Abstract
The application of auxiliary-field Monte Carlo techniques to the giant-dipole resonance (GDR) in hot nuclei is described. The method allows for a fully microscopic description of the GDR that includes all effects that were previously modeled macroscopically. Preliminary results obtained with a schematic interaction are presented for 16O and 20Ne using the 0p — 1s0d — 0ƒ 7 2 shell-model configuration space. The difficulties inherent in the method are detailed, and suggestions for future work are given.
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