The following diagram shows the kinetic energy of the ejected photoelectrons against the energy of incident radiation for two metal surfaces M1 and M2. If the energy of the incident radiation on M1 is equal to the work function of M2, the de Broglie wavelength of the ejected photoelectron is nm [Given: Mass of electron = 9.11x10−31 kg; Planck’s constant = 6.62x10−34 J s; 1 eV=1.6x10−19 J.] (round off to two decimal places)
To determine the de Broglie wavelength of the ejected photoelectron, we need to follow these steps:
Understanding the Problem: The diagram indicates that the threshold energy (work function) for M1 is 2.3 eV and for M2 is 2.9 eV. Given: Energy of incident radiation on M1 equals the work function of M2, which is 2.9 eV.
Calculate Kinetic Energy: The kinetic energy (K.E.) of the ejected electron from M1 is calculated as: K.E. = Energy of incident radiation - Work function of M1 K.E. = 2.9 eV - 2.3 eV = 0.6 eV Convert K.E. to joules: 0.6 eV = 0.6 x 1.6 x 10-19 J = 9.6 x 10-20 J
Calculate Velocity of Electron: Use the kinetic energy formula: \( \text{K.E.} = \frac{1}{2}mv^2 \) Solving for velocity (v), we have: \( v = \sqrt{\frac{2 \times \text{K.E.}}{m}} \) \( v = \sqrt{\frac{2 \times 9.6 \times 10^{-20}}{9.11 \times 10^{-31}}} \) \( v \approx 4.6 \times 10^5 \, \text{m/s} \)
Calculate de Broglie Wavelength: The de Broglie wavelength (λ) is given by: \( λ = \frac{h}{mv} \) where \( h = 6.62 \times 10^{-34} \, \text{J s} \) \( λ = \frac{6.62 \times 10^{-34}}{9.11 \times 10^{-31} \times 4.6 \times 10^5} \) \( λ \approx 1.58 \times 10^{-9} \, \text{m} \)
Verification and Conclusion: Convert to nanometers: \( λ \approx 1.58 \, \text{nm} \)
De Broglie Wavelength of the ejected photoelectron: 1.58 nm