# Magnetic phase diagram of the infinite-U Hubbard model with nearest- and   next nearest-neighbor hoppings

**Authors:** G. G. Blesio, M. G. Gonzalez, F. T. Lisandrini

arXiv: 1905.05838 · 2019-05-16

## TL;DR

This study maps the magnetic phases of the infinite-U Hubbard model with various hoppings, revealing how next-nearest neighbor interactions influence ferromagnetism and phase stability across different electron densities.

## Contribution

It provides the first detailed phase diagram showing the effects of next-nearest neighbor hopping on magnetic states in the Hubbard model.

## Key findings

- Next-nearest neighbor hopping stabilizes ferromagnetism up to |t'/t|=0.5.
- Fully spin-polarized states connect Nagaoka ferromagnetism to low-density itinerant ferromagnetism.
- Checkerboard insulator phase at t'=0 and ρ=0.75 is destabilized by t'.

## Abstract

We study the infinite-U Hubbard model on ladders of 2, 4 and 6 legs with nearest (t) and next-nearest (t') neighbor hoppings by means of the density-matrix renormalization group algorithm. In particular, we analyze the stability of the Nagaoka state for several values of t' when we vary the electron density $(\rho)$ from half-filling to the low-density limit. We build the two-dimensional phase diagram, where the fully spin-polarized and paramagnetic states prevail. We find that the inclusion of a non-frustrating next nearest neighbor hopping stabilizes the fully spin-polarized phase up until |t'/t|=0.5. Surprisingly, for this value of t', the ground state is fully spin-polarized for almost any electron density 1 $\gtrsim \rho \gtrsim$ 0, connecting the Nagaoka state to itinerant ferromagnetism at low density. Also, we find that the previously found checkerboard insulator phase at t'=0 and $\rho$=0.75 is unstable against t'.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1905.05838/full.md

## References

37 references — full list in the complete paper: https://tomesphere.com/paper/1905.05838/full.md

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Source: https://tomesphere.com/paper/1905.05838