For the AC circuit shown in the figure, \(R = 100\, \text{k}\Omega\) and \(C = 10\, \text{pF}\), the phase difference between \(V_{in}\) and \(V_{out}\) is \(90^\circ\) at the input signal frequency of ............. kHz. (Round off to 2 decimal places) 
Step 1: Condition for phase difference.
For an RC circuit, the phase difference between \(V_{in}\) and \(V_{out}\) is \(90^\circ\) when:
\[
\omega R C = 1
\]
Step 2: Substitute given values.
\[
R = 100 \times 10^3\, \Omega, C = 10 \times 10^{-12}\, \text{F}
\]
\[
\omega = \frac{1}{R C} = \frac{1}{(100 \times 10^3)(10 \times 10^{-12})} = 10^6\, \text{rad/s}
\]
Step 3: Find frequency.
\[
f = \frac{\omega}{2\pi} = \frac{10^6}{2\pi} = 1.59 \times 10^5\, \text{Hz} = 159.15\, \text{kHz}
\]
Step 4: Conclusion.
Hence, the input frequency for a \(90^\circ\) phase difference is \(159.15\, \text{kHz}\).




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.)