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The thermal radiation emitted by a body ...

The thermal radiation emitted by a body is proportional to `T^(n)` where T is its absolute temperature. The value of n is exactly 4 for

A

a blackbody

B

all bodies

C

bodies painted black only

D

polished bodies only.

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To solve the question, we need to analyze the relationship between thermal radiation and temperature as described by Stefan-Boltzmann's law. ### Step-by-Step Solution: 1. **Understanding the Relationship**: The thermal radiation emitted by a body is proportional to \( T^n \), where \( T \) is the absolute temperature. We need to determine the value of \( n \) for different types of bodies. 2. **Stefan-Boltzmann Law**: According to Stefan-Boltzmann's law, the total energy radiated per unit surface area of a black body is given by the equation: \[ U = \epsilon \sigma A T^4 \] where: - \( U \) is the total energy radiated, - \( \epsilon \) is the emissivity of the body (which varies for different materials), - \( \sigma \) is the Stefan-Boltzmann constant, - \( A \) is the surface area, - \( T \) is the absolute temperature. 3. **Identifying the Black Body**: A black body is defined as an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. For a perfect black body, the emissivity \( \epsilon = 1 \). 4. **Value of n**: From the equation, we can see that the thermal radiation emitted by a perfect black body is proportional to \( T^4 \) (since \( \epsilon = 1 \)). Therefore, for a black body, the value of \( n \) is exactly 4. 5. **Analyzing the Options**: - **a) Black body**: Correct, as we established that \( n = 4 \) for a black body. - **b) All bodies**: This is misleading; while the Stefan-Boltzmann law applies to all bodies, the value of \( n \) is specifically 4 for black bodies. - **c) Bodies painted black only**: This does not guarantee \( n = 4 \) as the emissivity may vary. - **d) Polished bodies only**: Polished bodies typically have low emissivity, hence \( n \) would not be 4. 6. **Conclusion**: The value of \( n \) is exactly 4 for a black body. ### Final Answer: The value of \( n \) is exactly 4 for a **black body**. ---

To solve the question, we need to analyze the relationship between thermal radiation and temperature as described by Stefan-Boltzmann's law. ### Step-by-Step Solution: 1. **Understanding the Relationship**: The thermal radiation emitted by a body is proportional to \( T^n \), where \( T \) is the absolute temperature. We need to determine the value of \( n \) for different types of bodies. 2. **Stefan-Boltzmann Law**: ...
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