22-Elec-B10 Electro-Optical Engineering · December 2017
Question 6 of 7: pin diode with a transimpedance front end — responsivity, bandwidth and required optical power
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
Paper format. 16-Elec-B10, Electro-Optical Engineering —
National Exams, December 2017. Three hours, closed book; one 8.5 in × 11 in
double-sided sheet of hand-written notes and a Casio or Sharp approved calculator are
permitted. Seven questions, all of equal value (20 marks each); the rubric says
any five questions constitute a complete paper. All seven are solved below,
because the set is a study resource rather than a timed sitting.
Reference texts.
G. Keiser, Optical Fiber Communications, 4th ed. — fibre modes,
dispersion, link power and rise-time budgets, photodetectors.
J. M. Senior, Optical Fiber Communications: Principles and Practice, 3rd ed.
— numerical aperture, intermodal/intramodal dispersion, receiver noise.
B. E. A. Saleh and M. C. Teich, Fundamentals of Photonics, 3rd ed. —
laser rate equations, photon lifetime, electro-optic modulators.
J. Wilson and J. F. B. Hawkes, Optoelectronics: An Introduction, 3rd ed.
— pin and avalanche photodiodes, Pockels cells.
Physical constants are the ones printed on page 1 of the examination paper:
$c = 2.998\times10^{8}\ \text{m/s}$, $q = 1.602\times10^{-19}\ \text{C}$,
$h = 6.626\times10^{-34}\ \text{J}\cdot\text{s}$,
$k = 1.381\times10^{-23}\ \text{J/K}$,
$\varepsilon_{0} = 8.854\times10^{-12}\ \text{F/m}$, and for the modulator crystal
$\varepsilon_{r}(\text{LiNbO}_3) = 32$, $n_{o} = 2.30$, $r = 30\ \text{pm/V}$.
Check: two book-keeping notes on the source paper.
The page-5 marking scheme lists five sub-parts, (a)–(e), for Questions 5 and 7, but
the printed questions on pages 3 and 4 carry only four sub-parts each; the mark totals
still come to 20, so the extra row is a marking-sheet artefact and every printed sub-part
is answered here. Question 6 also carries the hand-added annotation
“rework this one” next to its heading — an examiner’s note on the
printed paper, not part of the question. It is solved exactly as printed.
Question 6: pin diode with a transimpedance front end — responsivity,
bandwidth and required optical power (20 marks)
Given. A silicon pin diode feeding a transimpedance (shunt-feedback)
preamplifier.
Given data — Question 6
Quantity
Symbol
Value
Wavelength / external quantum efficiency
$\lambda$ / $\eta$
0.83 µm / 50 %
Dark current / temperature
$I_{d}$ / $T$
0.5 nA / 295 K
Feedback resistor / open-loop gain
$R_{f}$ / $A$
50 k$\Omega$ / 32
Diode resistance / capacitance
$R_{d}$ / $C_{d}$
1 M$\Omega$ / 1 pF
Amplifier input resistance / capacitance
$R_{a}$ / $C_{a}$
10 M$\Omega$ / 6 pF
Required post-detection bandwidth
$B$
10 MHz
Required signal-to-noise ratio
$\text{SNR}$
55 dB
Find. The responsivity, the bandwidth of the diode-plus-amplifier
combination and whether equalisation is needed, and the incident optical power in dBm that
achieves the specified SNR.
The pin diode and its transimpedance front end. Shunt feedback divides the effective input resistance by $(1+A)$, so the input pole set by $C_d + C_a$ is pushed far above what the same resistor would allow in a high-impedance design.
Approach. Responsivity comes straight from the quantum efficiency;
the bandwidth from the Miller-reduced input resistance working into the total input
capacitance; and the required power from equating the signal-to-noise ratio, with shot and
thermal noise, to the specified 55 dB and solving the resulting quadratic for the
photocurrent.
Responsivity. Each absorbed photon of energy $hc/\lambda$ yields
$\eta$ electrons of charge $q$, so
$$R_{0} = \frac{\eta q \lambda}{hc}
= \frac{(0.50)(1.602\times10^{-19})(0.83\times10^{-6})}
{(6.626\times10^{-34})(2.998\times10^{8})}$$
$$\boxed{R_{0} = 0.335\ \text{A/W}}$$
The convenient shortcut is $R_{0} = \eta\lambda[\mu\text{m}]/1.24 = 0.5(0.83)/1.24$, which
gives the same value.
Effective input resistance. Shunt feedback around a gain of $A$ makes
the summing node look like $R_{f}$ divided by the loop gain:
$$R_{\text{in}} = \frac{R_{f}}{1+A} = \frac{50\times10^{3}}{33} = 1.52\ \text{k}\Omega$$
The diode and amplifier bias resistances sit in parallel with it,
$R_{d}\parallel R_{a} = (1\ \text{M}\Omega)\parallel(10\ \text{M}\Omega) = 909\ \text{k}\Omega$,
which is so much larger that it barely matters:
$$R_{\text{eq}} = R_{\text{in}}\parallel(R_{d}\parallel R_{a}) = 1.513\ \text{k}\Omega$$
Combination bandwidth. The total capacitance shunting that node is
$C_{T} = C_{d}+C_{a} = 1 + 6 = 7\ \text{pF}$, so the front-end pole sits at
$$B_{\text{amp}} = \frac{1}{2\pi R_{\text{eq}} C_{T}}
= \frac{1}{2\pi (1512.7)(7\times10^{-12})}$$
$$\boxed{B_{\text{amp}} = 15.0\ \text{MHz}}$$
Since $15.0\ \text{MHz} \gt 10\ \text{MHz}$, the front end already passes the required
post-detection band, so no equalisation is necessary. (Had the same 50
k$\Omega$ been used as a plain high-impedance load, the pole would have sat at
$1/[2\pi(47.4\ \text{k}\Omega)(7\ \text{pF})] = 480\ \text{kHz}$ and heavy equalisation would
have been unavoidable — that factor of 31 is exactly the loop gain $1+A$, and it is the
reason the transimpedance topology is used.)
Noise sources at the required bandwidth. Thermal noise is generated by
the resistances shunting the input; taking the parallel combination
$R_{\text{th}} = R_{f}\parallel R_{d}\parallel R_{a} = 47.4\ \text{k}\Omega$,
$$\langle i_{th}^{2}\rangle = \frac{4kTB}{R_{\text{th}}}
= \frac{4(1.381\times10^{-23})(295)(10^{7})}{47.38\times10^{3}}
= 3.44\times10^{-18}\ \text{A}^{2}$$
The dark-current shot noise is
$\langle i_{d}^{2}\rangle = 2qI_{d}B = 1.60\times10^{-21}\ \text{A}^{2}$, three orders of
magnitude smaller, and the signal shot noise is $2qI_{p}B$.
Solve for the photocurrent. Writing the signal-to-noise ratio as a
power ratio, $\text{SNR} = 10^{55/10} = 3.162\times10^{5}$, and
$$\text{SNR} = \frac{I_{p}^{2}}{2q(I_{p}+I_{d})B + \langle i_{th}^{2}\rangle}$$
Rearranging gives a quadratic in $I_{p}$,
$$I_{p}^{2} - \text{SNR}\,(2qB)\,I_{p}
- \text{SNR}\left(2qI_{d}B + \langle i_{th}^{2}\rangle\right) = 0$$
$$I_{p}^{2} - (1.013\times10^{-6})I_{p} - 1.088\times10^{-12} = 0$$
whose positive root is
$$\boxed{I_{p} = 1.67\ \mu\text{A}}$$
Substituting back reproduces $\text{SNR} = 3.162\times10^{5}$ exactly, confirming the
root.
Convert to optical power. Dividing by the responsivity,
$$P_{\text{in}} = \frac{I_{p}}{R_{0}} = \frac{1.666\times10^{-6}}{0.3347}
= 4.98\ \mu\text{W}$$
$$P_{\text{in}}[\text{dBm}] = 10\log_{10}\!\left(\frac{4.978\times10^{-6}}{10^{-3}}\right)$$
$$\boxed{P_{\text{in}} = -23.0\ \text{dBm}}$$
The signal shot-noise term contributes about two-thirds of the total noise at this
operating point, so the receiver is close to the crossover between the thermal-limited and
shot-limited regimes — which is why the quadratic, rather than the simpler
thermal-only approximation, was worth solving.