Abstract
The thermal linear response theory with the inclusion of the non· Markovian effect is formulated based on the thermal cranked Hartree·Fock·Bogoliubov (THFB) theory. We propose the proper strength function which is suitable to be compared with y-ray spectra from giant resonances at high spin and high temperature. A clarification is given of the relation between the stability condition of the THFB solution and the equation in the thermal random phase approximation (TRPA).
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