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If temperature of IBB is decrease by T t...

If temperature of IBB is decrease by T to T/2 than worked out percentage loss in emissive rate

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To solve the problem of finding the percentage loss in emissive rate when the temperature decreases from \( T \) to \( \frac{T}{2} \), we can follow these steps: ### Step 1: Understand the relationship between emissive power and temperature According to Stefan-Boltzmann Law, the emissive power \( E \) of a body is proportional to the fourth power of its absolute temperature \( T \): \[ E \propto T^4 \] This means that if we know the temperature, we can find the emissive power. ### Step 2: Calculate the initial emissive power Let the initial temperature be \( T \). The initial emissive power \( E \) can be expressed as: \[ E = k T^4 \] where \( k \) is a proportionality constant. ### Step 3: Calculate the emissive power at the new temperature When the temperature decreases to \( \frac{T}{2} \), the new emissive power \( E' \) can be expressed as: \[ E' = k \left(\frac{T}{2}\right)^4 \] Calculating this gives: \[ E' = k \frac{T^4}{16} \] ### Step 4: Find the percentage loss in emissive power The percentage loss in emissive power can be calculated using the formula: \[ \text{Percentage Loss} = \left( \frac{E - E'}{E} \right) \times 100 \] Substituting the values of \( E \) and \( E' \): \[ \text{Percentage Loss} = \left( \frac{E - \frac{E}{16}}{E} \right) \times 100 \] This simplifies to: \[ \text{Percentage Loss} = \left( \frac{1 - \frac{1}{16}}{1} \right) \times 100 \] Calculating this gives: \[ \text{Percentage Loss} = \left( \frac{15}{16} \right) \times 100 = 93.75\% \] ### Final Answer Thus, the percentage loss in emissive rate when the temperature decreases from \( T \) to \( \frac{T}{2} \) is approximately \( 93.75\% \). ---

To solve the problem of finding the percentage loss in emissive rate when the temperature decreases from \( T \) to \( \frac{T}{2} \), we can follow these steps: ### Step 1: Understand the relationship between emissive power and temperature According to Stefan-Boltzmann Law, the emissive power \( E \) of a body is proportional to the fourth power of its absolute temperature \( T \): \[ E \propto T^4 \] This means that if we know the temperature, we can find the emissive power. ...
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