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Dual Nature of Radiation question

2022 · Shift 2 · Q52
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  5. /2022 · Shift 2 · Q52

Dual Nature of Radiation question

2022 · Shift 2 · Q52

JEE AdvancedPhysicsDual Nature of RadiationMCQ+3 / −1
When light of a given wavelength is incident on a metallic surface, the minimum potential needed to stop the emitted photoelectrons is 6.0 V6.0 \mathrm{~V}6.0 V. This potential drops to 0.6 V0.6 \mathrm{~V}0.6 V if another source with wavelength four times that of the first one and intensity half of the first one is used. What are the wavelength of the first source and the work function of the metal, respectively? [Take hce=1.24×10−6JmC−1\frac{h c}{e}=1.24 \times10^{-6} \mathrm{JmC}^{-1}ehc​=1.24×10−6JmC−1.]
  1. A
    1.72×10−7 m,1.20eV1.72 \times 10^{-7} \mathrm{~m}, 1.20 \mathrm{eV}1.72×10−7 m,1.20eV
  2. B
    1.72×10−7 m,5.60eV1.72 \times 10^{-7} \mathrm{~m}, 5.60 \mathrm{eV}1.72×10−7 m,5.60eV
  3. C
    3.78×10−7 m,5.60eV3.78 \times 10^{-7} \mathrm{~m}, 5.60 \mathrm{eV}3.78×10−7 m,5.60eV
  4. D
    3.78×10−7 m,1.20eV3.78 \times 10^{-7} \mathrm{~m}, 1.20 \mathrm{eV}3.78×10−7 m,1.20eV
View written solutionFree

Correct answer: A

Introduction

This problem involves the photoelectric effect. We will use Einstein's photoelectric equation, which relates the energy of incident photons, the work function of the metal, and the maximum kinetic energy of the emitted photoelectrons. The maximum kinetic energy is related to the stopping potential.

Einstein's Photoelectric Equation

The equation is given by: Kmax=hν−ΦK_{max} = h\nu - \PhiKmax​=hν−Φ where:

  • KmaxK_{max}Kmax​ is the maximum kinetic energy of the photoelectrons.
  • hν=hcλh\nu = \frac{hc}{\lambda}hν=λhc​ is the energy of the incident photon.
  • Φ\PhiΦ is the work function of the metal.

The maximum kinetic energy is also related to the stopping potential VsV_sVs​ by: Kmax=eVsK_{max} = e V_sKmax​=eVs​ where eee is the elementary charge.

Combining these, we get: eVs=hcλ−Φe V_s = \frac{hc}{\lambda} - \PhieVs​=λhc​−Φ Dividing the entire equation by eee, we can express all terms in units of electron-volts (eV) for energy, or volts (V) for potential. Let ΦeV\Phi_{eV}ΦeV​ be the work function in eV. The equation becomes: Vs=hceλ−Φe=hceλ−ΦeVV_s = \frac{hc}{e\lambda} - \frac{\Phi}{e} = \frac{hc}{e\lambda} - \Phi_{eV}Vs​=eλhc​−eΦ​=eλhc​−ΦeV​ We are given the value of the constant hce=1.24×10−6V⋅m\frac{hc}{e} = 1.24 \times 10^{-6} \mathrm{V} \cdot \mathrm{m}ehc​=1.24×10−6V⋅m.

Step 1: Formulate equations for the two given cases.

Case 1:

  • Wavelength of incident light = λ1=λ\lambda_1 = \lambdaλ1​=λ
  • Stopping potential = Vs1=6.0 VV_{s1} = 6.0 \mathrm{~V}Vs1​=6.0 V

Substituting these values into the photoelectric equation: 6.0=1.24×10−6λ−ΦeV⋯(1)6.0 = \frac{1.24 \times 10^{-6}}{\lambda} - \Phi_{eV} \quad \cdots (1)6.0=λ1.24×10−6​−ΦeV​⋯(1)

Case 2:

  • Wavelength of incident light = λ2=4λ\lambda_2 = 4\lambdaλ2​=4λ
  • Stopping potential = Vs2=0.6 VV_{s2} = 0.6 \mathrm{~V}Vs2​=0.6 V
  • The information about intensity being halved is irrelevant for calculating stopping potential, as stopping potential depends on the frequency (or wavelength) of incident light, not its intensity.

Substituting these values into the equation: 0.6=1.24×10−64λ−ΦeV⋯(2)0.6 = \frac{1.24 \times 10^{-6}}{4\lambda} - \Phi_{eV} \quad \cdots (2)0.6=4λ1.24×10−6​−ΦeV​⋯(2)

Step 2: Solve the system of two equations to find the wavelength λ\lambdaλ.

We have two linear equations with two unknowns, λ\lambdaλ and ΦeV\Phi_{eV}ΦeV​. We can eliminate ΦeV\Phi_{eV}ΦeV​ by subtracting equation (2) from equation (1). (6.0−0.6)=(1.24×10−6λ−ΦeV)−(1.24×10−64λ−ΦeV)(6.0 - 0.6) = \left( \frac{1.24 \times 10^{-6}}{\lambda} - \Phi_{eV} \right) - \left( \frac{1.24 \times 10^{-6}}{4\lambda} - \Phi_{eV} \right)(6.0−0.6)=(λ1.24×10−6​−ΦeV​)−(4λ1.24×10−6​−ΦeV​) 5.4=1.24×10−6λ−1.24×10−64λ5.4 = \frac{1.24 \times 10^{-6}}{\lambda} - \frac{1.24 \times 10^{-6}}{4\lambda}5.4=λ1.24×10−6​−4λ1.24×10−6​ 5.4=1.24×10−6λ(1−14)5.4 = \frac{1.24 \times 10^{-6}}{\lambda} \left( 1 - \frac{1}{4} \right)5.4=λ1.24×10−6​(1−41​) 5.4=1.24×10−6λ(34)5.4 = \frac{1.24 \times 10^{-6}}{\lambda} \left( \frac{3}{4} \right)5.4=λ1.24×10−6​(43​) Now, we solve for λ\lambdaλ: λ=1.24×10−6×35.4×4\lambda = \frac{1.24 \times 10^{-6} \times 3}{5.4 \times 4}λ=5.4×41.24×10−6×3​ λ=3.72×10−621.6\lambda = \frac{3.72 \times 10^{-6}}{21.6}λ=21.63.72×10−6​ λ≈0.1722×10−6 m\lambda \approx 0.1722 \times 10^{-6} \mathrm{~m}λ≈0.1722×10−6 m λ=1.72×10−7 m\lambda = 1.72 \times 10^{-7} \mathrm{~m}λ=1.72×10−7 m

Step 3: Solve for the work function ΦeV\Phi_{eV}ΦeV​.

We can substitute the value of λ\lambdaλ back into either equation (1) or (2). Let's use equation (1): 6.0=1.24×10−6λ−ΦeV6.0 = \frac{1.24 \times 10^{-6}}{\lambda} - \Phi_{eV}6.0=λ1.24×10−6​−ΦeV​ ΦeV=1.24×10−61.722×10−7−6.0\Phi_{eV} = \frac{1.24 \times 10^{-6}}{1.722 \times 10^{-7}} - 6.0ΦeV​=1.722×10−71.24×10−6​−6.0 ΦeV=1.240.1722−6.0\Phi_{eV} = \frac{1.24}{0.1722} - 6.0ΦeV​=0.17221.24​−6.0 ΦeV≈7.20−6.0\Phi_{eV} \approx 7.20 - 6.0ΦeV​≈7.20−6.0 ΦeV=1.20 eV\Phi_{eV} = 1.20 \mathrm{~eV}ΦeV​=1.20 eV

Conclusion

The wavelength of the first source is λ=1.72×10−7 m\lambda = 1.72 \times 10^{-7} \mathrm{~m}λ=1.72×10−7 m and the work function of the metal is Φ=1.20 eV\Phi = 1.20 \mathrm{~eV}Φ=1.20 eV.

Comparing our results with the given options:

  • A: 1.72×10−7 m,1.20eV1.72 \times 10^{-7} \mathrm{~m}, 1.20 \mathrm{eV}1.72×10−7 m,1.20eV
  • B: 1.72×10−7 m,5.60eV1.72 \times 10^{-7} \mathrm{~m}, 5.60 \mathrm{eV}1.72×10−7 m,5.60eV
  • C: 3.78×10−7 m,5.60eV3.78 \times 10^{-7} \mathrm{~m}, 5.60 \mathrm{eV}3.78×10−7 m,5.60eV
  • D: 3.78×10−7 m,1.20eV3.78 \times 10^{-7} \mathrm{~m}, 1.20 \mathrm{eV}3.78×10−7 m,1.20eV

Our calculated values match option A.

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