skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Magnetic impurity coupled to interacting conduction electrons

Journal Article · · Physical Review, B: Condensed Matter
 [1]
  1. Max-Planck-Institut fuer Physik komplexer Systeme, Bayreuther Strasse 40 Haus 16, D-01187 Dresden (Germany)

We consider a magnetic impurity which interacts by hybridization with a system of weakly correlated electrons and determine the energy of the ground state by means of a 1/{ital N}{sub {ital f}} expansion. The correlations among the conduction electrons are described by a Hubbard Hamiltonian and are treated to the lowest order in the interaction strength. We find that their effect on the Kondo temperature, {ital T}{sub {ital K}}, in the Kondo limit is twofold: first, the position of the impurity level is shifted due to the reduction of charge fluctuations, which reduces {ital T}{sub {ital K}}. Secondly, the bare Kondo exchange coupling is enhanced as spin fluctuations are enlarged. In total, {ital T}{sub {ital K}} increases. Both corrections require intermediate states beyond the standard Varma-Yafet ansatz. This shows that the Hubbard interaction does not just provide quasiparticles, which hybridize with the impurity, but also renormalizes the Kondo coupling. {copyright} {ital 1996 The American Physical Society.}

OSTI ID:
279089
Journal Information:
Physical Review, B: Condensed Matter, Vol. 53, Issue 9; Other Information: PBD: Mar 1996
Country of Publication:
United States
Language:
English

Similar Records

Magnetic impurity in the one-dimensional Hubbard model
Journal Article · Tue Jul 01 00:00:00 EDT 1997 · Physical Review, B: Condensed Matter · OSTI ID:279089

Two-impurity Anderson model: A variational study
Journal Article · Wed Sep 01 00:00:00 EDT 1993 · Physical Review, B: Condensed Matter; (United States) · OSTI ID:279089

Properties of YbAgCu{sub 4} at high pressures and magnetic fields
Journal Article · Tue Aug 01 00:00:00 EDT 1995 · Physical Review, B: Condensed Matter · OSTI ID:279089