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Problem: Anderson Model

      The Anderson Hamiltoniangif describes electrons in a transition metal, including the interactions between the electrons:

  eqnarray3033

where tex2html_wrap_inline7115 and tex2html_wrap_inline6917 indicate the spin state, tex2html_wrap_inline7119 , and tex2html_wrap_inline7121 ; this is similar for ``down" spins. The first term in the Hamiltonian corresponds to electrons in a broad conduction band with energy tex2html_wrap_inline6181 , where tex2html_wrap_inline5233 is the wavenumber. Assume that tex2html_wrap_inline6181 is known and that the corresponding density of states, tex2html_wrap_inline7129 , is constant. The second and third terms describe electrons in the narrow d band and the transfer between the two bands, respectively. There are tex2html_wrap_inline7133 states in the narrow band for each spin. The last term represents the interaction between the electrons on the d levels; only electrons with opposite spins are allowed to occupy these levels.

The bandwidth corresponding to tex2html_wrap_inline6181 is much larger than the transfer matrix element tex2html_wrap_inline7139 . The Fermi energy tex2html_wrap_inline5147 , tex2html_wrap_inline7143 , and tex2html_wrap_inline7145 are all well within the conduction band.gif

(a) What kind of magnetic behavior is expected for tex2html_wrap_inline6273 , if the number of d electrons is tex2html_wrap_inline7151 ? Discuss what happens to the magnetic properties if tex2html_wrap_inline7143 is less than or greater than tex2html_wrap_inline5147 , and tex2html_wrap_inline7145 is less or greater than tex2html_wrap_inline5147 .

  (b) For tex2html_wrap_inline7161 , the exact and full solution to the problem is not known. However, within the framework of the mean field approximation, we can have some ideas about the behavior of the system. Replace the Anderson Hamiltonian with

  eqnarray3061

and a similar one for the tex2html_wrap_inline6917 spins. Here tex2html_wrap_inline7165 is the expectation value of the tex2html_wrap_inline6917 spin occupation of the d state (the sum is over the occupied states).

  Use the self-consistency condition to calculate the magnitude of the localized moment, tex2html_wrap_inline7171 as a function of tex2html_wrap_inline7173 and tex2html_wrap_inline7175 , where tex2html_wrap_inline7177 .

Hint: Search for the solution in the form of tex2html_wrap_inline7179 with the normalization condition tex2html_wrap_inline7181 . The expectation value tex2html_wrap_inline7183 can be converted to an energy integral: tex2html_wrap_inline7185 , where g(E) is the density of states, determined by solving Eq. 9.12.

 


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Next: Solutions to Problems Up: Interactions and Phase Transitions Previous: Problem: Fermi Surface Nesting

This document can be accessed on the World Wide Web at "http//:solidstate.physics.sunysb.edu/book/prob/ ".

Laszlo Mihaly
Thu Oct 31 13:23:11 EST 1996


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