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A black body emits radiation at the rate...

A black body emits radiation at the rate P when its temperature is T. At this temperature the wavelength at which the radiation has maximum intensity is `lamda_0`, If at another temperature `T'` the power radiated is `P'` and wavelength at maximum intensity is `(lamda_0)/(2)` then

A

`P' T' =32PT`

B

`P' T'=16PT`

C

`P'T' =8PT`

D

`P'T'=4PT`

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The correct Answer is:
To solve the problem, we will use the concepts of Stefan-Boltzmann law and Wien's displacement law. Here’s a step-by-step breakdown of the solution: ### Step 1: Understand the given information We have a black body that emits radiation at a power \( P \) when its temperature is \( T \). The wavelength at which the radiation has maximum intensity is \( \lambda_0 \). At a new temperature \( T' \), the power radiated is \( P' \) and the wavelength at maximum intensity is \( \frac{\lambda_0}{2} \). ### Step 2: Apply Stefan-Boltzmann Law According to the Stefan-Boltzmann law, the power radiated by a black body is given by: \[ P = e \sigma A T^4 \] For a black body, emissivity \( e = 1 \), so: \[ P = \sigma A T^4 \] For the new temperature \( T' \): \[ P' = \sigma A (T')^4 \] ### Step 3: Apply Wien's Displacement Law Wien's displacement law states that the wavelength of maximum intensity (\( \lambda \)) is inversely proportional to the absolute temperature (\( T \)): \[ \lambda = \frac{B}{T} \] where \( B \) is Wien's constant. For the original temperature \( T \): \[ \lambda_0 = \frac{B}{T} \] For the new temperature \( T' \) where the maximum wavelength is \( \frac{\lambda_0}{2} \): \[ \frac{\lambda_0}{2} = \frac{B}{T'} \] ### Step 4: Relate the temperatures From the equation above, we can express \( T' \): \[ T' = \frac{B}{\frac{\lambda_0}{2}} = \frac{2B}{\lambda_0} \] Now, substituting \( \lambda_0 = \frac{B}{T} \) into this equation gives: \[ T' = \frac{2B}{\frac{B}{T}} = 2T \] ### Step 5: Substitute \( T' \) into the power equation Now we substitute \( T' = 2T \) into the power equation: \[ P' = \sigma A (T')^4 = \sigma A (2T)^4 = \sigma A \cdot 16T^4 = 16\sigma A T^4 \] Thus, we can relate \( P' \) to \( P \): \[ P' = 16P \] ### Step 6: Relate \( P' \) and \( T' \) Now, using the relationship we obtained: \[ P' T' = 16P \cdot 2T = 32PT \] ### Conclusion Thus, the relationship we derived is: \[ P' T' = 32PT \] This means that the correct answer is option 1. ---

To solve the problem, we will use the concepts of Stefan-Boltzmann law and Wien's displacement law. Here’s a step-by-step breakdown of the solution: ### Step 1: Understand the given information We have a black body that emits radiation at a power \( P \) when its temperature is \( T \). The wavelength at which the radiation has maximum intensity is \( \lambda_0 \). At a new temperature \( T' \), the power radiated is \( P' \) and the wavelength at maximum intensity is \( \frac{\lambda_0}{2} \). ### Step 2: Apply Stefan-Boltzmann Law According to the Stefan-Boltzmann law, the power radiated by a black body is given by: \[ ...
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