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 $E = \frac{U}{V} \propto T^4$ and pressure $P = \frac{1}{3} \left( \frac{U}{V} \right)$. If the shell now undergoes an adiabatic expansion,the relation between $T$ and $R$ is:

  • A
    $T \propto e^{-3R}$
  • B
    $T \propto \frac{1}{R}$
  • C
    $T \propto \frac{1}{R^3}$
  • D
    $T \propto e^{-R}$

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