First-Principles Calculation of Spin-Relaxation Due to Alloy and Electron-Phonon Scattering in Strained GeSn
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arXiv
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| Format: | Preprint |
| Publié: |
2025
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| _version_ | 1866908365434650624 |
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| author | Sewell, Kevin Murphy-Armando, Felipe |
| author_facet | Sewell, Kevin Murphy-Armando, Felipe |
| contents | GeSn has emerged as a promising material for spintronics due to its long spin-lifetime, compatibility with silicon technology, high mobility and tunable electronic properties. Of particular interest is the transition from an indirect to a direct band gap with increasing Sn content, which enhances optical properties, electron transport and we find also affects spin transport behaviour, which is critical for spintronics applications. We use first-principles electronic-structure theory to determine the spin-flip electron-alloy scattering parameters in n-type GeSn alloys. We also calculate the previously undetermined intervalley electron spin-phonon scattering parameters between the $L$ and $Γ$ valleys. These parameters are used to determine the electron-alloy and electron-phonon scattering contributions to the n-type spin-relaxation of GeSn, as a function of alloy content and temperature. As in the case of phonon scattering, alloy scattering reduces the spin-relaxation time. However, switching the spin transport from the typical $L$ valley of Ge to the $Γ$ valley by sufficient addition of Sn, the relaxation time can be substantially increased. For unstrained, room temperature GeSn, we find a Sn concentration of at least $10\%$ is required to achieve a spin-relaxation time greater than Ge, with $17\%$ Sn needed to increase the spin-relaxation time from the nanosecond range to the microsecond range. At low temperatures (30K), adding $10\%$ Sn can increase the spin-relaxation time from $10^{-7}$s to 0.1s. Applying biaxial tensile strain to GeSn further increases the spin-relaxation time and at a lower Sn content than in unstrained GeSn. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_10350 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | First-Principles Calculation of Spin-Relaxation Due to Alloy and Electron-Phonon Scattering in Strained GeSn Sewell, Kevin Murphy-Armando, Felipe Materials Science GeSn has emerged as a promising material for spintronics due to its long spin-lifetime, compatibility with silicon technology, high mobility and tunable electronic properties. Of particular interest is the transition from an indirect to a direct band gap with increasing Sn content, which enhances optical properties, electron transport and we find also affects spin transport behaviour, which is critical for spintronics applications. We use first-principles electronic-structure theory to determine the spin-flip electron-alloy scattering parameters in n-type GeSn alloys. We also calculate the previously undetermined intervalley electron spin-phonon scattering parameters between the $L$ and $Γ$ valleys. These parameters are used to determine the electron-alloy and electron-phonon scattering contributions to the n-type spin-relaxation of GeSn, as a function of alloy content and temperature. As in the case of phonon scattering, alloy scattering reduces the spin-relaxation time. However, switching the spin transport from the typical $L$ valley of Ge to the $Γ$ valley by sufficient addition of Sn, the relaxation time can be substantially increased. For unstrained, room temperature GeSn, we find a Sn concentration of at least $10\%$ is required to achieve a spin-relaxation time greater than Ge, with $17\%$ Sn needed to increase the spin-relaxation time from the nanosecond range to the microsecond range. At low temperatures (30K), adding $10\%$ Sn can increase the spin-relaxation time from $10^{-7}$s to 0.1s. Applying biaxial tensile strain to GeSn further increases the spin-relaxation time and at a lower Sn content than in unstrained GeSn. |
| title | First-Principles Calculation of Spin-Relaxation Due to Alloy and Electron-Phonon Scattering in Strained GeSn |
| topic | Materials Science |
| url | https://arxiv.org/abs/2505.10350 |