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=U/V propT^4` and pressure `P=1/3(U/V)`. If the shell now undergoes an adiabatic expansion the relation between T and R is :

Options

A. `Tprop(1)/(R)`
B. `Tprop(1)/(R^(3))`
C. `Tprope^(-R)`
D. `Tprope^(-3R)`