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SNR gain of non-coherent FM detector

Short answer

For non-coherent FM detection, noise after discriminator has parabolic PSD ∝ f². The SNR improvement SNR_o/SNR_i = 3β²(β+1) for a single-tone modulating signal with deviation ratio β, demonstrating noise reduction proportional to β².

Derive the expression for evaluation the gain parameter (SNR₀/SNRᵢ) of non-coherent FM detector.

A non-coherent FM detector (limiter + frequency discriminator) responds to the instantaneous frequency of the received signal; no local carrier is needed. The gain parameter SNRo/SNRi\text{SNR}_o/\text{SNR}_i is found assuming high carrier-to-noise ratio (above threshold).

FM signal and receiver. s(t)=Accos⁡[ωct+2πkf∫m(t)dt]s(t)=A_c\cos\left[\omega_ct+2\pi k_f\int m(t)dt\right], instantaneous frequency deviation kfm(t)k_fm(t). Receiver: BPF (BTB_T) → limiter → discriminator (output =12πdϕdt=\frac{1}{2\pi}\frac{d\phi}{dt}) → LPF (WW).

Noise in phasor form. Write the narrowband noise as n(t)=r(t)cos⁡[ωct+ψ(t)]n(t)=r(t)\cos[\omega_ct+\psi(t)]. At high carrier-to-noise ratio (Ac≫rA_c\gg r), the resultant phase is

θ(t)≈ϕ(t)+r(t)Acsin⁡[ψ(t)−ϕ(t)]\theta(t)\approx\phi(t)+\frac{r(t)}{A_c}\sin[\psi(t)-\phi(t)]
            r(t)
          .------>          resultant = carrier + noise
         /  ^               small noise phasor rotates
 Ac     /   | r sin(psi-phi) the carrier phasor slightly
 ------>----+

The noise term is statistically equivalent to ns(t)Ac\frac{n_s(t)}{A_c} (the phase ϕ\phi can be dropped for noise calculation). Discriminator output:

v(t)=12πdθdt=kfm(t)+12πAcdns(t)dtv(t)=\frac{1}{2\pi}\frac{d\theta}{dt}=k_fm(t)+\frac{1}{2\pi A_c}\frac{dn_s(t)}{dt}

Output signal power: So=kf2PS_o=k_f^2P.

Output noise power. nsn_s has PSD N0N_0 for ∣f∣≤BT/2\lvert f\rvert\le B_T/2. Differentiation multiplies the spectrum by j2πfj2\pi f, so the noise PSD at discriminator output is

Snd(f)=(2πf)2(2πAc)2N0=N0f2Ac2,∣f∣≤BT2S_{n_d}(f)=\frac{(2\pi f)^2}{(2\pi A_c)^2}N_0=\frac{N_0f^2}{A_c^2},\qquad \lvert f\rvert\le\frac{B_T}{2}

This parabolic noise spectrum is the key property of FM. After the LPF (∣f∣≤W\lvert f\rvert\le W):

No=∫−WWN0f2Ac2df=2N0W33Ac2N_o=\int_{-W}^{W}\frac{N_0f^2}{A_c^2}df=\frac{2N_0W^3}{3A_c^2}
 S(f) |\                   /|
      | \                 / |   parabolic noise
      |  \               /  |   after discriminator
      |   \.           ./   |   (only |f|<W kept)
      +----+-----+-----+----+--> f
          -W     0     W

Output SNR:

SNRo=kf2P2N0W3/3Ac2=3Ac2kf2P2N0W3\text{SNR}_o=\frac{k_f^2P}{2N_0W^3/3A_c^2}=\frac{3A_c^2k_f^2P}{2N_0W^3}

Input SNR. Received power Ac22\frac{A_c^2}{2} (constant envelope); noise in BTB_T is N0BTN_0B_T:

SNRi=Ac22N0BT,SNRref=Ac22N0W\text{SNR}_i=\frac{A_c^2}{2N_0B_T},\qquad \text{SNR}_{ref}=\frac{A_c^2}{2N_0W}

Gain and figure of merit:

FOM=SNRoSNRref=3kf2PW2SNRoSNRi=3kf2P BTW3\begin{aligned} \text{FOM} &= \frac{\text{SNR}_o}{\text{SNR}_{ref}}=\frac{3k_f^2P}{W^2} \\ \frac{\text{SNR}_o}{\text{SNR}_i} &= \frac{3k_f^2P\,B_T}{W^3} \end{aligned}

For a single tone m(t)=Amcos⁡ωmtm(t)=A_m\cos\omega_mt: P=Am2/2P=A_m^2/2, Δf=kfAm\Delta f=k_fA_m, β=Δf/W\beta=\Delta f/W, BT=2(β+1)WB_T=2(\beta+1)W (Carson):

FOM=32β2,SNRoSNRi=3β2(β+1)\text{FOM}=\frac{3}{2}\beta^2,\qquad \frac{\text{SNR}_o}{\text{SNR}_i}=3\beta^2(\beta+1)

So FM noise performance improves with the square of the deviation ratio: FM trades bandwidth for SNR. FM beats AM (FOM=1/3\text{FOM}=1/3) when 32β2>13\frac32\beta^2>\frac13, i.e. β>0.471\beta>0.471 (about 0.5).

✓ Answer checked by Claude Opus 5.5 (high effort)

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