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      Optimum ground states of generalized Hubbard models with next-nearest neighbour interaction

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          Abstract

          We investigate the stability domains of ground states of generalized Hubbard models with next-nearest neighbour interaction using the optimum groundstate approach. We focus on the \(\eta\)-pairing state with momentum P=0 and the fully polarized ferromagnetic state at half-filling. For these states exact lower bounds for the regions of stability are obtained in the form of inequalities between the interaction parameters. For the model with only nearest neighbour interaction we show that the bounds for the stability regions can be improved by considering larger clusters. Additional next-nearest neighbour interactions can lead to larger or smaller stability regions depending on the parameter values.

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          Hubbard model with nearest-neighbor and bond-charge interaction: Exact ground-state solution in a wide range of parameters

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            Rigorous criteria for ferromagnetism in itinerant electron systems

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              \(\eta\)-pairing as a mechanism of superconductivity in models of strongly correlated electrons

              We consider extended versions of the Hubbard model which contain additional interactions between nearest neighbours. In this letter we show that a large class of these models has a superconducting ground state in arbitrary dimensions. In some special cases we are able to find the complete phase diagram. The superconducting phase exist even for moderate repulsive values of the Hubbard interaction \(U\).
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                Author and article information

                Journal
                12 May 1999
                Article
                10.1007/s100510050997
                cond-mat/9905157
                f3eda4bd-8e4d-4d65-82e4-88fb2c7af578
                History
                Custom metadata
                18 pages with 6 figures, LateX2e with BibteX, accepted for publication in Eur. Phys. J. B
                cond-mat.str-el

                Condensed matter
                Condensed matter

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