To solve the problem, we need to analyze the energy transitions in a hydrogen atom. The energy levels in a hydrogen atom are given by the formula:
En = -\(\frac{13.6}{n^2}\) eVwhere \(n\) is the principal quantum number. The energy of a photon emitted during a transition from a higher energy level \(n_1\) to a lower energy level \(n_2\) is:
ΔE = En_2 - En_1 = -\(\frac{13.6}{n_2^2}\) + \(\frac{13.6}{n_1^2}\)First, let’s find the energy differences for the specified transitions:
- Transition from third (n=3) to second level (n=2):
ΔE3→2 = -13.6\(\left(\frac{1}{2^2} - \frac{1}{3^2}\right)\) = 13.6\(\left(\frac{1}{4} - \frac{1}{9}\right)\) = 13.6\(\left(\frac{5}{36}\right)\) = 1.89 eV. - Transition from the highest level (n=∞) to the second level (n=2):
ΔE∞→2 = -13.6\(\left(\frac{1}{2^2} - \frac{1}{∞^2}\right)\) = 13.6\(\left(\frac{1}{4}\right)\) = 3.4 eV.
The ratio of energies given by:
\(\frac{ΔE_{3→2}}{ΔE_{∞→2}} = \frac{1.89}{3.4}\)Given that this is \(\frac{x}{x+4}\), equating both expressions gives:
\(\frac{x}{x+4} = \frac{1.89}{3.4}\)Solve for x:
x(3.4) = 1.89(x+4)
3.4x = 1.89x + 7.56
1.51x = 7.56
x ≈ 5