NONLINEAR-THEORY OF SHORT-WAVELENGTH FREE-ELECTRON LASERS

The nonlinear evolution of free-electron laser (FEL) amplifiers is stu died for infrared and shorter wavelengths. The configuration of intere st consists in the propagation of an energetic electron beam through a drift tube in the presence of a periodic wiggler magnetic field with planar symmetry. A three-dimensional formulation is derived in which t he electromagnetic field is represented as an expansion of Gaussian op tical modes. Since the wiggler model is characterized by planar symmet ry, the Gauss-Hermite modes are used for this purpose. A set of nonlin ear differential equations is derived for the evolution of the amplitu de and phase of each mode, and they are solved simultaneously in conju nction with the three-dimensional Lorentz force equations for an ensem ble of electrons in the presence of the magneto-static wiggler, self-e lectric and self-magnetic fields due to the charge and current distrib utions of the beam, and the electromagnetic fields. It is important to note that no wiggler average is used in the integration of the electr on trajectories. This permits the self-consistent modeling of effects associated with (1) the injection of the beam into the wiggler, (2) em ittance growth due to inhomogeneities in the wiggler and radiation fie lds as well as due to the self-fields, (3) the effect of wiggler imper fections, and (4) betatron oscillations. The optical guiding of the ra diation field is implicitly included in the formulation. This approach has important practical advantages in analyzing FELs, since it is nec essary only to characterize the beam upon injection into the wiggler, and the subsequent evolution is treated self-consistently. Numerical s imulations are performed for two examples corresponding to an infrared FEL at wavelengths near 3.5 mu m, and an x-ray FEL operating in the n eighborhood of 1.4 Angstrom wavelengths corresponding to the proposed linear coherent light source (LCLS) at the Stanford Linear Accelerator Center. Results for both cases indicate that the more severe limiting factor on the performance of the FEL is the beam emittance. For the i nfrared example, the transition to the thermal regime occurs for an ax ial energy spread of Delta gamma(z)/gamma(0) approximate to 0.19%, and optimal performance is obtained for Delta gamma(z)/gamma(0)<0.1% and gamma is the relativistic factor. This restriction is more severe for the LCLS parameters, for which the thermal transition is found for Del ta gamma(z)/gamma(0) approximate to 0.05% and optimal performance requ ires Delta gamma(z)/gamma(0) less than or equal to 0.01%. Wiggler impe rfections are found to be a much less important constraint on FEL desi gn. Simulations indicate that there is no coherent ''walkoff'' of the beam from the symmetry axis due to wiggler imperfections, and that the radiation field is sufficiently guided by the interaction that no sev ere degradation is found in the extraction efficiency or growth rate f or moderate levels of wiggler fluctuations.