For imperfect-gas calculations, one sometimes employs the Sutherland potential [u(r)= begin{cases}infty & text { for } r
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For imperfect-gas calculations, one sometimes employs the Sutherland potential
\[u(r)= \begin{cases}\infty & \text { for } r
Using this potential, determine the second virial coefficient of a classical gas. Also determine first-order corrections to the ideal-gas law and to the various thermodynamic properties of the system.
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