Heiss W.D. (ed.) Quantum dots.. a doorway to - tiera.ru
Heiss W.D. (ed.) Quantum dots.. a doorway to - tiera.ru
Heiss W.D. (ed.) Quantum dots.. a doorway to - tiera.ru
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44 J.M. Elzerman et al.<br />
The resulting current coming from the drain reservoir is f<strong>ed</strong> <strong>to</strong> a low-noise<br />
IV conver<strong>to</strong>r. In this work we use two types, depending on the desir<strong>ed</strong> bandwidth.<br />
The first one is design<strong>ed</strong> for low-frequency measurements. It has a<br />
bandwidth of about 1 kHz, and a noise floor of ∼5 fA/Hz 1/2 . The fe<strong>ed</strong>back<br />
resistance can be set <strong>to</strong> 10 MΩ, 100 MΩ or 1 GΩ, with an input resistance<br />
that is a fac<strong>to</strong>r 10 3 or 10 4 smaller (for the “low noise” or “low input resistance”<br />
setting, respectively). The faster IV conver<strong>to</strong>r has a bandwidth of<br />
about 150 kHz, and a current noise of ∼1 pA/Hz 1/2 at 100 kHz. The fe<strong>ed</strong>back<br />
resistance is 10 MΩ, corresponding <strong>to</strong> an input resistance of 1.3 kΩ. More<br />
characteristics are given in Sect. 4.<br />
The signal from the IV conver<strong>to</strong>r is then sent <strong>to</strong> an isolation amplifier,<br />
<strong>to</strong> provide optical isolation and possibly gain. Again we can choose a lowfrequency<br />
version (up <strong>to</strong> ∼1 kHz) or a high-frequency one (up <strong>to</strong> ∼300 kHz).<br />
The voltage from the isolation amplifier is finally measur<strong>ed</strong> by a digital multimeter<br />
(Keithley 2700) and sent <strong>to</strong> the computer via GPIB interface. Alternatively,<br />
we can use a lock-in amplifier (Stanford EG&G 5210) if the signal <strong>to</strong> be<br />
measur<strong>ed</strong> is periodic, or an ADwin Gold module for very fast measurements<br />
(up <strong>to</strong> 2.2 × 10 6 14-bit samples per second).<br />
Measurement Wires<br />
To make contact <strong>to</strong> the sample, 2 × 12 twist<strong>ed</strong> pairs of wires <strong>ru</strong>n from two<br />
connec<strong>to</strong>r boxes at room temperature all the way down <strong>to</strong> the “cold finger”<br />
at base temperature. The diameter and material of these wires is chosen <strong>to</strong><br />
minimize the heat load on the mixing chamber. From room temperature <strong>to</strong> 1<br />
Kelvin, 2 × 9 pairs consist of manganine wires (100 µm diameter), and 2 × 3<br />
pairs of copper wires (90 µm diameter). The copper wires can be us<strong>ed</strong> if a large<br />
current has <strong>to</strong> be appli<strong>ed</strong>. From 1 Kelvin <strong>to</strong> the mixing chamber, superconducting<br />
“Niomax” wires (50 µm diameter) are us<strong>ed</strong>. From the mixing chamber<br />
<strong>to</strong> the bot<strong>to</strong>m of the cold finger, where thermal conductivity is no longer a<br />
constraint, we have standard copper wires. At base temperature, one wire of<br />
each twist<strong>ed</strong> pair is connect<strong>ed</strong> <strong>to</strong> “cold ground” (i.e. the cold finger), which is<br />
electrically connect<strong>ed</strong> <strong>to</strong> clean ground via the metal parts of the fridge.<br />
All wires are thermally anchor<strong>ed</strong> <strong>to</strong> the fridge, by carefully wrapping them<br />
around copper posts, at several temperature stages (4 K, 1 K, ∼100 mK and<br />
∼10 mK). At room temperature, the resistance of the wires is about 250 Ω or<br />
150 Ω for the manganine or copper wires, respectively. At low temperature it<br />
is about 50 Ω. The wires have various parasitic capacitances <strong>to</strong> their twist<strong>ed</strong><br />
partner and <strong>to</strong> ground, as indicat<strong>ed</strong> in Fig. 11 and Fig. 12.<br />
Filtering<br />
The wires connect the device <strong>to</strong> the measurement electronics at room temperature,<br />
so they have <strong>to</strong> be carefully filter<strong>ed</strong> <strong>to</strong> avoid that the electrons in