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Which one of the following graphs best represents the ways in which the total power P radiated by a black body depends upon the thermodynamic temperature T of the body?

A

B

C

D

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The correct Answer is:
To solve the question of how the total power \( P \) radiated by a black body depends on the thermodynamic temperature \( T \), we can follow these steps: ### Step 1: Understand Stefan-Boltzmann Law According to the Stefan-Boltzmann Law, the total power \( P \) radiated by a black body is directly proportional to the fourth power of its absolute temperature \( T \). This can be mathematically expressed as: \[ P = \sigma A T^4 \] where \( \sigma \) is the Stefan-Boltzmann constant and \( A \) is the surface area of the body. ### Step 2: Analyze the Relationship From the equation \( P = \sigma A T^4 \), we can see that as the temperature \( T \) increases, the power \( P \) increases with the fourth power of \( T \). This indicates a non-linear relationship, specifically a polynomial relationship of degree 4. ### Step 3: Identify the Graph Type Since the relationship is \( P \propto T^4 \), the graph of \( P \) versus \( T \) will be a curve that starts at the origin (0,0) and rises steeply as \( T \) increases. This is characteristic of a parabolic curve. ### Step 4: Select the Correct Option Among the options provided, we need to identify which graph represents a fourth-degree polynomial relationship. The correct graph will show a steep increase in power as temperature increases, confirming that it is a parabolic curve. ### Conclusion Based on the analysis, the graph that best represents the relationship between the total power \( P \) radiated by a black body and the thermodynamic temperature \( T \) is the one that shows a parabolic curve, which corresponds to option C.

To solve the question of how the total power \( P \) radiated by a black body depends on the thermodynamic temperature \( T \), we can follow these steps: ### Step 1: Understand Stefan-Boltzmann Law According to the Stefan-Boltzmann Law, the total power \( P \) radiated by a black body is directly proportional to the fourth power of its absolute temperature \( T \). This can be mathematically expressed as: \[ P = \sigma A T^4 \] where \( \sigma \) is the Stefan-Boltzmann constant and \( A \) is the surface area of the body. ...
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