Abstract
The energy bands of Cu have been calculated self-consistently through use of the improved exchange approximation of Herman, Van Dyke, and Ortenburger (the so-called Xαβ method). The resulting bands are compared with the self-consistent energy bands calculated by the Xα method with α=1.00, 56, 0.721, and 23. The Xα and Xαβ energy-band widths (sp, d) are compared with photoemission data. The differences between the energy-band calculations and the atomic calculations are described. A brief discussion is given of the role of the virial theorem and the variational principle.