Abstract
The thermodynamic and transport properties of intermetallic compounds with Ce, Eu, and Yb ions are discussed using the periodic Anderson model with an infinite correlation between electrons. At high temperatures, these systems exhibit typical features that can be understood in terms of a single-impurity Anderson or Kondo model with Kondo scale . At low temperatures, one often finds a normal state governed by the Fermi liquid (FL) laws with characteristic energy scale . The slave boson solution of the periodic model shows that and depend not only on the degeneracy and the splitting of the states, the number of and electrons, and their coupling but also on the shape of the conduction-electrons density of states ( DOS) in the vicinity of the chemical potential . The ratio depends on the details of the band structure which makes the crossover between the high- and low-temperature regimes system dependent. We show that the DOS with a sharp peak close to yields , which explains the “slow crossover” observed in or . The DOS with a minimum or a pseudogap close to yields ; this leads to an abrupt transition between the high- and low-temperature regimes, as found in -like systems. In the case of and , where , we show that the pressure dependence of the coefficient of the electrical resistance, , and the residual resistance are driven by the change in the degeneracy of the states. The FL laws obtained for explain the correlation between the specific-heat coefficient and the thermopower slope or between and the resistivity coefficient . The FL laws also show that the Kadowaki-Woods ratio, , and the ratio assumes nonuniversal values due to different low-temperature degeneracies of various systems. The correlation effects can invalidate the Wiedemann-Franz law and lead to an enhancement of the thermoelectric figure of merit. They can also enhance (or reduce) the low-temperature response of the periodic Anderson model with respect to the predictions of a single-impurity model with the same high-temperature behavior as the periodic one.
- Received 28 November 2008
DOI:https://doi.org/10.1103/PhysRevB.79.115139
©2009 American Physical Society