Nature of ground states in one-dimensional electron-phonon Hubbard models at half filling
The renormalization group technique is applied to one-dimensional electron-phonon Hubbard models at half filling and zero temperature. For the Holstein-Hubbard model, the results of one-loop calculations are congruent with the phase diagram obtained by quantum Monte Carlo simulations in the (U, g su...
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Veröffentlicht in: | Physical review. B, Condensed matter and materials physics Condensed matter and materials physics, 2015-02, Vol.91 (8), Article 085114 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The renormalization group technique is applied to one-dimensional electron-phonon Hubbard models at half filling and zero temperature. For the Holstein-Hubbard model, the results of one-loop calculations are congruent with the phase diagram obtained by quantum Monte Carlo simulations in the (U, g sub(ph)) plane for the phonon-mediated interaction g sub(ph) and the Coulomb interaction U. The incursion of an intermediate phase between a fully gapped charge-density-wave state and a Mott antiferromagnet is supported along with the growth of its size with the molecular phonon frequency omega sub(0). We find additional phases enfolding the base boundary of the intermediate phase. A Luttinger liquid line is found below some critical U* approximately g* sub(ph), followed at larger U ~ g sub(ph) by a narrow region of bond-order-wave ordering which is either charge or spin gapped depending on U. For the Peierls-Hubbard model, the region of the (U, g sub(ph)) plane with a fully gapped Peierls-bond-order-wave state shows a growing domination over the Mott gapped antiferromagnet as the Debye frequency omega D decreases. A power-law dependence g sub(ph) ~ U super(2)[eta] is found to map out the boundary between the two phases, whose exponent is in good agreement with the existing quantum Monte Carlo simulations performed when a finite nearest-neighbor repulsion term V is added to the Hubbard interaction. |
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ISSN: | 1098-0121 1550-235X |
DOI: | 10.1103/PhysRevB.91.085114 |