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An electron in the first excited state ...

An electron in the first excited state of H atom absorbed a photon and further excited. The de broglie wavelength of the electron in this state is found to be `13.4` Å. Find the wavelength of the photon absorbed by the electron in angstroms. Also find the longest and the shortest wavelength emitted when this electron de-excited back to the ground state.

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To solve the problem step by step, we will first determine the wavelength of the photon absorbed by the electron when it transitions from the first excited state (n=2) to a higher energy level (n=4). Then, we will find the longest and shortest wavelengths emitted when the electron de-excites back to the ground state (n=1). ### Step 1: Determine the value of n for the excited state Given the de Broglie wavelength (λ) of the electron in the excited state is 13.4 Å, we can use the formula derived from Bohr's model: \[ 2\pi r = n \lambda \] Where \( r \) is the radius of the electron's orbit given by: \[ r = \frac{n^2}{Z} \cdot 0.529 \, \text{Å} \] For hydrogen, \( Z = 1 \). Therefore, we can rewrite the equation as: \[ 2\pi \left( \frac{n^2}{1} \cdot 0.529 \right) = n \cdot 13.4 \] This simplifies to: \[ 2\pi \cdot 0.529 n^2 = n \cdot 13.4 \] Dividing both sides by \( n \) (assuming \( n \neq 0 \)): \[ 2\pi \cdot 0.529 n = 13.4 \] Now, solving for \( n \): \[ n = \frac{13.4}{2\pi \cdot 0.529} \] Calculating this gives: \[ n \approx 4 \] ### Step 2: Find the wavelength of the absorbed photon To find the wavelength of the photon absorbed when the electron transitions from n=2 to n=4, we use the Rydberg formula: \[ \frac{1}{\lambda} = R_H \left( \frac{1}{n_L^2} - \frac{1}{n_H^2} \right) \] Where: - \( R_H \) (Rydberg constant) = \( \frac{1}{912} \, \text{Å} \) - \( n_L = 2 \) (lower energy level) - \( n_H = 4 \) (higher energy level) Substituting the values: \[ \frac{1}{\lambda} = \frac{1}{912} \left( \frac{1}{2^2} - \frac{1}{4^2} \right) \] Calculating this gives: \[ \frac{1}{\lambda} = \frac{1}{912} \left( \frac{1}{4} - \frac{1}{16} \right) = \frac{1}{912} \left( \frac{4 - 1}{16} \right) = \frac{3}{16 \cdot 912} \] Calculating \( \lambda \): \[ \lambda = \frac{16 \cdot 912}{3} \approx 4.86 \times 10^3 \, \text{Å} \] ### Step 3: Find the longest and shortest wavelengths emitted When the electron de-excites from n=4 to n=1, it can do so in multiple steps. The longest wavelength corresponds to the transition from n=4 to n=3, and the shortest wavelength corresponds to the transition from n=4 to n=1. **Longest Wavelength (n=4 to n=3):** Using the Rydberg formula again: \[ \frac{1}{\lambda_{max}} = R_H \left( \frac{1}{3^2} - \frac{1}{4^2} \right) \] Calculating: \[ \frac{1}{\lambda_{max}} = \frac{1}{912} \left( \frac{1}{9} - \frac{1}{16} \right) = \frac{1}{912} \left( \frac{16 - 9}{144} \right) = \frac{7}{144 \cdot 912} \] Calculating \( \lambda_{max} \): \[ \lambda_{max} = \frac{144 \cdot 912}{7} \approx 1.87 \times 10^4 \, \text{Å} \] **Shortest Wavelength (n=4 to n=1):** Using the Rydberg formula: \[ \frac{1}{\lambda_{min}} = R_H \left( \frac{1}{1^2} - \frac{1}{4^2} \right) \] Calculating: \[ \frac{1}{\lambda_{min}} = \frac{1}{912} \left( 1 - \frac{1}{16} \right) = \frac{1}{912} \left( \frac{15}{16} \right) = \frac{15}{16 \cdot 912} \] Calculating \( \lambda_{min} \): \[ \lambda_{min} = \frac{16 \cdot 912}{15} \approx 855 \, \text{Å} \] ### Final Answers: - Wavelength of the absorbed photon: \( \approx 4860 \, \text{Å} \) - Longest wavelength emitted: \( \approx 1.87 \times 10^4 \, \text{Å} \) - Shortest wavelength emitted: \( \approx 855 \, \text{Å} \)

To solve the problem step by step, we will first determine the wavelength of the photon absorbed by the electron when it transitions from the first excited state (n=2) to a higher energy level (n=4). Then, we will find the longest and shortest wavelengths emitted when the electron de-excites back to the ground state (n=1). ### Step 1: Determine the value of n for the excited state Given the de Broglie wavelength (λ) of the electron in the excited state is 13.4 Å, we can use the formula derived from Bohr's model: \[ 2\pi r = n \lambda \] ...
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