190 Light–Matter Interaction
The description of the various processes in Fig. 3.15 by Eqs. (3.127)–(3.129) dif-
fers only in the initial conditions, that is the field amplitudes at the crystal input.
This system of equations is analogous to the ones encountered for SHG. For
relatively weak pulses, conversion efficiencies are low, and the group velocity
dispersion contributes to a broadening of the generated radiation.
As in the case of SHG, there is a particularly interesting regime which
combines the complexities of short pulses, high intensity, and long interaction
lengths. The pulses have to be sufficiently short that simultaneous phase match-
ing cannot be achieved over the pulse bandwidth. The crystal length and pulse
intensities are sufficiently