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

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131<br />

where p(O) is the density operator in thermal equilibrium, <strong>and</strong> p(i) represent the ith<br />

order perturbation to p(O). Once p is determined, the nonlinear polarization is calculated<br />

as<br />

(5.9)<br />

vVe simplify the rules for Feynman diagrams by observing that the three virtual<br />

transitions for second-harmonic generation leave the state unaltered. Although each<br />

photon process induces a phase shift in p(2), the net phase shift is zero for SHG.<br />

Therefore, we will disregard the net phase shift caused by each photon process. The<br />

rules for double sided Feynman diagrams are as follows.<br />

1. The state starts with Il)p~?)(ll. For SHG, the state also ends with Il)p}?l(ll.<br />

2. For the ket side, a vertex that brings the state from Il) to 1m) by absorption <strong>of</strong> a<br />

photon with angular frequency WI corresponds to the matrix element<br />

(ml - erjE(wdll)<br />

iii<br />

(5.10)<br />

where -erj is the dipole moment operator along the direction i <strong>and</strong> E(;.;d is the<br />

electric field. For an emission process, the matrbc element is<br />

(ml - eriE*(wdll)<br />

iii<br />

(5.11)<br />

Similarly, the matrix element that represents absorption <strong>of</strong> a photon on the bra side<br />

is<br />

-(ll - eriE(wdlm)<br />

iii<br />

(5.12)<br />

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

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