To solve this problem, we need to use the concept of energy levels in a hydrogen atom. The energy difference between two levels \( n_1 \) and \( n_2 \) in a hydrogen atom can be calculated using the Rydberg formula: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] where \( \lambda \) is the wavelength of emitted radiation, and \( R_H \) is the Rydberg constant.
Step 1: Calculate \( \lambda_0 \)
For an electron jumping from the second excited state (\( n=3 \)) to the first excited state (\( n=2 \)), the wavelength is \(\lambda_0\). Thus: \[ \frac{1}{\lambda_0} = R_H \left( \frac{1}{2^2} - \frac{1}{3^2} \right) = R_H \left( \frac{1}{4} - \frac{1}{9} \right) = R_H \cdot \frac{5}{36} \]
Step 2: Calculate new wavelength
When the electron jumps from the third excited state (\( n=4 \)) to the second orbit (\( n=2 \)): \[ \frac{1}{\lambda} = R_H \left( \frac{1}{2^2} - \frac{1}{4^2} \right) = R_H \left( \frac{1}{4} - \frac{1}{16} \right) = R_H \cdot \frac{3}{16} \]
Step 3: Relate \( \lambda \) and \( \lambda_0 \)
Given \(\lambda = \frac{20}{x} \lambda_0\), equate the two expressions: \[ \frac{1}{\frac{20}{x}\lambda_0} = R_H \cdot \frac{3}{16} \]
Replacing \(\lambda_0\): \[ \frac{x}{20\lambda_0} = R_H \cdot \frac{3}{16} \]
Using the expression for \( \lambda_0 \): \[ \frac{x}{20} \cdot R_H \cdot \frac{5}{36} = R_H \cdot \frac{3}{16} \]
Simplifying and solving for \( x \): \[ \frac{x}{20} \cdot \frac{5}{36} = \frac{3}{16} \rightarrow \frac{5x}{720} = \frac{3}{16} \rightarrow 5x = 135 \rightarrow x = 27 \]
Therefore, \( x = 27 \), which is within the expected range (27,27).