
The wavelength of a spectral line in the hydrogen spectrum is given by:
\[ \frac{1}{\lambda} = RZ^2 \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right), \]
where \( R \) is the Rydberg constant, \( Z \) is the atomic number, \( n_1 \) is the lower energy level, and \( n_2 \) is the higher energy level.
For the shortest wavelength in the Balmer series:
\[ n_1 = 2, \quad n_2 = \infty \]
\[ \frac{1}{\lambda_B} = RZ^2 \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) = RZ^2 \left( \frac{1}{4} \right). \]
For the shortest wavelength in the Lyman series:
\[ n_1 = 1, \quad n_2 = \infty \]
\[ \frac{1}{\lambda_L} = RZ^2 \left( \frac{1}{1^2} - \frac{1}{\infty^2} \right) = RZ^2 (1). \]
Taking the ratio of wavelengths:
\[ \frac{\lambda_B}{\lambda_L} = \frac{\frac{1}{RZ^2 \frac{1}{4}}}{\frac{1}{RZ^2 (1)}} = 4 : 1. \]
Thus, the ratio is:
\[ \lambda_B : \lambda_L = 4 : 1. \]
Final Answer: 4:1 (Option 1)
The problem asks for the ratio of the shortest wavelength of the Balmer series to the shortest wavelength of the Lyman series for a hydrogen atom.
1. Rydberg's Formula: The wavelength \( \lambda \) of the radiation emitted when an electron in a hydrogen-like atom makes a transition from a higher energy level \( n_i \) to a lower energy level \( n_f \) is given by Rydberg's formula:
\[ \frac{1}{\lambda} = R Z^2 \left( \frac{1}{n_f^2} - \frac{1}{n_i^2} \right) \]where \( R \) is the Rydberg constant and \( Z \) is the atomic number. For a hydrogen atom, \( Z = 1 \).
2. Lyman and Balmer Series:
3. Shortest Wavelength (Series Limit): The energy of the emitted photon is \( E = \frac{hc}{\lambda} \). To have the shortest wavelength (\( \lambda_{\text{min}} \)), the energy of the transition must be maximum. This occurs when the electron transitions from the highest possible energy level, which is \( n_i = \infty \).
Step 1: Determine the shortest wavelength of the Lyman series (\( \lambda_{\text{Lyman, min}} \)).
For the Lyman series, the final state is \( n_f = 1 \). For the shortest wavelength, the initial state is \( n_i = \infty \). For hydrogen, \( Z=1 \). Substituting these values into Rydberg's formula:
\[ \frac{1}{\lambda_{\text{Lyman, min}}} = R (1)^2 \left( \frac{1}{1^2} - \frac{1}{\infty^2} \right) \]Since \( \frac{1}{\infty^2} = 0 \), the equation simplifies to:
\[ \frac{1}{\lambda_{\text{Lyman, min}}} = R (1 - 0) = R \]Therefore, the shortest wavelength for the Lyman series is:
\[ \lambda_{\text{Lyman, min}} = \frac{1}{R} \]Step 2: Determine the shortest wavelength of the Balmer series (\( \lambda_{\text{Balmer, min}} \)).
For the Balmer series, the final state is \( n_f = 2 \). For the shortest wavelength, the initial state is \( n_i = \infty \). Again, for hydrogen, \( Z=1 \). Substituting these values into Rydberg's formula:
\[ \frac{1}{\lambda_{\text{Balmer, min}}} = R (1)^2 \left( \frac{1}{2^2} - \frac{1}{\infty^2} \right) \]This simplifies to:
\[ \frac{1}{\lambda_{\text{Balmer, min}}} = R \left( \frac{1}{4} - 0 \right) = \frac{R}{4} \]Therefore, the shortest wavelength for the Balmer series is:
\[ \lambda_{\text{Balmer, min}} = \frac{4}{R} \]Step 3: Calculate the ratio of the shortest wavelength of the Balmer series to that of the Lyman series.
\[ \frac{\lambda_{\text{Balmer, min}}}{\lambda_{\text{Lyman, min}}} = \frac{4/R}{1/R} \] \[ \frac{\lambda_{\text{Balmer, min}}}{\lambda_{\text{Lyman, min}}} = 4 \]Thus, the ratio of the shortest wavelength of the Balmer series to the shortest wavelength of the Lyman series is 4:1.
Let \( f : \mathbb{R} \to \mathbb{R} \) be a twice differentiable function such that \[ (\sin x \cos y)(f(2x + 2y) - f(2x - 2y)) = (\cos x \sin y)(f(2x + 2y) + f(2x - 2y)), \] for all \( x, y \in \mathbb{R}. \)
If \( f'(0) = \frac{1}{2} \), then the value of \( 24f''\left( \frac{5\pi}{3} \right) \) is: