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

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30<br />

1/e 2 its ma.'{imum value. This distribution can be converted to the angular frequency<br />

distribution<br />

l2.26)<br />

through the vacuum dispersion relationship w = kc = 2rrc/ A. The angular frequency<br />

b<strong>and</strong>width varied as the pulse duration changed. Typically, ~w ranged from 0.021<br />

to 0.053 fs- 1 over the spectral range <strong>of</strong> the Ti:Ah03 laser.<br />

Also note. the wavevectors are expressed explicitly as a function <strong>of</strong> the angular<br />

frequency, k(wd, in order to exhibit the dispersive nature <strong>of</strong> the medium. vVe can<br />

simplify equations (2.23) <strong>and</strong> (2.24) <strong>and</strong> facilitate the calculation <strong>of</strong> the nonlinear<br />

polarization induced by an ultrafast fundamental source by exp<strong>and</strong>ing the wavevector<br />

k(wd to first-order as a power series in (WI - w o ), i.e.<br />

( 'J ·r) -.-1<br />

In Appendix A. the expansion up to first-order is rigorously justified for the systems<br />

<strong>of</strong> interest. The second-order expansion term accounts for the broadening <strong>of</strong> the<br />

fundamental pulse. vVe calculate that for our quartz sample thicknesses, the pulse is<br />

broadened less than 0.3%. For the GaN samples, the broadening is even less. Hence.<br />

a first-order expansion is valid. The symbols in equation (2.27) have their usual<br />

meanings; n(wo) is the index <strong>of</strong> refraction at frequency Wo <strong>and</strong> c is the speed <strong>of</strong> light.<br />

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

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