Step 1: Recall Green's second identity.
Green's second identity relates two scalar functions \(\psi\) and \(\phi\) over a volume \(V\) and its bounding surface \(S\):
\[
\int_V (\psi \nabla^2 \phi - \phi \nabla^2 \psi) dV = \oint_S \left(\psi \frac{\partial \phi}{\partial n} - \phi \frac{\partial \psi}{\partial n}\right) dS
\]
This is a standard result derived using the divergence theorem.
Step 2: Check each option.
- (A) represents the divergence theorem, but lacks \(\nabla \psi\) terms, hence incomplete in this context.
- (B) matches exactly with Green's second identity — correct.
- (C) has a sign error — the plus sign makes it incorrect.
- (D) confuses Stokes' theorem: it should relate a line integral of \(\vec{u}\) around \(C\) to \((\nabla \times \vec{u})\) over \(S\), but the expression given involves \(\phi\), hence incorrect.
Step 3: Conclusion.
Thus, only option (B) is correct.

At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)