经典和量子光学 skyrmions 在大气流中的拓强度
Zhenyu Guo1, Cade Peters2, Nilo Mata-Cervera1
1Centre for Disruptive Photonic Technologies, School of Physical and Mathematical Sciences, Nanyang Technological University, Singapore, Singapore.
Nature communications
|January 27, 2026
概括
经典和量子光学 skyrmions 在模拟的大气流中表现出了显著的拓弹性. 它们的固有结构确保了强大的信息传输,克服了复杂介质的退化挑战,用于先进的通信系统.
科学领域:
- 量子光学就是量子光学.
- 复杂媒体物理学的复杂媒体物理
- 拓式光子学 拓式光子学
背景情况:
- 结构光在复杂的介质 (如大气流) 中的降解阻碍了通信,能源运输,成像和传感方面的应用.
- 无论是经典的还是量子的光学 skyrmions,都提供了独特的拓性质,可以抵抗这种降解.
研究的目的:
- 通过模拟的大气流传输时,研究经典和量子光学 skyrmions 的拓弹性.
- 探索这些结构在杂环境中强大的信息传输的潜力.
主要方法:
- 构建经典和量子光学天体.
- 通过实验模拟的大气流传输这些天体.
- 在传输前后分析拓特征和结构完整性.
- 支持分析和数值建模.
主要成果:
- 经典和量子光学 skyrmions 显示保存的拓特征,尽管其他属性的显著扭曲和退化 (例如,光子纠,矢量结构).
- 非局部量子 skyrmions中的量子纠迅速降解,但它们的拓结构保持稳定.
- 当地古典天体的拓结构在广泛的流强度范围内得到保留.
结论:
- 由于不可分离性和片面通道特性,古典和量子 skyrmions 的拓行为在杂的环境中是相当的.
- 这种拓弹性使信息传输能够稳定,为弹性地面和卫星到地面通信系统铺平了道路.
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