The line integral of the electric field along a path is related to the change in electric potential \( V \) between the start and end points of the path. Mathematically:
\[ \oint_{\mathcal{C}} \mathbf{E} \cdot d\mathbf{l} = V_C - V_M \]
where:
The electric potential due to a point charge \( q \) at a distance \( r \) is given by:
\[ V = \frac{kq}{r} \]
where \( k \) is Coulombβs constant.
Both points \( C \) and \( M \) are at the same distance \( 2d \) from the charges \( Q \) (at A) and \( 2Q \) (at B), since \( MCL \) is a semicircle of radius \( 2d \). Therefore, the electric potential at both \( C \) and \( M \) is the same.
For any point on the semicircle:
\[ V = \frac{kQ}{2d} + \frac{k(2Q)}{2d} = \frac{3kQ}{2d} \]
Thus,
\[ V_C = V_M \]
Since the potentials at points \( C \) and \( M \) are equal (\( V_C = V_M \)):
\[ \oint_{\mathcal{C}} \mathbf{E} \cdot d\mathbf{l} = V_C - V_M = 0 \]
The line integral of the electric field along the given path is zero.
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/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)