# Phonon-assisted magnetic Mott-insulating state in the charge density   wave phase of single-layer 1TNbSe2

**Authors:** Matteo Calandra

arXiv: 1803.08361 · 2018-07-18

## TL;DR

This study reveals that single-layer 1TNbSe2 exhibits a phonon-assisted magnetic Mott-insulating state within its charge density wave phase, driven by electron correlations and lattice distortions, as shown by first-principles calculations.

## Contribution

It demonstrates the stabilization of a magnetic Mott insulator in 1TNbSe2 due to Hubbard interactions and lattice effects, providing new insights into correlated phases in 2D materials.

## Key findings

- Charge density wave with specific periodicity matches experimental data.
- Hubbard U induces a magnetic Mott insulating state.
- Lattice distortion enhances the Mott gap and magnetic properties.

## Abstract

We study the structural, electronic and vibrational properties of single-layer 1TNbSe$_2$ from first principles. Within the generalized gradient approximation, the 1T polytype is highly unstable with respect to the 2H. The DFT+U method improves the stability of the 1T phase, explaining its detection in experiments. A charge density wave occurs with a $\sqrt{13}\times\sqrt{13}~R30^{\circ}$ periodicity, in agreement with STM data. At $U=0$, the David-star reconstruction displays a flat band below the Fermi level with a marked d$_{z^2-r^2}$ orbital character of the central Nb. The Hubbard interaction induces a magnetic Mott insulating state. Magnetism distorts the lattice around the central Nb atom in the star, reduces the hybridization between the central Nb d$_{z^2-r^2}$ orbital and the neighbouring Se p-states and lifts in energy the flat band becoming non-bonding. This cooperative lattice and magnetic effect amplifies the Mott gap. Single-layer 1TNbSe$_2$ is then a phonon-assisted spin-$1/2$ Magnetic Mott insulator.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1803.08361/full.md

## References

31 references — full list in the complete paper: https://tomesphere.com/paper/1803.08361/full.md

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Source: https://tomesphere.com/paper/1803.08361