Step 1: Using De Moivre's theorem.
According to De Moivre's theorem:
\[
(\cos \theta + i \sin \theta)^n = \cos n\theta + i \sin n\theta
\]
Step 2: Expand using binomial theorem.
\[
(\cos \theta + i \sin \theta)^n = \sum_{k=0}^{n} \binom{n}{k} (\cos \theta)^{n-k} (i \sin \theta)^k
\]
Step 3: Separate real and imaginary parts.
- Real part gives \(\cos n\theta = \cos^n \theta - \binom{n}{2} \cos^{n-2}\theta \sin^2\theta + \binom{n}{4} \cos^{n-4}\theta \sin^4\theta - \dots\)
- Imaginary part gives \(\sin n\theta = \binom{n}{1} \cos^{n-1}\theta \sin\theta - \binom{n}{3} \cos^{n-3}\theta \sin^3\theta + \dots\)
Step 4: Conclusion.
Hence, option (A) correctly represents the real part, which gives the expression for \(\cos n\theta.\)

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.)