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प्रश्न
Answer in brief:
What is a perfect blackbody? How can it be realized in practice?
उत्तर
- A perfect blackbody, also known as a blackbody, is a body that absorbs all of the radiant energy that is incident on it.
- Fery created a spherical blackbody, which consists of a double-walled hollow sphere having a tiny hole or aperture, through which radiant heat can enter, as shown in Figure. The sphere's inside wall is blackened with lampblack, while the outside is silver plated. To reduce heat loss through conduction and convection, the space between the two walls is evacuated.
- Any radiation entering the sphere through the aperture is reflected several times, with around 97% of it being absorbed by the lampblack covering at each incidence.
- After a series of internal reflections, the radiation is almost fully absorbed. The probability of incident radiation escaping out is reduced by a conical projection on the inside wall opposite the opening.
Ferry’s blackbody
- When the sphere is placed in a bath of appropriate fused salts to maintain the desired temperature, the hole acts as a source of black-body radiation. The intensity and nature of the radiation are solely determined by the temperature of the walls.
- A blackbody has a coefficient of absorption of one by definition. As a result, its coefficients of reflection and transmission are both zero.
- The radiation emitted by a blackbody, known as blackbody radiation, covers the complete electromagnetic spectrum. As a result, a blackbody is also known as a full radiator.
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संबंधित प्रश्न
Show the graphical representation of radiant power of a black body per unit range of wavelength as a function of wavelength.
Draw a neat labeled diagram of Ferry’s black body.
Explain the construction and working of Ferry’s black body.
Compare the rates of emission of heat by a blackbody maintained at 627°C and at 127°C, if the black bodies are surrounded by an enclosure at 27°C. What would be the ratio of their rates of loss of heat?
Why is a conical projection in front of the hole i.n Fen-y's blackbody?
The energy spectrum of a black body exhibits a maximum around a wavelength '`lambda`'. The temperature of a black body is now changed such that the energy is maximum around a wavelength 3`lambda`/4. The power radiated by a black body will now increase by a factor of ______.
A black body has maximum wavelength `lambda_"m"` at temperature 2200 K. wavelength at temperature 3300 K will be ______.
For a perfectly black body, the graph is plotted between the frequency of the radiation with maximum intensity (vm) and the absolute temperature T. Out of the following, which is the correct graph?
A blackbody at 327 °C, when suspended in a black enclosure at 27 °C, loses heat at a certain rate. Find the temperature of the body at which its rate of loss of heat by radiation will be half of the above rate. Assume that the other conditions remain unchanged.
Draw a neat labelled diagram of Ferry’s perfectly black body.