Step 1: {Understanding the Rydberg Formula}
The Rydberg formula for the wavelength \( \lambda \) of emitted radiation during an electron transition is:
\[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \]
Here, \( R \) is the Rydberg constant, \( Z \) is the atomic number, and \( n_1 \) and \( n_2 \) are the principal quantum numbers.
Step 2: {Applying to Hydrogen and Helium Ions}
For hydrogen (\( Z = 1 \)), the transition wavelength \( n_2 \to n_1 \) is:
\[ \frac{1}{\lambda_H} = R(1)^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \]
For the He$^+$ ion (\( Z = 2 \)), the transition wavelength \( n_4 \to n_3 \) is:
\[ \frac{1}{\lambda_{He}} = R(2)^2 \left( \frac{1}{n_3^2} - \frac{1}{n_4^2} \right) \]
When \( \lambda_H = \lambda_{He} \), the equation becomes:
\[ \frac{1}{n_1^2} - \frac{1}{n_2^2} = 4 \left( \frac{1}{n_3^2} - \frac{1}{n_4^2} \right) \]
The integer solution \( n_3 = 2 \) and \( n_4 = 4 \) satisfies this condition.
Therefore, the correct transition is \( n = 4 \to n = 2 \, \>. \)
A particle is moving in a straight line. The variation of position $ x $ as a function of time $ t $ is given as:
$ x = t^3 - 6t^2 + 20t + 15 $.
The velocity of the body when its acceleration becomes zero is: