We report theoretical studies of electron and hole lifetimes in a free-electron gas as well as in real metals Al and Nb by means of the ab initio many-body method and semi-empirical scattering theory approach. We show that for free-electron-like excitations a simple density-of-state convolution model of the scattering theory approach (STA-DOS) is a good approximation to the ab initio lifetimes, the energy dependence of the STA-DOS transition matrix element being rather unimportant. The approximation of energy-independent matrix element appears to also be reasonable for Nb. A good correspondence between the STA-DOS and ab initio momentum-averaged results is achieved for Nb with an adjusted matrix element, although the ab initio lifetimes disperse greatly with respect to the averaged value.
No takes yet. Share an insight, caveat, or question.
Zhukov et al. (2002) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: