The flux of the curl of a vector field through a surface is given by:
\[ \Phi = \iint_S (\nabla \times \vec{F}) \cdot d\vec{A} \]
Using Stokes’ Theorem, this flux can be related to the circulation around the boundary of the surface, which in this case is a circular loop of radius 2 centered at the origin.
Since \( \vec{F}(x, y) \) is a vector field in the x-y plane, the curl of \( \vec{F} \) in the z-direction can be evaluated using the given components.
Upon solving for the flux, we find that the magnitude of the flux through the circular loop is:
\[ 2\pi \]
Thus, the correct answer is (B).
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.)