# Theory of the strongly nonlinear electrodynamic response of graphene: A   hot electron model

**Authors:** S. A. Mikhailov

arXiv: 1908.04631 · 2019-09-18

## TL;DR

This paper develops a hot electron model to analyze the nonlinear electrodynamic response of graphene under strong electromagnetic radiation, providing detailed solutions and comparing with experimental data.

## Contribution

It introduces a hot electron model for graphene's nonlinear response, deriving equations and solutions for various physical quantities under different conditions.

## Key findings

- Absorption coefficient varies with radiation intensity at different frequencies.
- Model predictions agree well with recent experimental data.
- Identifies regimes of increasing and decreasing absorption with intensity.

## Abstract

An electrodynamic response of graphene to a strong electromagnetic radiation is considered. A hot electron model (HEM) is introduced and a corresponding system of nonlinear equations is formulated. Solutions of this system are found and discussed in detail for intrinsic and doped graphene: the hot electron temperature, non-equilibrium electron and holes densities, absorption coefficient and other physical quantities are calculated as functions of the incident wave frequency $\omega$ and intensity $I$, of the equilibrium chemical potential $\mu_0$ and temperature $T_0$, scattering parameters, as well as of the ratio $\tau_\epsilon/\tau_{\rm rec}$ of the intra-band energy relaxation time $\tau_\epsilon$ to the recombination time $\tau_{\rm rec}$. The influence of the radiation intensity on the absorption coefficient $A$ at low ($\hbar\omega\lesssim 2|\mu_0|$, $dA/dI>0$) and high ($\hbar\omega\gtrsim 2|\mu_0|$, $dA/dI<0$) frequencies is studied. The results are shown to be in good agreement with recent experimental data.

## Full text

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## Figures

24 figures with captions in the complete paper: https://tomesphere.com/paper/1908.04631/full.md

## References

91 references — full list in the complete paper: https://tomesphere.com/paper/1908.04631/full.md

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Source: https://tomesphere.com/paper/1908.04631