# Enhanced nematic fluctuations near an antiferromagnetic Mott insulator   and possible application to high-$T_{c}$ cuprates

**Authors:** Peter P. Orth, Bhilahari Jeevanesan, Rafael M. Fernandes, J\"org, Schmalian

arXiv: 1703.02210 · 2019-04-24

## TL;DR

This paper explores how nematic fluctuations are enhanced near a Mott insulator with antiferromagnetic order, suggesting a link to nematicity observed in underdoped cuprate superconductors, through strong-coupling models and simulations.

## Contribution

It introduces a strong-coupling model including Cu-$d$ and O-$p$ orbitals that reveals biquadratic spin interactions leading to nematic fluctuations, a novel mechanism for nematicity in cuprates.

## Key findings

- Biquadratic coupling favors stripe-like magnetic fluctuations.
- Enhanced nematic susceptibility appears at a temperature scale set by $J$.
- Implications for magnetic spectrum and nematicity in cuprates.

## Abstract

Motivated by the widespread experimental observations of nematicity in strongly underdoped cuprate superconductors, we investigate the possibility of enhanced nematic fluctuations in the vicinity of a Mott insulator that displays N\'eel-type antiferromagnetic order. By performing a strong-coupling expansion of an effective model that contains both Cu-$d$ and O-$p$ orbitals on the square lattice, we demonstrate that quadrupolar fluctuations in the $p$-orbitals inevitably generate a biquadratic coupling between the spins of the $d$-orbitals. The key point revealed by our classical Monte Carlo simulations and large-$N$ calculations is that the biquadratic term favors local stripe-like magnetic fluctuations, which result in an enhanced nematic susceptibility that onsets at a temperature scale determined by the effective Heisenberg exchange $J$. We discuss the impact of this type of nematic order on the magnetic spectrum and outline possible implications on our understanding of nematicity in the cuprates.

## Full text

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## Figures

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## References

49 references — full list in the complete paper: https://tomesphere.com/paper/1703.02210/full.md

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Source: https://tomesphere.com/paper/1703.02210