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# Analyse the experimental evidence gathered about black body radiation, including Wien’s Law related to Planck’s contribution to a changed model of light

**Black Body:**A hypothetical object that absorbs all incoming radiation.- A practical example of an item that resembles a black body is a small hole in a box with a black interior.

- When a black body becomes warmer than its surroundings, it becomes a perfect emitter.
**Black Body Radiation:**Electromagnetic radiation that is emitted by a black body.- The radiation emitted from a black body extends over all wavelengths of the electromagnetic spectrum.

- Classical theory predicted that the intensity of radiation would increase indefinitely as wavelengths
- However, experimental results showed that intensity peaked at a wavelength characteristic of the temperature of the black body.

- Moreover, it also showed the wavelength of peak intensity of radiation emitted by a black body decreases as the temperature of the body increases.
- This wavelength of peak intensity only depends on the temperature of the body.
- This relation is defined as Wien’s Law : , where
*b = 2.9 x 10*^{-3 }Km

– __Plank’s proposal of a new model__

- The contradiction between classical theory and experimental results was resolved by Max Planck.
- Planck proposed that radiant energy may be treated statistically as if it were exchanged in multiples of a certain discrete amount, or quanta.
- Each frequency of radiation has a characteristic quantum of energy.
- This is given by the equation:
*E = hf*- where:
- E = energy in joules (J)
- h = a constant, now known as Planck’s constant (6.63 x 10
^{-34}J s) - f = frequency in hertz (Hz)

- This assumption allowed Plank to reproduce the results obtained experimentally from theory.

Extract from *Physics Stage 6 Syllabus © 2017 *NSW Education Standards Authority (NESA)