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Screened Anderson model

Journal Article · · Physical Review, B: Condensed Matter; (USA)
 [1];  [2]
  1. Department of Physics, The University of Tennessee, Knoxville, Tennessee 37996-1501 (USA)
  2. Solid State Division, Oak Ridge National Laboratory, TN (USA) Department of Physics, The University of Tennessee, Knoxville, Tennessee 37996-1501 (USA)

The occupation number ({ital n}{sub {ital f}}) of the impurity orbital ({ital f}) in the Anderson model is calculated as a function of the orbital energy ({var epsilon}{sub {ital f}}), taking into account finite values for the Coulomb interactions between the impurity and the conduction electrons ({ital G}) and between two electrons inside of the localized orbital ({ital U}). For small values of {ital G}, the transitions {ital f}{sup 2}{r arrow}{ital f}{sup 1}{r arrow}{ital f}{sup 0} occur, with a step at {ital n}{sub {ital f}}=1. By increasing {ital G} this step vanishes, with a direct transition {ital f}{sup 2}{r arrow}{ital f}{sup 0}, which is a typical result of an effective {ital U}{lt}0.

DOE Contract Number:
AC05-84OR21400
OSTI ID:
5536252
Journal Information:
Physical Review, B: Condensed Matter; (USA), Journal Name: Physical Review, B: Condensed Matter; (USA) Vol. 43:13; ISSN 0163-1829; ISSN PRBMD
Country of Publication:
United States
Language:
English