A white Gaussian noise \(w(t)\) with zero mean and power spectral density \(\frac{N_0}{2}\), when applied to a first-order RC low-pass filter produces an output \(n(t)\). At a particular time \(t = t_k\), the variance of the random variable \(n(t_k)\) is:
Show Hint
To analyze noise in RC filters, calculate the output variance by integrating the power spectral density over all frequencies. Remember to use substitution and standard integral results for efficiency.
Step 1: Derive the transfer function for the RC low-pass filter.
The transfer function of a first-order RC low-pass filter is given by:
\[
H(f) = \frac{1}{1 + j2\pi fRC}.
\]
Step 2: Connect the power spectral density and variance.
The output power spectral density \(S_{n}(f)\) is related to the input \(S_{w}(f)\) as:
\[
S_{n}(f) = |H(f)|^2 S_{w}(f).
\]
For white Gaussian noise, \(S_{w}(f) = \frac{N_0}{2}\). The magnitude squared of the transfer function becomes:
\[
|H(f)|^2 = \frac{1}{1 + (2\pi fRC)^2}.
\]
Step 3: Compute the variance of the output.
The variance of the output noise \(n(t_k)\) is the integral of \(S_{n}(f)\) over all frequencies:
\[
{Variance} = \int_{-\infty}^\infty S_{n}(f) df = \int_{-\infty}^\infty \frac{\frac{N_0}{2}}{1 + (2\pi fRC)^2} df.
\]
Using the substitution \(\omega = 2\pi f\), the integral becomes:
\[
{Variance} = \frac{N_0}{2} \int_{-\infty}^\infty \frac{1}{1 + (\omega RC)^2} \frac{d\omega}{2\pi}.
\]
The standard integral result for \(\frac{1}{1 + x^2}\) is:
\[
\int_{-\infty}^\infty \frac{1}{1 + (\omega RC)^2} d\omega = \frac{\pi}{RC}.
\]
Substituting this result, the variance is:
\[
{Variance} = \frac{N_0}{2} \cdot \frac{\pi}{RC} \cdot \frac{1}{2\pi} = \frac{N_0}{4RC}.
\]
Final Answer:
\[\boxed{{(1) } \frac{N_0}{4RC}}\]