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Superconducting Technology Assessment - nitrd

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Josephson output interfaces have demonstrated low bit error rate at 10 Gbps, using 8 kA/cm 2 junctions. A critical<br />

current density of 20 kA/cm 2 is probably sufficient for 50 Gbps output interfaces.<br />

The output voltage of demonstrated JJ interface circuits is sufficient to sustain a low bit error rate at 50 Gbps.<br />

Reasonable estimates can be made of the signal power required at the Josephson output drivers. If ribbon cable<br />

can carry electrical signals with 3 dB of signal loss to amplifiers at 40 K with 3 dB noise figure, then 4 mV pp on the<br />

Josephson drivers will sustain a bit error rate of 1e-15.<br />

The crossbar switch program provides a rich experience base in the art of ribbon cables. In particular the trade off<br />

between heat leak and signal loss is well understood.<br />

5.3.3 OUTPUT: 4 K RSFQ TO ROOM TEMPERATURE ELECTRONICS<br />

– ISSUES AND CONCERNS<br />

A focused program to provide the capability to output 50 Gbps from cold to warm electronics must overcome some<br />

remaining technical challenges, both electronic and optical.<br />

Electronics Issues<br />

There are two major electronic challenges:<br />

■ Designing custom integrated circuits in a high-speed semiconductor technology to minimize<br />

refrigeration heat loads. These include analog equalizers to compensate for frequency dependent<br />

cable losses, wideband low-noise amplifiers, and 50 Gbps decision circuits. COTS parts are<br />

optimized for room-temperature operation and they run very hot. ASICs optimized for low<br />

power operation at cryogenic temperatures will be needed. The circuitry which directly drives<br />

electro-optical components such as VCSELs or modulators must be easily integrable with these<br />

device technologies.<br />

■ Designing ribbon cables with better dielectrics to carry signals at 50 Gbps. Existing cables have<br />

significant dielectric losses at frequencies above 10 GHz. Data at 50 Gbps has significant power<br />

at frequencies up to 35 GHz for NRZ format, and up to 70 GHz for RZ format. The development<br />

of better RF cables, particularly for 4 K to intermediate temperature, is discussed in Section 6.<br />

Optics Issues<br />

Although development of components to either generate or modulate optical streams at 50 Gbps at cryogenic<br />

temperatures will require substantial investment, the panel believes current efforts in the field support optimism<br />

that one or more of the possible approaches will be successful by 2010. In decreasing order of difficulty these<br />

efforts are:<br />

■ Achieving low drive power, word-wide arrays of VCSELS, capable of operating at 50 Gbps either<br />

as a directly modulated laser or as an injection-locked modulator.<br />

■ Achieving 50 Gbps word-wide receiver arrays complete with data processing electronics, for<br />

room-temperature operation.<br />

■ Producing a frequency comb laser to be used in conjunction with low-power modulators<br />

to allow use of Dense Wavelength Division Multiplexing to reduce optical fiber count to one<br />

input and one output fiber per processor, each carrying up to 4 Tbps.<br />

107

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