To solve this problem, we use the Rydberg formula for hydrogen-like ions to calculate the frequency of emitted radiation during electron transitions: \[ \nu = RZ^2\left(\frac{1}{n_1^2} - \frac{1}{n_2^2}\right) \] where \( \nu \) is the frequency, \( R \) is the Rydberg constant (\(1.097 \times 10^7 \, \text{m}^{-1}\)), \( Z \) is the atomic number, and \( n_1 \) and \( n_2 \) are the principal quantum numbers of the two levels.
Given \( \nu_{2 \to 1} = 3 \times 10^{15} \, \text{Hz} \), we find:
\[ \nu_{2 \to 1} = RZ^2\left(\frac{1}{1^2} - \frac{1}{2^2}\right) = RZ^2\left(\frac{3}{4}\right) \]
Using this as a basis, let's calculate \( \nu_{3 \to 1} \):
\[ \nu_{3 \to 1} = RZ^2\left(\frac{1}{1^2} - \frac{1}{3^2}\right) = RZ^2\left(\frac{8}{9}\right) \]
From \( \nu_{2 \to 1} = 3 \times 10^{15} \, \text{Hz} \),
\[ 3 \times 10^{15} = RZ^2\left(\frac{3}{4}\right) \]
Solving for \( RZ^2 \),
\[ RZ^2 = \frac{4 \times 3 \times 10^{15}}{3} = 4 \times 10^{15} \]
Substitute this into \( \nu_{3 \to 1} \):
\[ \nu_{3 \to 1} = 4 \times 10^{15}\left(\frac{8}{9}\right) = \frac{32}{9} \times 10^{15} \, \text{Hz} \]
Comparing this to the requested format \(\frac{x}{9} \times 10^{15}\text{ Hz}\), \(x = 32\). The value \(x = 32\) .
Given: - Frequency of radiation for transition \( n = 2 \) to \( n = 1 \): \( \nu_{2 \to 1} = 3 \times 10^{15} \, \text{Hz} \) - Transition of interest: \( n = 3 \) to \( n = 1 \)
Step 1: Energy Levels for Hydrogen-Like Ion
The energy difference between levels in a hydrogen-like atom is given by: \[ \Delta E \propto \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] The frequency of emitted radiation is proportional to the energy difference: \[ \nu \propto \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \]
Step 2: Calculating the Frequency Ratio
For the transition from \( n = 2 \) to \( n = 1 \):
\[ \nu_{2 \to 1} \propto \left( \frac{1}{1^2} - \frac{1}{2^2} \right) = \left( 1 - \frac{1}{4} \right) = \frac{3}{4} \]
For the transition from \( n = 3 \) to \( n = 1 \):
\[ \nu_{3 \to 1} \propto \left( \frac{1}{1^2} - \frac{1}{3^2} \right) = \left( 1 - \frac{1}{9} \right) = \frac{8}{9} \]
Step 3: Finding the Frequency for \( n = 3 \) to \( n = 1 \) Transition
The ratio of the frequencies for the two transitions is:
\[ \frac{\nu_{3 \to 1}}{\nu_{2 \to 1}} = \frac{\frac{8}{9}}{\frac{3}{4}} = \frac{8}{9} \times \frac{4}{3} = \frac{32}{27} \]
Thus:
\[ \nu_{3 \to 1} = \nu_{2 \to 1} \times \frac{32}{27} \]
Substituting the given value:
\[ \nu_{3 \to 1} = 3 \times 10^{15} \times \frac{32}{27} = \frac{32}{9} \times 10^{15} \, \text{Hz} \]
Step 4: Comparing with Given Expression
The frequency is given as \( \frac{x}{9} \times 10^{15} \, \text{Hz} \). By comparison:
\[ x = 32 \]
Conclusion: The value of \( x \) is 32.
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)