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超紫外天文光谱仪校准,使用来自纳米光子酸波导的激光频率
Markus Ludwig1, Furkan Ayhan2, Tobias M Schmidt3
1Deutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607, Hamburg, Germany.
Nature communications
|September 2, 2024
概括
天文学家现在可以使用紫外线激光频率子进行精确的光谱仪校准. 这一突破使得在寻找外星生命和宇宙学方面的新发现成为可能.
科学领域:
- 天文学 天文学
- 频谱学是一种光谱学.
- 光子学是指光子学的使用方法.
背景情况:
- 天文学光谱对于系外行星研究,宇宙学和测试物理常数至关重要.
- 激光频率 (星际) 为天文光谱仪提供高精度校准.
- 由于材料分散和光谱分离,将星际校准扩展到400nm以下的紫外线 (UV) 光谱是具有挑战性的.
研究的目的:
- 为了展示使用激光频率笔在紫外线光谱范围内进行天文光谱仪校准.
- 为了克服UV星际开发的挑战,用于宇宙学应用.
主要方法:
- 利用芯片集成的高度非线性光子学在周期性极点,纳米制造的酸波导中.
- 使用了一台强大的红外电光发电机.
- 集成了一个基于芯片的微共振器子用于UV发电.
主要成果:
- 成功证明了400nm以下的紫外线星际校准.
- 展示了集成光子学用于生成紫外线激光频率的使用.
- 验证了UV天文光谱学的可行方法.
结论:
- 这项工作为紫外线中精确的天文光谱学提供了途径.
- 开发的紫外线星际技术可以增强下一代基于地面和基于太空的天文仪器.
- 它为探测系外行星和宇宙学研究提供了新的可能性.
相关概念视频
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material, molecules absorb light depending on the energy required for electronic transitions. As a result...
UV–Vis Spectrometers
The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell. Samples for...

