# Experimental Characterization of Ultrafast, Tunable and Broadband   Optical Kerr Nonlinearity in Graphene

**Authors:** Siddharatha Thakur, Behrooz Semnani, Safieddin Safavi-Naeini, Amir, Hamed Majedi

arXiv: 1903.07241 · 2019-10-15

## TL;DR

This paper systematically measures and characterizes the ultrafast, tunable, and broadband optical Kerr nonlinearity in graphene, revealing its spectral, temporal, and pulse-width dependencies in the near-infrared regime.

## Contribution

It provides a comprehensive experimental and theoretical analysis of graphene's Kerr nonlinearity, including spectral dependence, temporal dynamics, and pulse-width effects, with quantum theory validation.

## Key findings

- Kerr coefficient $n_{2,eff}$ scales with wavelength squared
- Nonlinear response peaks at zero delay and relaxes on carrier timescales
- Kerr nonlinearity remains positive across conditions

## Abstract

In this study we systematically measure the near-infrared spectral dependence, the sub-picosecond temporal evolution and pulse-width dependence of the effective Kerr coefficient ($n_{2,eff}$) of graphene in hundreds of femtosecond regime. The spectral dependence measured using the Z-scan technique is corroborated by quantum theory to extract a $n_{2,eff} \propto \lambda^2$ dependence. The temporal evolution extracted using the time-resolved Z-scan measurement shows the nonlinear response peaking at zero delay time and relaxing on a time scale of carrier relaxation. Since the Kerr-type response originated from the optically induced carrier population difference, the time-scale of the evolution of the nonlinear response is apt. The $n_{2,eff}$ shows a dependence on the pulse-width attributed to the relative heating and cooling times of the carriers. This dependence is strong when the pulse-duration is on the same time-scale as the decay constant. Throughout our study the $n_{2,eff}$ remains positive.

## Full text

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## Figures

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## References

33 references — full list in the complete paper: https://tomesphere.com/paper/1903.07241/full.md

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Source: https://tomesphere.com/paper/1903.07241