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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.

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)

Question text not reproduced: the examination questions are © Engineers and Geoscientists BC. Open the official past paper (linked at the top of this page) to read the question, then follow the worked solution below.

Given. A silicon pin diode feeding a transimpedance (shunt-feedback) preamplifier.

Given data — Question 6
QuantitySymbolValue
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.

pin photodiode driving a transimpedance front end−V_biashνpin diode1 MΩ1 pF10 MΩ6 pFdiodeamplifier input−+A = 32v_outR_f = 50 kΩtransimpedance feedbacksumming node sees R_f /(1 + A) shunted by C_d + C_a
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.

  1. 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.
  2. 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: $$R_{\text{eq}} = R_{\text{in}}\parallel(R_{d}\parallel R_{a}) = 1.513\ \text{k}\Omega$$
  3. 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.)
  4. 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 $2qI_{p}B$.
  5. 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.
  6. 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.
Final results — Question 6
QuantitySymbolResult
(a) Responsivity at 0.83 µm$R_{0}$0.335 A/W
(b) Effective input resistance$R_{\text{eq}}$1.51 k$\Omega$
(b) Combination bandwidth$B_{\text{amp}}$15.0 MHz
(b) Equalisation required?—No — 15.0 MHz exceeds the 10 MHz need
(c) Thermal noise (10 MHz)$\langle i_{th}^{2}\rangle$ $3.44\times10^{-18}$ A$^{2}$
(c) Required photocurrent$I_{p}$1.67 µA
(c) Required optical power$P_{\text{in}}$4.98 µW = −23.0 dBm