Transverse instability and universal decay of spin spiral order in the Heisenberg model

We analyze the intrinsic stability of spin spiral states in the two-dimensional Heisenberg model isolated from its environment. Our analysis reveals that the SU(2) symmetric point hosts a dynamic instability that is enabled by the existence of energetically favorable transverse deformations-both in real and spin space-of the spiral order. The instability is universal in the sense that it applies to systems with any spin number, spiral wave vector, and spiral amplitude. Unlike the Landau or modulational instabilities which require impurities or periodic potential modulation of an optical lattice, quantum fluctuations alone are sufficient to trigger the transverse instability. We analytically find the most unstable mode and its growth rate, and compare our analysis with phase-space methods. By adding an easy-plane exchange coupling that reduces the Hamiltonian symmetry from SU(2) to U(1), the stability boundary is shown to continuously interpolate between the modulational instability and the transverse instability. This suggests that the transverse instability is an intrinsic mechanism that hinders long-range phase coherence even in the presence of exchange anisotropy.

Automated summary

In this study, we analyze the intrinsic stability of spin spiral states in the two-dimensional Heisenberg model. We find that the SU(2) symmetric point exhibits a dynamic instability caused by energetically favorable transverse deformations in both real and spin space of the spiral order. This instability is universal and applies to systems with any spin number, spiral wave vector, and spiral amplitude. Unlike traditional Landau or modulational instabilities, this instability can be triggered solely by quantum fluctuations. By introducing an easy-plane exchange coupling, we show that the stability boundary continuously interpolates between the modulational instability and the transverse instability.