
Show more…