23.05.2014 Views

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

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

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

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

139<br />

6.2 Nonlinear Rotational Symmetry <strong>of</strong> GaN<br />

In section 2.3 we discussed the relationship between the allowed second-order susceptibility<br />

elements <strong>and</strong> the symmetry <strong>of</strong> the media. In this section we discuss our<br />

investigations <strong>of</strong> the symmetry <strong>of</strong> GaN by second-harmonic generation. By measuring<br />

second-harmonic intensity as a function <strong>of</strong> the angle between the incident beam <strong>and</strong><br />

crystal a.'{es for a variety <strong>of</strong> polarizations, we probed the symmetry <strong>of</strong> our Ga.\" thin<br />

films. Fig. 6.1 displays the geometry <strong>of</strong> the sample <strong>and</strong> the fundamental <strong>and</strong> secondharmonic<br />

beams. Because SHG is mediated by a third rank tensor, second-harmonic<br />

generation is a more sensitive probe <strong>of</strong> crystal symmetry than linear spectroscopies,<br />

which are mediated by second rank tensors.<br />

The second-harmonic response <strong>of</strong> GaN is determined by transforming the dipole<br />

allowed second-order nonlinearities in the crystal frame <strong>of</strong> reference to the lab frame<br />

<strong>of</strong> reference. i.e.<br />

(2),lab _ R(A.). R( '). R( .) (2),crystal<br />

Xijk - liJ 10

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!