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William Angerer - Department of Physics and Astronomy - University ...

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199<br />

From this criteria, we determine the time required to satisfy this inequality. The<br />

count rate is expressed as<br />

(7.15)<br />

where i represents SHG or back. The critical detection time, Td is therefore<br />

(7.16)<br />

where Ide is the duty cycle ratio <strong>of</strong> the the gate, e.g. Ide = 0.4 for a 400 f.lS gate <strong>and</strong><br />

a chopper frequency <strong>of</strong> 1 kHz. Equation (7.16) illustrates the importance <strong>of</strong> reducing<br />

the background count to the lowest possible value. For example if the SHG photon<br />

count rate is 100 Hz <strong>and</strong> the background count rate is 1000 Hz. then Td = 19 s. In<br />

contrast. lowering the background rate to 100 Hz with the same signal count rate<br />

reduces the detection time to 0.27 s. In practice, we were able so far to lower the<br />

background count rate to ",,15 Hz by placing the detection apparatus in a nearly light<br />

tight box <strong>and</strong> covering the entire apparatus with black cloth.<br />

During a typical measurement <strong>of</strong> the nonlinear response <strong>of</strong> carbon nanotubes. \ve<br />

scanned a 10 f.lm x 10 f.lm area <strong>of</strong> the sample mask at a rate <strong>of</strong> one pixel per 10 s.<br />

So far we have not been able to unambiguously detect the carbon nanotubes in our<br />

measurements. Using the above analysis, we determined that TSHG < 6 Hz.<br />

Reproduced with permission <strong>of</strong> the copyright owner. Further reproduction prohibited without permission.

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