Abstract
The stability of the metallic phase for the electronically three-dimensional AC$ 60$ compounds is considered theoretically. A calculation of a possible metal-insulator transition temperature as a function of the degree of imperfect nesting of the Fermi surface is performed. We find that RbC$ 60$ and CsC$ 60$ are unique systems so far where the instability of the metallic phase originates from the nearly half filled conduction band and not from a low dimensionality of the electronic properties.
Original language | English |
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Pages (from-to) | 13861-13864 |
Number of pages | 4 |
Journal | Physical Review B |
Volume | 56 |
Issue number | 21 |
DOIs | |
Publication status | Published - 1997 |
Austrian Fields of Science 2012
- 103009 Solid state physics