Abstract

We explore the effect of the imaginary part of the self-energy, ImΣ(k,ω)Im\Sigma(\vec{k},\omega), having a single pole, Ω(k,ω)\Omega(\vec{k},\omega), with spectral weight, α(k)\alpha(\vec{k}), and quasi-particle lifetime, Γ(k)\Gamma(\vec{k}), on the density of states. We solve the set of parameters, Ω(k,ω\Omega(\vec{k},\omega), α(k)\alpha(\vec{k}), and Γ(k)\Gamma(\vec{k}) by means of the moment approach (exact sum rules) of Nolting. Our choice for Σ(k,ω)\Sigma(k,\omega), satisfies the Kramers - Kronig relationship automatically. Due to our choice of the self - energy, the system is not a Fermi liquid for any value of the interaction, a result which is also true in the moment approach of Nolting without lifetime effects. By increasing the value of the local interaction, U/WU/W, at half-filling (ρ=1/2\rho = 1/2), we go from a paramagnetic metal to a paramagnetic insulator, (Mott metal - insulator transition (MMITMMIT)) for values of U/WU/W of the order of U/W1U/W \geq 1 (WW is the band width) which is in agreement with numerical results for finite lattices and for infinity dimensions (D=D = \infty). These results settle down the main weakness of the spherical approximation of Nolting: a finite gap for any finite value of the interaction, i.e., an insulator for any finite value of U/WU/W. Lifetime effects are absolutely indispensable. Our scheme works better than the one of improving the narrowing band factor, B(k)B(\vec{k}), beyond the spherical approximation of Nolting.Comment: 5 pages and 5 ps figures (included

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    Last time updated on 02/01/2020