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Design Article

Audio amplifier topology with push-pull transimpedance stage - Part 3: Experimental verification

Samuel Groner

10/24/2012 11:28 AM EDT

Noise, stability, PSRR and slew rate

Next I have evaluated the equivalent input noise of both amplifiers. Measured in a 22 Hz to 22 kHz bandwidth, the amplifier from figure 11 achieves –122.6 dBu (this includes the noise from the feedback network, with an effective total resistance of 98Ω). While this is already an excellent figure, the new amplifier topology does even better with –124.5 dBu.

This surprisingly large difference cannot be attributed to the input differential pair, as its implementation is equal for both amplifiers, and spread in transistor performance is probably lower than the measured deviation. To the extent that I have investigated this, I can explain the observed behaviour with the current mirror noise contribution. As noted in section 4, the new amplifier topology allows the choice of much larger emitter resistors for the current mirror (for the presented implementations the values are 2 kΩ for the new push-pull stage, and 150 Ω for the standard amplifier), which reduces current mirror noise.

Despite the additional noise contribution of the folded cascodes, this leads to overall better noise performance for the novel amplifier architecture. The emitter resistors of the standard topology cannot be made significantly larger without further circuit changes, as the current mirror output might become saturated under certain conditions.

Well-mannered overload behaviour is, particularly with more complex amplifier topologies, not always easily achieved. Typical artefacts include [2]:

  • Polarity reversal during clipping
  • Oscillation during, or during recovery from, clipping
  • Prolonged recovery from clipping

Fortunately the basic overload behaviour of the novel amplifier topology is quite good; figure 14 depicts the output voltage of the model amplifier from figure 12 attempting to provide a 10 kHz, 4 VPP triangle waveform output with ±15 V power supplies. There is some prolonged recovery from clipping discernible, but no polarity reversal or instability.

Figure 14: Overload behavior of the model amplifier from figure 12.

In contrast, the standard amplifier topology shows distinctly asymmetric overload behaviour, and for negative clipping, considerable artefacts (see figure 15). While I do not believe that there are drastic audible differences between the overload behaviour of the two amplifier topologies - last but not least, serious clipping sounds pretty bad anyway, and the observed artefacts occur in the µs range - an oscilloscope display similar to figure 14 will surely please a reviewer's eyes much more than one close to figure 15.

Figure 15: Overload behavior of the model amplifier using the standard amplifier topology.

These measurements neglect the contribution of the power transistors in the output buffer. Often these suffer themselves from considerable recovery time [2], and it may be desirable to prevent saturation of these transistors by clamping the output voltage of the transimpedance stage to a well defined threshold below the power supply voltage. Implementation of such a clamping arrangement is often difficult, particularly because it must not impair the distortion performance of the amplifier below clipping. Some possible implementations may be found in [2].

As the model amplifier from figure 12 does not implement voltage regulators for the amplifier front end, and hence the potential power supply rejection advantage of the new topology is not fully realised, I have not carried out detailed power supply rejection measurements yet. Initial measurements however indicate that the main injection mechanism is indeed absent, and that the model amplifier from figure 12 has - even without the voltage regulators - overall better power supply rejection than the standard amplifier implementation shown in figure 11.

Last but not least the slew rate of these two model amplifiers was evaluated. The measurement results were +46.8 V/µs and –45.6 V/µs for the standard topology and +42.3 V/µs and –43.4 V/µs for the novel amplifier. These results are mainly determined by the primary slew rate limitation (finite output current of the input stage), which masked the expected advantage of the novel topology. The overall lower slew rate of the novel amplifier is probably just a result of parts tolerances, which lead to lower input stage quiescent current; possibly there is also a minor systematic effect from the input stage folded cascodes.

To also model the, at high frequencies potentially considerable, drive current demand of a power output stage, I've added a 3.3 kΩ resistor from the second stage output node to ground. This was sufficient tomake the slew rate behaviour of the standard topology more asymmetric (the measured values are +42.4 V/µs and –44.6 V/µs). The new push-pull configuration however easily supported the increased output current. The resulting slew rates are +41.4 V/µs and –42.6 V/µs, which is nearly the same as what is observed without the loading resistor.

To more thoroughly verify the absence of slew rate limitations in the second stage, I have also constructed a model amplifier based on the topology sketched in figure 8, using the input stage modifications derived in [8] and the very same second stage implementation as shown in figure 12. With a total input stage quiescent current of about 20 mA, and a compensation capacitor of 100 pF, the achieved slew rate was +226.6 V/µs and –228.3 V/µs. Additional loading at the transimpedance stage output altered this to just +223.5 V/µs and –222.4 V/µs.

This is enough evidence to conclude that the novel transimpedance stage indeed supports very high slew rates; simulation results indicate that, with appropriate changes to the input stage, much higher values are theoretically possible. However the effects from finite small-signal bandwidth soon makes further efforts in this direction meaningless.


Next: Conclusion




pcsalex

10/25/2012 7:18 AM EDT

Figure 12, Q9 and Q10 collectors shorted!

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pcsalex

10/25/2012 7:21 AM EDT

sorrry figure 12 Q9 and Q10 base are shorted ?

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ZekeR

11/2/2012 5:04 PM EDT

It's okay. Q9 and Q10 minimize the stage's crossover distortion. Their bases are meant to be connected.

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Fabio007

11/5/2012 2:48 AM EST

Q9, Q10 with collectors together and to gnd, and bases together: Yes I can see that these just buffer the signal (current) at Q5 collector before reaching Q11 Q12, however I would feel more comfortable it they operated with some voltage across their respective CB junctions - at least the SPICE modelling would be more accurate, I think; plus the Ft should be better (higher), so maybe those feed-forward capacitors C4, C5 could be smaller. A Vbe multiplier (or diode string) between collectors of Q5 and Q8 (with bypass capacitor) would be just fine for this, so that Q9 and Q10 both operate with Vcb of about 2V. This would not affect Q11 and Q12 except for reselecting bias resistors R13, R14.

Also I note there is just one diode string for the bias voltages for the output stage and input stages. This means signal (and load) current modulation of the base currents of Q15, Q16 will affect currents flowing in bias diodes D1 to D10, which will then affect the other stages.

Question: is there a reason the bias voltage for input stage (Q3, and Q4, Q5) is higher that of the output stage Q15, Q16 (5 diode drops vs just 2), or is this an attempt to reduce the aforementioned bias voltage modulation without resorting to separate bias networks and their associated increased bias current?

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Fabio007

11/7/2012 5:53 AM EST

This is a good topology; it has nice features (like the signal remaining a current right up until being converted to a voltage by a well-biased common-base stage that can charge/discharge capacitances rapidly). However, I’m not so sure the comparison of the “amplifier with new trans-impedance stage” in fig 12 with the “standard 2 stage topology” of figure 11 is entirely fair.

The amplifier of fig 12 has an extra transistor providing gain compared to the amplifier of fig 11. In Fig 12 the current signal output of the differential stage (the folded cascade stage does not amplify, it only provides a level-shifting function) is amplified by TWO transistors: both Q9 and Q11. This amplified current then gets converted to a voltage by the common-base amplifier stage Q15. This is three (3) transistors in total providing the gain of the output signal from the differential stage. Compare this with figure 11. Only Q6 and Q7 (forming a trans-impedance amplifier) amplify the output of the differential stage.

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Fabio007

11/7/2012 5:53 AM EST

Further, in Fig 11 the output stage is not complementary (push-pull) driven as is the case in Fig 12. In fig 11 Q7’s collector is loaded by a standard constant current source formed by Q9. In fig 12, Q10, Q12, form the complementary driver for Q16; there is no such complementary driver for Q9 in Fig 11.

Note also the extra bias current of fig 12, where Q9 is biased at 1mA, Q11 at 6mA, and Q15 at 7mA. Whereas in fig 11 the trans-impedance stage has bias currents of 1mA for Q6, and 6mA for Q7; there is no third stage biased at a current close to that of Q7.

Looking at transistor count: Fig 11 has a total of 11 transistors. Fig 12 has a total of 18; the extra 7 transistors are due to:-
a) folded cascade level shifter (3 extra if we include Q6);
b) one extra gain transistor (Fig 12s Q11)
c) three extra for the complementary driver (Fig 12s Q10, Q12, Q14).

For a fair comparison pitting purely topology against topology, perhaps it would be fairer to throw an extra 7 transistors at Fig 11 (say, by adding an extra gain transistor between Q6 and Q7 biased at about 6mA, and then add a complementary driven load for collector of Q7), and then seeing how they compare.

If that is done, then it may well happen that the amplifier of Fig 12 may still come out ahead for the measurements of interest (THD +N, and power supply ripple rejection); but I suspect the difference may not be all that great.

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