Skip to main content

ESD of an energy signal (ideal BPF example)

Short answer

Energy spectral density Ψ_g(f) = |G(f)|² (J/Hz) describes energy distribution of an energy signal. Derived by passing g(t) through an ideal narrow BPF of bandwidth Δf at f₀; output energy ≈ 2|G(f₀)|²Δf, giving energy per unit bandwidth as |G(f)|². Properties: area equals total energy, real and non-negative, even for real signals, no phase information, Fourier pair with energy autocorrelation, and Ψ_y(f)=|H(f)|²Ψ_x(f) through LTI systems.

Derive a general expression for an energy spectral density of an energy signal with an example of an ideal BPF. Mention basic properties of the energy spectral density.

The energy spectral density (ESD) Ψg(f)\Psi_g(f) of an energy signal tells how its energy is distributed with frequency; Ψg(f) df\Psi_g(f)\,df is the energy in a small band dfdf.

Derivation using an ideal BPF

Let g(t)g(t) be an energy signal with Fourier transform G(f)G(f) and energy E=∫∣g(t)∣2dtE=\int\lvert g(t)\rvert^2dt. To find how much energy lies near a frequency f0f_0, pass g(t)g(t) through an ideal narrow band-pass filter centred at f0f_0 with bandwidth Δf\Delta f:

H(f)={1,f0−Δf2≤∣f∣≤f0+Δf20,otherwiseH(f)=\begin{cases}1, & f_0-\frac{\Delta f}{2}\le\lvert f\rvert\le f_0+\frac{\Delta f}{2}\\0, & \text{otherwise}\end{cases}
              |H(f)|
     +--+     |     +--+
     |  |     |     |  |  <- width df each
 ----+--+-----+-----+--+----> f
       -f0    0       f0

Step 1 – output spectrum: Y(f)=H(f)G(f)Y(f)=H(f)G(f).

Step 2 – output energy by Rayleigh's theorem:

Ey=∫−∞∞∣Y(f)∣2df=∫−∞∞∣H(f)∣2∣G(f)∣2dfE_y=\int_{-\infty}^{\infty}\lvert Y(f)\rvert^2df=\int_{-\infty}^{\infty}\lvert H(f)\rvert^2\lvert G(f)\rvert^2df

Step 3 – narrow filter: ∣H(f)∣2=1\lvert H(f)\rvert^2=1 only in the two narrow bands. If Δf\Delta f is small, ∣G(f)∣2\lvert G(f)\rvert^2 is nearly constant there, and for a real signal ∣G(−f0)∣=∣G(f0)∣\lvert G(-f_0)\rvert=\lvert G(f_0)\rvert:

Ey≈∣G(f0)∣2Δf+∣G(−f0)∣2Δf=2∣G(f0)∣2ΔfE_y\approx\lvert G(f_0)\rvert^2\Delta f+\lvert G(-f_0)\rvert^2\Delta f=2\lvert G(f_0)\rvert^2\Delta f

Step 4 – interpret: the energy in the band of total width 2Δf2\Delta f (positive plus negative frequencies) is 2∣G(f0)∣2Δf2\lvert G(f_0)\rvert^2\Delta f. So the energy per unit bandwidth at f0f_0 is

Ψg(f)=∣G(f)∣2(J/Hz)\Psi_g(f)=\lvert G(f)\rvert^2\quad(\text{J/Hz})

Summing over all bands gives the total energy:

E=∫−∞∞Ψg(f) df=∫−∞∞∣G(f)∣2dfE=\int_{-\infty}^{\infty}\Psi_g(f)\,df=\int_{-\infty}^{\infty}\lvert G(f)\rvert^2df

Example: for g(t)=A rect(t/T)g(t)=A\,\text{rect}(t/T), G(f)=AT sinc(fT)G(f)=AT\,\text{sinc}(fT) and Ψg(f)=A2T2sinc2(fT)\Psi_g(f)=A^2T^2\text{sinc}^2(fT); its area is A2TA^2T, equal to the time-domain energy.

Basic properties of ESD

  1. Area gives energy: ∫Ψg(f)df=E\int\Psi_g(f)df=E.
  2. Real and non-negative: Ψg(f)=∣G(f)∣2≥0\Psi_g(f)=\lvert G(f)\rvert^2\ge0.
  3. Even function for real g(t)g(t): Ψg(−f)=Ψg(f)\Psi_g(-f)=\Psi_g(f).
  4. No phase information: time-shifted signals have the same ESD.
  5. Wiener–Khinchin pair: Ψg(f)\Psi_g(f) is the Fourier transform of the energy autocorrelation Rg(τ)=∫g(t)g∗(t−τ)dtR_g(\tau)=\int g(t)g^*(t-\tau)dt.
  6. Through an LTI system: Ψy(f)=∣H(f)∣2Ψx(f)\Psi_y(f)=\lvert H(f)\rvert^2\Psi_x(f).

✓ Answer checked by Claude Opus 5.5 (high effort)

All Communication Systems chapter 1 questions →