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

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Chapter 3<br />

Experimental Ultrafast Nonlinear Optical Spectroscopy<br />

In this chapter we discuss the nonlinear optical spectroscopy experimental setup. A<br />

further discussion <strong>of</strong> our spectra normalization <strong>and</strong> the effects <strong>of</strong> an ultrafast laser<br />

pulse on our measured second-harmonic generation signals (see also section 2.4.2) is<br />

given. In addition, the characteristics <strong>of</strong> the fundamental light generating source. the<br />

Ti:AI 2 0 3 laser, are discussed at length.<br />

3.1 Optical Setup<br />

Fig. 3.1 displays a schematic <strong>of</strong> the nonlinear optical setup. This setup is somewhat<br />

similar to the one used by M. S. Yeganeh <strong>and</strong> J. Qi [49, 41J, but with a different<br />

fundamental light source. The fundamental light source with frequency ....: was a<br />

Ti:AI 2 0 3 laser, the details <strong>of</strong> which will be more thoroughly discussed in section 3.3.<br />

Briefly, the Ti:AI 2 0 3 laser produces ultrashort near IR laser pulses (",,700-1000 nm)<br />

at rate <strong>of</strong> 76 MHz. The individual ultrashort pulses have sufficiently high peak powers<br />

(",,50 kvV) to produce measurable nonlinear optical effects. Polarization <strong>of</strong> both<br />

51<br />

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

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