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     EduGorilla 
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    Consider a spherical shell of radius R at temperature T. The black body radiation inside it can be considered as an ideal gas of photons with internal energy per unit volume u =  T4 and pressure p =  If the shell now undergoes an adiabatic expansion, the relation between T and R is

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    1. T e–R
    2. T e–3R
    3. T
    4. T
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