High temperature non-collinear magnetism in a classical bilinear-biquadratic Heisenberg model
Kanika Pasrija, Sanjeev Kumar

TL;DR
This study demonstrates that non-collinear magnetism at high temperatures in CuO can be explained by a classical spin model with biquadratic interactions, without requiring lattice distortions or inversion symmetry breaking.
Contribution
It introduces a classical bilinear-biquadratic Heisenberg model that explains high-temperature non-collinear magnetism in CuO through pure spin interactions.
Findings
Biquadratic coupling influences magnetic ground state selection.
Non-collinear magnetic states are stable at finite temperatures.
Inhomogeneous spiral phase stabilized by entropic effects.
Abstract
Motivated by the magnetically-driven high-temperature ferroelectric behavior of CuO and the subsequent theoretical efforts to understand this intriguing phenomenon, we study a spin model on a two-dimensional square lattice which possesses some of the key features of the models proposed for CuO. The model consists of Heisenberg couplings between nearest and next-nearest neighbor spins, and biquadratic couplings between nearest neighbors. We use a combination of variational calculations and classical Monte Carlo simulations to study this model at zero and finite temperatures. We show that even an arbitrarily weak biquadratic coupling plays a crucial role in selecting the magnetic ground state. More importantly, a non-collinear magnetic state, characterized by a finite spin current, is stable at finite temperatures. The interesting aspect is that the present model neither includes an…
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