High Resolution IR-Cavity Ringdown Spectroscopy on Reactive Gas-phase Species

反应气相物质的高分辨率红外腔衰荡光谱

• 批准号: 326572190
• 负责人: Dr. Guido Fuchs
• 金额: --
• 依托单位: Institut für Physik
• 依托单位国家: 德国
• 项目类别: Research Grants
• 财政年份: 2017
• 资助国家: 德国
• 起止时间: 2016-12-31 至 2022-12-31
• 项目状态: 已结题
• 来源: https://gepris.dfg.de/gepris/projekt/326572190?language=en
• 关键词: Resolution; IR; Cavity; Ringdown; Spectroscopy

There is a surprisingly rich chemistry to be found in different regions in outer space. For example, in the vicinity of dying stars atoms combine to molecules and serve as seed material for dust formation (e.g. silicon carbides). Unlike on earth, interstellar molecules are very often non-saturated compounds that are highly reactive or even of ionic nature (like ionic complexes of hydrogen or noble gases). These species, which are difficult to produce in terrestrial laboratories, are valuable probes to determine the local physical conditions in cosmic environments. Now, with the availability of high-resolution IR instruments on telescopes like EXES/SOFIA and TEXES/N-Gemini a strongly increased demand set in for IR spectroscopic data. In addition, the highly sensitive James Webb space telescope will most likely start already in 2018. Thus, it is now possible to overcome the IR-opaque earthly atmosphere and to view into the mid-IR sky with high resolution astrophysical instruments. It is expected that the already scheduled line surveys will lead to new molecule detections. Specifically species that have no permanent dipole moment and cannot be investigated at radio wavelengths will be new on the list. Many of the expected molecules have characteristic spectra at mid-IR wavelengths. These spectra cannot be calculated by purely theoretical means to the necessary level of precision for astrophysical detections. Without new laboratory measurements the data situation is clearly deficient. The lack of experimental data has several reasons. One difficulty is the production of astrophysically relevant molecules in sufficient abundances, because these species are very reactive and only short-lived. Furthermore, very often adequate light sources for high-resolution mid-IR spectroscopy are missing. The aim of this work is to perform high-resolution and extremely sensitive measurements on astrophysically relevant molecules. Powerful quantum cascade lasers (QCLs) operating above 4.5 mu and OPO systems for the region 2-4.7 mu will be utilized as suitable light sources. These laser systems will be an integral part of the newly to-build highly sensitive cavity-ringdown (CRD) spectrometer. The IR-CRD spectrometer will be combined with special plasma molecule sources (laser ablation/electr. discharge) to produce in-situ high molecule abundances. With the irradiation of microwave radiation double resonance experiments will be feasible which are particularly suitable to investigate molecule plasmas. In practice, it is planned to measure silicon carbides (e.g. Si2C2) and ionic complexes (like [Ar-N2]+).

在外层空间的不同区域可以发现令人惊讶的丰富的化学物质。例如，在垂死的恒星附近，原子联合收割机结合成分子，并作为尘埃形成的种子材料（例如碳化硅）。与地球不同，星际分子通常是高度反应性的不饱和化合物，甚至具有离子性质（如氢或稀有气体的离子复合物）。这些物种很难在陆地实验室中产生，是确定宇宙环境中当地物理条件的宝贵探针。现在，随着EXES/索菲亚和TEXES/N-Gemini等望远镜上高分辨率红外仪器的可用性，对红外光谱数据的需求大幅增加。此外，高灵敏度的詹姆斯·韦伯太空望远镜很可能将于2018年启动。因此，现在有可能克服红外不透明的地球大气层，并使用高分辨率天体物理仪器观察中红外天空。预计已经安排的线路调查将导致新的分子检测。特别是那些没有永久偶极矩，无法在无线电波长下研究的物种将是新的。许多预期的分子在中红外波长处具有特征光谱。这些光谱无法通过纯理论手段计算到天体物理探测所需的精确程度。如果没有新的实验室测量数据，数据情况显然是不足的。缺乏实验数据有几个原因。困难之一是产生足够丰度的天体物理相关分子，因为这些物质非常活泼，寿命很短。此外，经常缺少用于高分辨率中红外光谱的足够光源。这项工作的目的是对天体物理学相关分子进行高分辨率和极灵敏的测量。强大的量子级联激光器（QCL）的操作以上4.5亩和OPO系统的区域2-4.7亩将被用作合适的光源。这些激光系统将成为新建成的高灵敏度腔衰荡（CRD）光谱仪的组成部分。IR-CRD光谱仪将与特殊的等离子体分子源（激光烧蚀/放电）相结合，以产生原位高分子丰度。利用微波辐射进行双共振实验是可行的，特别适合于研究分子等离子体。在实践中，计划测量碳化硅（例如Si 2C 2）和离子络合物（如[Ar-N2]+）。