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MHT CET 2024 (10 May, Shift 2) · Thermal Radiation: Black Body, Stefan & Wien

Thermal Radiation: Black Body, Stefan & Wien question from MHT CET 2024 (10 May, Shift 2)

Q69MHT CET 2024 · 10 MAY · SHIFT 2Medium

Thermal Radiation: Black Body, Stefan & Wien

The black discs x,yx, y and z have radii 1 m,2 m1\text{ m}, 2\text{ m} and 3 m respectively. The wavelengths corresponding to maximum intensity are 200 nm,300 nm200\text{ nm}, 300\text{ nm} and 400 nm respectively. The relation between emissive power Ex,EyE_x, E_y and EzE_z is

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Answer: (a)

  1. Power E∝R2T4∝R2λm4E \propto R^2 T^4 \propto \frac{R^2}{\lambda_m^4}.
  2. Taking λ\lambda in units of 100 nm: Ex∝124=0.0625E_x \propto \frac{1}{2^4} = 0.0625, Ey∝434=0.049E_y \propto \frac{4}{3^4} = 0.049, Ez∝944=0.035E_z \propto \frac{9}{4^4} = 0.035.
  3. So Ex>Ey>EzE_x > E_y > E_z, answer (a).
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