JEE Challenger
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Ratio of Change in De Broglie Wavelength to Incident Wavelength

A photosensitive material with work function ϕ0\phi_0 is exposed to monochromatic light of wavelength λ\lambda (λ<hcϕ0)\left(\lambda < \frac{hc}{\phi_0}\right). The fastest emitted photoelectron has a de Broglie wavelength denoted by λd\lambda_d. A small variation in incident light wavelength by Δλ\Delta \lambda causes a corresponding change Δλd\Delta \lambda_d in λd\lambda_d. Determine the expression to which the ratio Δλd/Δλ\Delta \lambda_d / \Delta \lambda is proportional.

Options

A

λd/λ\lambda_d/\lambda

B

λd2/λ2\lambda_d^2/\lambda^2

C

λd3/λ\lambda_d^3/\lambda

D

λd3/λ2\lambda_d^3/\lambda^2

Correct

Step-by-Step Solution

To find the relation for the ratio ∣ΔλdΔλ∣\left| \frac{\Delta \lambda_d}{\Delta \lambda} \right|, we apply Einstein's photoelectric equation and the de Broglie wavelength formula.

According to Einstein's photoelectric equation, the maximum kinetic energy Kmax⁡K_{\max} of an emitted photoelectron is given by: Kmax⁡=hcλ−ϕ0K_{\max} = \frac{hc}{\lambda} - \phi_0

The de Broglie wavelength λd\lambda_d of the fastest emitted photoelectron is related to its maximum kinetic energy Kmax⁡K_{\max} by: λd=hpmax⁡=h2mKmax⁡\lambda_d = \frac{h}{p_{\max}} = \frac{h}{\sqrt{2m K_{\max}}}

Squaring both sides and expressing λd\lambda_d in terms of λ\lambda: λd2=h22m(hcλ−ϕ0)\lambda_d^2 = \frac{h^2}{2m \left(\frac{hc}{\lambda} - \phi_0\right)}

Taking the reciprocal of both sides: λd−2=2mh2(hcλ−ϕ0)\lambda_d^{-2} = \frac{2m}{h^2} \left(\frac{hc}{\lambda} - \phi_0\right)

To find the relationship between small changes Δλd\Delta \lambda_d and Δλ\Delta \lambda, we differentiate both sides with respect to λ\lambda: −2λd−3dλddλ=2mh2(−hcλ2)-2 \lambda_d^{-3} \frac{d\lambda_d}{d\lambda} = \frac{2m}{h^2} \left(-\frac{hc}{\lambda^2}\right)

Simplifying the equation: 1λd3dλddλ=mchλ2\frac{1}{\lambda_d^3} \frac{d\lambda_d}{d\lambda} = \frac{mc}{h \lambda^2}

Rearranging for the ratio of the differentials: dλddλ=(mch)λd3λ2\frac{d\lambda_d}{d\lambda} = \left(\frac{mc}{h}\right) \frac{\lambda_d^3}{\lambda^2}

For small variations Δλd\Delta \lambda_d and Δλ\Delta \lambda: ∣ΔλdΔλ∣=(mch)λd3λ2\left| \frac{\Delta \lambda_d}{\Delta \lambda} \right| = \left(\frac{mc}{h}\right) \frac{\lambda_d^3}{\lambda^2}

Since mm, cc, and hh are physical constants, we conclude that: ΔλdΔλ∝λd3λ2\frac{\Delta \lambda_d}{\Delta \lambda} \propto \frac{\lambda_d^3}{\lambda^2}

Correct Answer: D (λd3/λ2\lambda_d^3/\lambda^2)