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UV photoprocessing of CO2 ice: a complete quantification of photochemistry and photon-induced desorption processes

机译:二氧化碳冰的紫外线光处理:对光化学和光子诱导的解吸过程的完整定量

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Context. Ice mantles that formed on top of dust grains are photoprocessed by the secondary ultraviolet (UV) field in cold and dense molecular clouds. UV photons induce photochemistry and desorption of ice molecules. Experimental simulations dedicated to ice analogs under astrophysically relevant conditions are needed to understand these processes. Aims. We present UV-irradiation experiments of a pure CO2 ice analog. Calibration of the quadrupole mass spectrometer allowed us to quantify the photodesorption of molecules to the gas phase. This information was added to the data provided by the Fourier transform infrared spectrometer on the solid phase to obtain a complete quantitative study of the UV photoprocessing of an ice analog. Methods. Experimental simulations were performed in an ultra-high vacuum chamber. Ice samples were deposited onto an infrared transparent window at 8K and were subsequently irradiated with a microwave-discharged hydrogen flow lamp. After irradiation, ice samples were warmed up until complete sublimation was attained. Results. Photolysis of CO2 molecules initiates a network of photon-induced chemical reactions leading to the formation of CO, CO3, O2, and O3. During irradiation, photon-induced desorption of CO and, to a lesser extent, O2 and CO2 took place through a process called indirect desorption induced by electronic transitions, with maximum photodesorption yields (Ypd) of ~1.2 × 10-2 molecules incident photon-1, ~9.3 × 10-4 molecules incident photon-1, and ~1.1 × 10-4 molecules incident photon-1, respectively. Conclusions. Calibration of mass spectrometers allows a direct quantification of photodesorption yields instead of the indirect values that were obtained from infrared spectra in most previous works. Supplementary information provided by infrared spectroscopy leads to a complete quantification, and therefore a better understanding, of the processes taking place in UV-irradiated ice mantles.
机译:上下文。在冷而稠密的分子云中,次级紫外线(UV)场对形成在尘埃颗粒顶部的冰幔进行了光处理。紫外线光子诱导光化学和冰分子的解吸。为了理解这些过程,需要在与天体有关的条件下进行专门用于冰类似物的实验模拟。目的我们介绍了纯CO2冰类似物的紫外线照射实验。通过四极质谱仪的校准,我们可以量化分子在气相中的光解吸。将该信息添加到傅里叶变换红外光谱仪在固相上提供的数据中,以获得对冰类似物的UV光处理的完整定量研究。方法。在超高真空室中进行了实验模拟。将冰样品沉积在8K的红外透明窗口上,然后用微波放电的氢气流灯照射。辐照后,将冰样品加热直至完全升华。结果。 CO2分子的光解可引发光子诱导的化学反应网络,从而导致CO,CO3,O2和O3的形成。在辐照过程中,光子诱导的CO解吸,并在较小程度上由O2和CO2的解吸发生,该过程称为电子跃迁引起的间接解吸,最大入射光子脱附率约为1.2×10-2分子(Ypd)。 1,〜9.3×10-4分子入射光子-1和〜1.1×10-4分子入射光子-1。结论。质谱仪的校准可以直接定量分析光解吸的产率,而不是以前大多数工作中从红外光谱获得的间接值。红外光谱法提供的补充信息可对在紫外线照射下的冰幔中发生的过程进行完整的量化,从而更好地理解。

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