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Find the binding anergy of an electron i...

Find the binding anergy of an electron in the ground state of a hydrogen like atom in whose spectrum the thrid Balmer line is equal to 108.5 mm.

A

`54.4 eV`

B

`13.6 eV`

C

`112.4 eV`

D

None of these

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To find the binding energy of an electron in the ground state of a hydrogen-like atom, given that the third Balmer line has a wavelength of 108.5 nm, we can follow these steps: ### Step 1: Understand the Balmer series The Balmer series corresponds to transitions of electrons in a hydrogen-like atom from higher energy levels (n ≥ 2) to the n = 2 level. The third line in the Balmer series corresponds to a transition from n = 5 to n = 2. ### Step 2: Calculate the energy of the photon emitted The energy of a photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] where: - \( h \) is Planck's constant (\( 4.135667696 \times 10^{-15} \) eV·s), - \( c \) is the speed of light (\( 3 \times 10^8 \) m/s), - \( \lambda \) is the wavelength in meters. Convert the wavelength from nm to meters: \[ \lambda = 108.5 \, \text{nm} = 108.5 \times 10^{-9} \, \text{m} \] Now, substituting the values: \[ E = \frac{(4.135667696 \times 10^{-15} \, \text{eV·s})(3 \times 10^8 \, \text{m/s})}{108.5 \times 10^{-9} \, \text{m}} \] Calculating this gives: \[ E \approx 11.4 \, \text{eV} \] ### Step 3: Relate the energy to the binding energy The energy of the photon corresponds to the difference in energy levels: \[ E = E_2 - E_5 \] Using the formula for the energy levels of a hydrogen-like atom: \[ E_n = -\frac{Z^2 \cdot 13.6 \, \text{eV}}{n^2} \] where \( Z \) is the atomic number. For the transition from n = 5 to n = 2: \[ E = \left(-\frac{Z^2 \cdot 13.6}{2^2}\right) - \left(-\frac{Z^2 \cdot 13.6}{5^2}\right) \] \[ E = Z^2 \cdot 13.6 \left(\frac{1}{4} - \frac{1}{25}\right) \] ### Step 4: Simplify the expression Calculating the fractions: \[ \frac{1}{4} = \frac{25}{100} \] \[ \frac{1}{25} = \frac{4}{100} \] Thus, \[ \frac{1}{4} - \frac{1}{25} = \frac{25 - 4}{100} = \frac{21}{100} \] Now substituting this back into the energy equation: \[ E = Z^2 \cdot 13.6 \cdot \frac{21}{100} \] ### Step 5: Solve for the binding energy We know \( E \approx 11.4 \, \text{eV} \): \[ 11.4 = Z^2 \cdot 13.6 \cdot \frac{21}{100} \] Rearranging gives: \[ Z^2 = \frac{11.4 \cdot 100}{13.6 \cdot 21} \] Calculating \( Z^2 \): \[ Z^2 \approx \frac{1140}{285.6} \approx 4 \] Thus, \( Z \approx 2 \). ### Step 6: Calculate the binding energy Now we can find the binding energy: \[ \text{Binding Energy} = 13.6 Z^2 \] Substituting \( Z = 2 \): \[ \text{Binding Energy} = 13.6 \cdot 2^2 = 13.6 \cdot 4 = 54.4 \, \text{eV} \] ### Final Answer The binding energy of the electron in the ground state of the hydrogen-like atom is approximately **54.4 eV**.

To find the binding energy of an electron in the ground state of a hydrogen-like atom, given that the third Balmer line has a wavelength of 108.5 nm, we can follow these steps: ### Step 1: Understand the Balmer series The Balmer series corresponds to transitions of electrons in a hydrogen-like atom from higher energy levels (n ≥ 2) to the n = 2 level. The third line in the Balmer series corresponds to a transition from n = 5 to n = 2. ### Step 2: Calculate the energy of the photon emitted The energy of a photon can be calculated using the formula: \[ E = \frac{hc}{\lambda} \] ...
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DC PANDEY ENGLISH-MODERN PHYSICS - 1-Level 1 Objective
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