# Sub-$\mu$eV Decoherence-Induced Population Pulsation Resonances in an   InGaN system

**Authors:** Cameron Nelson, Yong-Ho Ra, Zetian Mi, Paul Berman, Duncan G. Steel

arXiv: 1705.10782 · 2017-09-13

## TL;DR

This study reveals that decoherence causes population pulsation resonances in InGaN nanowires at room temperature, with high spectral resolution showing asymmetric lineshapes and estimating decoherence times around 125 fs.

## Contribution

It demonstrates that decoherence-induced population pulsations produce narrow resonances in InGaN systems, with quantitative analysis of decoherence times using optical Bloch equations.

## Key findings

- Decoherence time of 125 fs estimated from lineshape analysis
- Resonances originate from coherent population pulsations
- Lineshapes fit well with optical Bloch equations, indicating discrete levels

## Abstract

We report on high frequency resolution coherent nonlinear optical spectroscopy on an ensemble of InGaN disks in GaN nanowires at 300 K. Sub-$\mu$eV resonances in the inhomogeneously broadened third order ($\chi^{(3)}$) absorption spectrum show asymmetric line shapes, where the degree of asymmetry depends on the wavelength of the excitation beams. Theory based on the Optical Bloch Equations (OBE) indicates that the lineshape asymmetry is a result of fast decoherence in the system and the narrow resonances originate from coherent population pulsations that are induced by decoherence in the system. Using the OBE, we estimate that the decoherence time of the optically induced dipole (formed between the unexcited ground state the excited electron-hole pair) at room temperature is 125 fs, corresponding to a linewidth of ~10 meV. The decay time of the excitation is ~5-10 ns, depending on the excitation energy. The lineshapes are well fit with the OBE indicating that the resonances are characterized by discrete levels with no evidence of many body physics.

## Full text

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## Figures

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## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1705.10782/full.md

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Source: https://tomesphere.com/paper/1705.10782