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What is the energy difference and the frequency of light emitted when the electron in a hydrogen atom undergoes transition from the energy level `n = 4` to the energy `n = 3` given that the value of Rydberg constant is `1.0974 xx 10^(7)m^(-1)`?

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To find the energy difference and the frequency of light emitted when an electron in a hydrogen atom transitions from the energy level \( n = 4 \) to \( n = 3 \), we can follow these steps: ### Step 1: Use the Rydberg Formula The Rydberg formula for the wavelength of light emitted during a transition in a hydrogen atom is given by: \[ \frac{1}{\lambda} = R \cdot \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] Where: - \( R \) is the Rydberg constant \( (1.0974 \times 10^7 \, \text{m}^{-1}) \) - \( n_1 = 3 \) (final energy level) - \( n_2 = 4 \) (initial energy level) ### Step 2: Calculate the Wavelength Substituting the values into the formula: \[ \frac{1}{\lambda} = 1.0974 \times 10^7 \cdot \left( \frac{1}{3^2} - \frac{1}{4^2} \right) \] Calculating \( \frac{1}{3^2} \) and \( \frac{1}{4^2} \): \[ \frac{1}{3^2} = \frac{1}{9} \quad \text{and} \quad \frac{1}{4^2} = \frac{1}{16} \] Finding a common denominator (144): \[ \frac{1}{9} = \frac{16}{144} \quad \text{and} \quad \frac{1}{16} = \frac{9}{144} \] Thus: \[ \frac{1}{3^2} - \frac{1}{4^2} = \frac{16}{144} - \frac{9}{144} = \frac{7}{144} \] Now substituting back into the Rydberg formula: \[ \frac{1}{\lambda} = 1.0974 \times 10^7 \cdot \frac{7}{144} \] Calculating \( \frac{1}{\lambda} \): \[ \frac{1}{\lambda} = \frac{1.0974 \times 10^7 \cdot 7}{144} \] ### Step 3: Calculate the Frequency We know that the frequency \( \nu \) is related to the wavelength \( \lambda \) by the equation: \[ \nu = \frac{c}{\lambda} \] Where \( c \) is the speed of light \( (3 \times 10^8 \, \text{m/s}) \). Since we have \( \frac{1}{\lambda} \), we can express the frequency as: \[ \nu = R \cdot c \cdot \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] Substituting the known values: \[ \nu = 1.0974 \times 10^7 \cdot 3 \times 10^8 \cdot \frac{7}{144} \] Calculating this gives: \[ \nu = \frac{3.0002 \times 10^{15}}{144} \approx 2.083 \times 10^{14} \, \text{s}^{-1} \] ### Step 4: Calculate the Energy Difference The energy difference \( \Delta E \) can be calculated using Planck's equation: \[ \Delta E = h \cdot \nu \] Where \( h \) is Planck's constant \( (6.626 \times 10^{-34} \, \text{J s}) \). Substituting the values: \[ \Delta E = 6.626 \times 10^{-34} \cdot 2.083 \times 10^{14} \] Calculating this gives: \[ \Delta E \approx 1.38 \times 10^{-19} \, \text{J} \] ### Final Results - The energy difference \( \Delta E \) is approximately \( 1.38 \times 10^{-19} \, \text{J} \). - The frequency \( \nu \) is approximately \( 2.083 \times 10^{14} \, \text{s}^{-1} \).

To find the energy difference and the frequency of light emitted when an electron in a hydrogen atom transitions from the energy level \( n = 4 \) to \( n = 3 \), we can follow these steps: ### Step 1: Use the Rydberg Formula The Rydberg formula for the wavelength of light emitted during a transition in a hydrogen atom is given by: \[ \frac{1}{\lambda} = R \cdot \left( \frac{1}{n_1^2} - \frac{1}{n_2^2} \right) \] ...
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