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

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158<br />

where v /2 is the group velocity <strong>of</strong> the free wave in the sapphire <strong>and</strong> Vbl is the group<br />

velocity <strong>of</strong> the bound wave in GaN. We calculated this time by replacing each wavevector<br />

with the inverse <strong>of</strong> its group velocity. This transformation follows directly from a<br />

first-order expansion with respect to angular frequency <strong>of</strong> the wavevectors that appear<br />

in phases (see section 2.4.2). Thus, ultrafast effects are included in the D~B wave by<br />

multiplying the phase by a Gaussian centered at the time required to propagate the<br />

wave from point:\. to point B, i.e.<br />

(6.35 )<br />

where ~w is the angular frequency b<strong>and</strong>width <strong>of</strong> our Ti:AI 2 0 3 laser. The ultrafast<br />

effects are incorporated into the other D waves by similar transformations.<br />

6.4 Second-Harmonic Generation Spectra from GaN / Ah03<br />

In this section we discuss our SHG spectra from GaN / :\.1 2 0 3 in the p-in/s-out <strong>and</strong><br />

p-in/p-out polarizations. From these spectra we extract X~~x <strong>and</strong> :'(~~x' respectively.<br />

In addition, from our rotational symmetry measurements as a function <strong>of</strong> the angle<br />

<strong>of</strong> incidence, we determined that the sample miscut does not induce any symmetry<br />

r b'dd l' . . (2) (2)<br />

lor 1 en non meantles, e.g. Xzzx or Xxzx'<br />

In order to accurately calculate the effects <strong>of</strong> group velocity mismatch in our Ga0;<br />

films, we measured ~w at each wavelength by determining the wavelength distribution<br />

<strong>of</strong> the pulse with a monochrometer. In practice, group velocity mismatch is most<br />

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

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