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Quantum Christoffel Nonlinear Magnetization

Xiao-Bin Qiang, Xiaoxiong Liu, Hai-Zhou Lu, X. C. Xie

Abstract

The Christoffel symbol is an essential quantity in Einstein's general theory of relativity. We discover that an electric field can induce a nonlinear magnetization in quantum materials, described by a Christoffel symbol defined in the Hilbert space of quantum states (quantum Christoffel symbol). Quite different from the previous scenarios, this orbital magnetization does not need spin-orbit coupling and inversion symmetry breaking. Through symmetry analysis and first-principles calculations, we identify a number of point groups and 2D material candidates (e.g., BiF$_3$, ZnI$_2$, and Ru$_4$Se$_5$) that host this quantum Christoffel nonlinear magnetization. More importantly, this nonlinear magnetization allows the quantum Christoffel symbol to be probed by optical techniques such as magneto-optical Kerr spectroscopy or transport measurements such as tunneling magneto-resistance. This quantum Christoffel nonlinear magnetization gives a paradigm of how geometry dictates physics.

Quantum Christoffel Nonlinear Magnetization

Abstract

The Christoffel symbol is an essential quantity in Einstein's general theory of relativity. We discover that an electric field can induce a nonlinear magnetization in quantum materials, described by a Christoffel symbol defined in the Hilbert space of quantum states (quantum Christoffel symbol). Quite different from the previous scenarios, this orbital magnetization does not need spin-orbit coupling and inversion symmetry breaking. Through symmetry analysis and first-principles calculations, we identify a number of point groups and 2D material candidates (e.g., BiF, ZnI, and RuSe) that host this quantum Christoffel nonlinear magnetization. More importantly, this nonlinear magnetization allows the quantum Christoffel symbol to be probed by optical techniques such as magneto-optical Kerr spectroscopy or transport measurements such as tunneling magneto-resistance. This quantum Christoffel nonlinear magnetization gives a paradigm of how geometry dictates physics.
Paper Structure (1 section, 18 equations, 3 figures, 2 tables)

This paper contains 1 section, 18 equations, 3 figures, 2 tables.

Table of Contents

  1. End Matter

Figures (3)

  • Figure 1: In Einstein's general relativity, the Christoffel symbol $\Gamma_{ij}^k$ describe how basis vectors $\boldsymbol{e}_i$ transform across the coordinates $\boldsymbol{x}$ of the curved spacetime. We find a nonlinear magnetization $\mathbf{M}$ in response to an electric field $\mathbf{E}$ can be described by a quantum Christoffel symbol $\boldsymbol{\Gamma}$ in momentum space ($k_x$-$k_y$), in terms of $\mathbf{M}\propto \mathbf{E} \mathbf{E} \int \boldsymbol{\Gamma}$. A heuristic picture is as follows. One role of the electric field $\mathbf{E}$ is to induce a curved quantum space, described by $\boldsymbol{\Gamma}$. The other role of $\mathbf{E}$ is to drive a "loop current" of electron orbital motion in the curved quantum space, leading to the magnetization $\mathbf{M}$ that is quadratic in $\mathbf{E}$.
  • Figure 2: (a) Lattice structure of the 2D BiF$_3$ grown along the [001] crystallographic direction. (b) Band structure of the 2D BiF$_3$ along the high symmetry line with and without spin-orbit coupling (SOC). (c) First-principles calculation results of the nonlinear magnetization coefficient $\alpha_{zxx}$ as a function of the Fermi energy $\varepsilon_F$, by using Eq. (\ref{['Eq: alpha_full']}) (with and without SOC) and also with the Haldane-like perturbation $\mathcal{H}'$ Eq. (\ref{['Eq: Hp']}) ($t'$ = 2 meV), respectively. In the calculation with $\mathcal{H}'$, the hopping parameter $t'$ = 2 meV, relaxation time $\tau$ = 100 ps, and additional electric field $\mathbf{E}$ = 0.02 V/$\mu$m. (d) First-principles calculation results of $\alpha_{zxx}$ as a function of the Fermi energy $\varepsilon_F$, by using Eq. (\ref{['Eq: alpha_CS']}) (Christoffel) and Eq. (\ref{['Eq: alpha_full']}) (Total), respectively. The non-Christoffel contribution is much smaller than the contribution described by the quantum Christoffel symbol. (e) Kerr rotation angle $\theta_\text{K}$ as a function of photon energy $\hbar \omega$, at Fermi level -0.25 eV and -0.10 eV, respectively. The Kerr angle measures how much a linearly polarized light is rotated after being reflected from the sample and is a direct probe of magnetization.
  • Figure 3: Nonlinear magnetization coefficient $\alpha_{zxx}$ for the effective model [Eq. \ref{['Eq: model']}]. (a) $\alpha_{zxx}$ as a function of the Fermi energy $\varepsilon_F$ without particle-hole symmetry ($\lambda = 0.5$ eV$\cdot$nm$^2$), for the contribution from the quantum Christoffel nonlinear magnetization and non-Christoffel contribution. (b) $\alpha_{zxx}$ as a function of the particle-hole symmetry breaking parameter $\lambda$ at $\varepsilon_F = 0.2$ eV and $t = 0.9$ eV$\cdot$nm$^2$. (c) $\alpha_{zxx}$ as a function of $\varepsilon_F$ for the particle-hole symmetric case ($\lambda = 0$) at several values of $t$, which breaks the $\mathcal{C}_{x,y}^2$ rotational and $\mathcal{M}_{x,y}$ mirror reflection symmetries. (d) $\alpha_{zxx}$ as a function of $t$ at $\lambda = 0$ and $\varepsilon_F = 0.2$, 0.3, and 0.4 eV. Insets in (a) and (c) compare the band structures without and with particle-hole symmetry, respectively. Other model parameters are $v = 1$ eV$\cdot$nm and $m = 0.1$ eV.