Match the temperature of a black body given in List-I with an appropriate statement in List-II, and choose the correct option.
[Given: Wien's constant as m-K and V-m]
| List-I | List-II |
|---|---|
| (P) 2000 K | (1) The radiation at peak wavelength can lead to emission of photoelectrons from a metal of work function 4 eV |
| (Q) 3000 K | (2) The radiation at peak wavelength is visible to human eye. |
| (R) 5000 K | (3) The radiation at peak emission wavelength will result in the widest central maximum of a single slit diffraction. |
| (S) 10000 K | (4) The power emitted per unit area is 1/16 of that emitted by a blackbody at temperature 6000 K. |
| (5) The radiation at peak emission wavelength can be used to image human bones. |
- A
P 3, Q 5, R 2, S 3
- B
P 3, Q 2, R 4, S 1
- C
P 3, Q 4, R 2, S 1
- D
P 1, Q 2, R 5, S 3
Peak wavelengths from Wien's law. m-K.
(P) K nm (infrared, largest among the four). The longest wavelength produces the widest diffraction maximum since the half-angle scales as . Match (3).
(Q) K nm. The Stefan-Boltzmann law gives power per unit area , so . Match (4).
(R) K nm, which lies in the visible spectrum. Match (2).
(S) K nm. The corresponding photon energy is eV, which exceeds a eV work function and ejects photoelectrons. Match (1).
Mapping: P 3, Q 4, R 2, S 1. Answer: (C).