17-Phys-B2 Electro-Optical Engineering · December 2018
Question 4 of 7: Receiver SNR — Thermal and Shot-Noise Limits, APD Gain and Photon Counting
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Paper format. 17-Phys-B2 Electro-Optical Engineering,
National Examination December 2018 — a three-hour closed-book examination (one
8.5×11 inch double-sided handwritten note sheet permitted). The cover page states any
five of the seven questions constitute a complete paper and only the first
five as they appear in the answer book are marked; every question is nonetheless answered in
full below so the paper remains a complete study resource.
Reference texts. G. Keiser, Optical Fiber Communications, 4th ed.
(fiber modes, dispersion and bend loss; laser-diode longitudinal modes and DFB gratings; PIN
photodiode responsivity, noise and receiver design; link power and dispersion budgets); B. E. A.
Saleh and M. C. Teich, Fundamentals of Photonics, 2nd ed. (semiconductor optical gain,
LED spontaneous-emission linewidth, avalanche-photodiode noise); A. Yariv, Quantum
Electronics / E. Hecht, Optics, 5th ed. (Mach–Zehnder interferometry and
electro-optic modulators).
Question 4: Receiver SNR — Thermal and Shot-Noise Limits, APD Gain and Photon Counting (20 marks)
Find. (a) SNR, (b) thermal-limited SNR, (c) shot-limited SNR (quantum
limit), (d) APD gain $M$ for SNR = quantum limit − 5 dB, (e) photons/bit at
100 Mbps.
Approach. Compute the unmultiplied signal current $I_s=RP$, then the shot
and thermal noise variances $\sigma_{\text{shot}}^2=2q(I_s+I_d)B$ and
$\sigma_{\text{th}}^2=4kTB/R_L$; the actual SNR is $I_s^2/(\sigma_{\text{shot}}^2+\sigma_{\text{th}}^2)$
and each limiting case keeps only one noise term. For an ideal ($F=1$) APD of gain $M$, signal
and shot noise both scale with $M$ while thermal noise does not, so raising $M$ pushes the SNR
toward the shot-noise (quantum) limit.
Part (a) — actual SNR. The signal current is
$$I_s=RP=(0.5\ \text{A/W})(1\times10^{-6}\ \text{W})=0.50\ \mu\text{A}.$$
The shot-noise variance (signal + dark current) and thermal-noise variance are
$$\sigma_{\text{shot}}^2=2q(I_s+I_d)B,\qquad \sigma_{\text{th}}^2=\frac{4kTB}{R_L},$$
which evaluate to $\sigma_{\text{shot}}^2\approx8.07\times10^{-17}\ \text{A}^2$ and
$\sigma_{\text{th}}^2\approx1.66\times10^{-13}\ \text{A}^2$ — thermal noise already
dominates by more than three orders of magnitude with this small $50\ \Omega$ load. The total
SNR is
$$\mathrm{SNR}=\frac{I_s^2}{\sigma_{\text{shot}}^2+\sigma_{\text{th}}^2}
=\boxed{1.51\ (\,1.78\ \text{dB}\,)}.$$
Part (b) — thermal-noise-limited SNR. Keeping only
$\sigma_{\text{th}}^2$,
$$\mathrm{SNR}_{\text{th}}=\frac{I_s^2}{\sigma_{\text{th}}^2}
=\boxed{1.51\ (\,1.79\ \text{dB}\,)},$$
essentially identical to the total SNR above — confirming this receiver is thermal-noise
limited as designed (unmultiplied, $50\ \Omega$ load, no gain).
Part (c) — shot-noise-limited SNR (quantum limit). Keeping only
$\sigma_{\text{shot}}^2$,
$$\mathrm{SNR}_{\text{shot}}=\frac{I_s^2}{\sigma_{\text{shot}}^2}
=\boxed{3096\ (\,34.91\ \text{dB}\,)}.$$
This is roughly $10^3$ times better than the thermal-limited value — the gap an APD's
internal gain is meant to close.
Part (d) — APD gain for SNR = quantum limit − 5 dB. As
$M\to\infty$ an ideal APD's SNR approaches $\mathrm{SNR}_{\text{shot}}$ from part (c) (both
signal and shot noise scale as $M^2$, so $M$ cancels, while the fixed thermal term becomes
negligible) — that is exactly the "quantum limit." The target is
$$\mathrm{SNR}_{\text{target}}=\mathrm{SNR}_{\text{shot}}\times10^{-5/10}
=3096\times0.3162\approx979.$$
With gain $M$, $I_s(M)=MI_s$ and $\sigma_{\text{shot}}^2(M)=M^2\cdot2q(I_s+I_d)B$ (negligible
excess noise, $F=1$) while $\sigma_{\text{th}}^2$ is unchanged, so
$$\mathrm{SNR}(M)=\frac{M^2I_s^2}{M^2\sigma_{\text{shot}}^2+\sigma_{\text{th}}^2}
=\mathrm{SNR}_{\text{target}}.$$
Solving this quadratic in $M^2$ gives
$$M=\boxed{30.8}.$$
Part (e) — photons per bit at 100 Mbps PCM. The photon energy at
$1.3\ \mu\text{m}$ is
$$h\nu=\frac{hc}{\lambda}=0.954\ \text{eV},$$
and at 100 Mbps the bit period is $T_b=1/(100\times10^{6})=10\ \text{ns}$, so the energy
delivered per bit at the (unmultiplied) received power $P=1\ \mu\text{W}$ is
$E_{\text{bit}}=PT_b=1\times10^{-14}\ \text{J}$, giving
$$N_{\text{photon/bit}}=\frac{E_{\text{bit}}}{h\nu}=\boxed{65443\ \text{photons/bit}}.$$