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When photones of energy 4.0 eV fall on t...

When photones of energy 4.0 eV fall on the surface of a metal A, the ejected photoelectrons have maximum kinetic energy `T_(A)` ( in eV) and a de-Broglie wavelength `lambda_(A)`. When the same photons fall on the surface of another metal B, the maximum kinetic energy of ejected photoelectrons is `T_(B) = T_(A) -1.5eV`. If the de-Broglie wavelength of these photoelectrons is `lambda_(B) =2 lambda _(A)`, then the work function of metal B is

A

2eV

B

3eV

C

2.5 eV

D

3.5 eV

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To find the work function of metal B, we will follow these steps: ### Step 1: Understand the given information We know that: - The energy of the incident photons, \( E = 4.0 \, \text{eV} \). - The maximum kinetic energy of photoelectrons from metal A is \( T_A \). - The maximum kinetic energy of photoelectrons from metal B is \( T_B = T_A - 1.5 \, \text{eV} \). - The de-Broglie wavelength of photoelectrons from metal B is \( \lambda_B = 2 \lambda_A \). ### Step 2: Use the de-Broglie wavelength formula The de-Broglie wavelength \( \lambda \) of a particle is given by: \[ \lambda = \frac{h}{\sqrt{2mT}} \] Where: - \( h \) is Planck's constant, - \( m \) is the mass of the electron, - \( T \) is the kinetic energy. For metal A, we have: \[ \lambda_A = \frac{h}{\sqrt{2mT_A}} \] For metal B, we have: \[ \lambda_B = \frac{h}{\sqrt{2mT_B}} \] ### Step 3: Relate the wavelengths Given that \( \lambda_B = 2 \lambda_A \): \[ \frac{h}{\sqrt{2mT_B}} = 2 \cdot \frac{h}{\sqrt{2mT_A}} \] ### Step 4: Simplify the equation Cancel \( h \) and \( \sqrt{2m} \) from both sides: \[ \frac{1}{\sqrt{T_B}} = \frac{2}{\sqrt{T_A}} \] ### Step 5: Square both sides Squaring both sides gives: \[ \frac{1}{T_B} = \frac{4}{T_A} \] This implies: \[ T_A = 4T_B \] ### Step 6: Substitute the expression for \( T_B \) From the earlier relation \( T_B = T_A - 1.5 \, \text{eV} \), we substitute \( T_A \): \[ T_B = 4T_B - 1.5 \] ### Step 7: Rearranging the equation Rearranging gives: \[ 1.5 = 4T_B - T_B \] \[ 1.5 = 3T_B \] ### Step 8: Solve for \( T_B \) Thus, \[ T_B = \frac{1.5}{3} = 0.5 \, \text{eV} \] ### Step 9: Use Einstein's photoelectric equation According to Einstein's photoelectric equation: \[ T_B = E - \phi_B \] Where \( \phi_B \) is the work function of metal B. Substituting the known values: \[ 0.5 = 4 - \phi_B \] ### Step 10: Solve for \( \phi_B \) Rearranging gives: \[ \phi_B = 4 - 0.5 = 3.5 \, \text{eV} \] ### Final Answer The work function of metal B is \( \phi_B = 3.5 \, \text{eV} \). ---
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