# Magnetic oscillations of in-plane conductivity in quasi-two-dimensional   metals

**Authors:** T. I. Mogilyuk, P. D. Grigoriev

arXiv: 1901.09064 · 2019-01-29

## TL;DR

This paper develops a theoretical framework for understanding magnetic oscillations in the in-plane conductivity of layered quasi-2D metals, providing analytical expressions and analyzing their behavior under various conditions.

## Contribution

The paper introduces a new analytical approach to describe magnetic quantum oscillations and slow oscillations in in-plane conductivity of quasi-2D metals, including phase and amplitude analysis.

## Key findings

- MQO and SlO have opposite phase in weak magnetic fields
- Amplitude of SlO changes sign at a specific cyclotron frequency condition
- Differences between in-plane and out-of-plane conductivity oscillations are identified

## Abstract

We develop the theory of transverse magnetoresistance in layered quasi-two-dimensional metals. Using the Kubo formula and harmonic expansion, we calculate intralayer conductivity in a magnetic field perpendicular to conducting layers. The analytical expressions for the amplitudes and phases of magnetic quantum oscillations (MQO) and of the so-called slow oscillations (SlO) are derived and applied to analyze their behavior as a function of several parameters: magnetic field strength, interlayer transfer integral and the Landau-level width. Both the MQO and SlO of intralayer and interlayer conductivities have approximately opposite phase in weak magnetic field and the same phase in strong field. The amplitude of SlO of intralayer conductivity changes sign at $\omega_c\tau_0=\sqrt{3}$. There are several other qualitative difference between magnetic oscillations of in-plane and out-of-plane conductivity. The results obtained are useful to analyze experimental data on magnetoresistance oscillations in various strongly anisotropic quasi-2D metals.

## Full text

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## Figures

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## References

65 references — full list in the complete paper: https://tomesphere.com/paper/1901.09064/full.md

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Source: https://tomesphere.com/paper/1901.09064