Evolution of single-particle green functions with correlation in the hubbard model at half-filling: sum rules for the spectral density

1999 ◽  
Vol 259-261 ◽  
pp. 773-774
Author(s):  
J.J Rodrı́guez-Núñez ◽  
S Schafroth ◽  
H Beck
1995 ◽  
Vol 52 (4) ◽  
pp. 2463-2470 ◽  
Author(s):  
B. Mehlig ◽  
H. Eskes ◽  
R. Hayn ◽  
M. B. J. Meinders

2008 ◽  
Vol 154 (1) ◽  
pp. 52-63 ◽  
Author(s):  
Yu. A. Izyumov ◽  
N. I. Chashchin
Keyword(s):  

1995 ◽  
Vol 51 (19) ◽  
pp. 13774-13777 ◽  
Author(s):  
A. A. Aligia ◽  
Liliana Arrachea ◽  
E. R. Gagliano

2007 ◽  
Vol 460-462 ◽  
pp. 248-251
Author(s):  
Werner Hanke ◽  
Markus Aichhorn ◽  
Enrico Arrigoni ◽  
Michael Potthoff

1997 ◽  
Vol 08 (05) ◽  
pp. 1145-1158
Author(s):  
J. J. Rodríguez-Núñez ◽  
S. Schafroth

We implement the numerical method of summing Green function diagrams on the Matsubara frequency axis for the fluctuation exchange (FLEX) approximation. Our method has previously been applied to the attractive Hubbard model for low density. Here we apply our numerical algorithm to the Hubbard model close to half filling (ρ =0.40), and for T/t = 0.03, in order to study the dynamics of one- and two-particle Green functions. For the values of the chosen parameters we see the formation of three branches which we associate with the two-peak structure in the imaginary part of the self-energy. From the imaginary part of the self-energy we conclude that our system is a Fermi liquid (for the temperature investigated here), since Im Σ( k , ω) ≈ w2 around the chemical potential. We have compared our fully self-consistent FLEX solutions with a lower order approximation where the internal Green functions are approximated by free Green functions. These two approches, i.e., the fully self-consistent and the non-self-consistent ones give different results for the parameters considered here. However, they have similar global results for small densities.


1989 ◽  
Vol 40 (13) ◽  
pp. 8939-8944 ◽  
Author(s):  
P. W. Anderson ◽  
B. S. Shastry ◽  
D. Hristopulos

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