# Synergetic effect of spin-orbit coupling and Zeeman splitting on the   optical conductivity in the one-dimensional Hubbard model

**Authors:** Adrien Bolens, Hosho Katsura, Masao Ogata, Seiji Miyashita

arXiv: 1704.03153 · 2017-06-14

## TL;DR

This paper investigates how spin-orbit coupling and Zeeman splitting together influence the optical conductivity in a one-dimensional Hubbard model, revealing conditions for electric dipole spin resonance and effects of electron interactions.

## Contribution

It provides a detailed analysis of the combined effects of SOC and ZS on optical properties, including analytical and numerical results for different interaction regimes.

## Key findings

- EDSR occurs only when both SOC and ZS are present.
- Resonance is enhanced at small U and suppressed at large U.
- Magnetic field suppresses resonance, but SOC can recover it depending on the angle.

## Abstract

We study how the synergetic effect of spin-orbit coupling (SOC) and Zeeman splitting (ZS) affects the optical conductivity in the one-dimensional Hubbard model using the Kubo formula. We focus on two phenomena: (1) the electric dipole spin resonance (EDSR) in the metallic regime and (2) the optical conductivity in the Mott-insulating phase above the optical gap. In both cases, we calculate qualitatively the effects of SOC and ZS and how they depend on the relative angle between the SOC vector and the magnetic field direction. First, we investigate the spin resonance without electron correlation (the Hubbard parameter $U=0$). Although, neither SOC nor ZS causes any resonance by itself in the optical conductivity, the EDSR becomes possible when both of them exist. The resulting contribution to the optical conductivity is analyzed analytically. The effect of $U$ on the spin resonance is also studied with a numerical method. It is found that at half-filling, the resonance is first enhanced for small $U$ and then suppressed when the optical gap is large enough. In the strong coupling limit $U \rightarrow \infty$ at half-filling, we also refer to the resonance between the lower and upper Hubbard bands appearing at $\omega \sim U$, above the optical gap. A large magnetic field tends to suppress the signal while it is recovered thanks to SOC depending on the relative angle of the magnetic field.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1704.03153/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1704.03153/full.md

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Source: https://tomesphere.com/paper/1704.03153