Exploring Anthracene in Laser-Induced Carbon Plasma Studies with Long-Wave Infrared Laser-Induced Breakdown Spectroscopy for Understanding Carbon Microstructure Formation in Space

IF 2.9 3区 化学 Q2 CHEMISTRY, MULTIDISCIPLINARY
Clayton S.-C. Yang*, Vincent J. Esposito, Laszlo Nemes, Feng Jin, Sudhir Trivedi, Uwe Hommerich and Alan C. Samuels, 
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Abstract

Long-wave infrared laser-induced breakdown spectroscopy (LWIR LIBS) of anthracene, a representative polycyclic aromatic hydrocarbon, under high-energy plasma conditions, combined with harmonic and anharmonic emission spectral simulations and HITRAN-based analyses, uncovers potential pathways of molecular fragmentation, recombination, and intermediate formation, identifying small hydrocarbons (e.g., CH4 and C2H2) and aromatic compounds (e.g., benzene and naphthalene). The experimental setup facilitated the simultaneous acquisition of UV/vis/NIR and LWIR spectra, offering a comprehensive analysis of molecular dynamics in a controlled plasma environment. Key findings demonstrate the influence of carrier gases, with argon inducing extensive fragmentation and helium maintaining the structural integrity of anthracene. Intriguingly, emission features at 6.98 and 8.3 μm suggest the possible presence of transient fullerenes, warranting further investigation. This study highlights the utility of LWIR LIBS for elucidating the fundamental mechanisms of cosmic carbon synthesis, offering insights into interstellar dust formation, planetary surface chemistry, and the pathways of prebiotic organic evolution. Future integration with mass spectrometry is proposed to enhance molecular identification and expand the understanding of plasma-induced carbon chemistry.

Abstract Image

利用长波红外激光诱导击穿光谱技术探索激光诱导碳等离子体中的蒽
高能等离子体条件下具有代表性的多环芳烃蒽的长波红外激光诱导击穿光谱(LWIR LIBS),结合谐波和非谐波发射光谱模拟和基于hitran的分析,揭示了分子断裂、重组和中间产物形成的潜在途径,识别了小碳氢化合物(如CH4和C2H2)和芳香族化合物(如苯和萘)。实验装置有助于同时获取UV/vis/NIR和LWIR光谱,在受控等离子体环境中提供全面的分子动力学分析。关键发现证明了载气的影响,氩气引起广泛的碎裂,氦气保持了蒽的结构完整性。有趣的是,在6.98和8.3 μm处的发射特征表明可能存在瞬态富勒烯,值得进一步研究。这项研究强调了LWIR LIBS在阐明宇宙碳合成基本机制方面的实用性,为星际尘埃形成、行星表面化学和益生元有机进化途径提供了见解。未来将与质谱结合,以加强分子鉴定和扩大对等离子体诱导碳化学的理解。
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来源期刊
ACS Earth and Space Chemistry
ACS Earth and Space Chemistry Earth and Planetary Sciences-Geochemistry and Petrology
CiteScore
5.30
自引率
11.80%
发文量
249
期刊介绍: The scope of ACS Earth and Space Chemistry includes the application of analytical, experimental and theoretical chemistry to investigate research questions relevant to the Earth and Space. The journal encompasses the highly interdisciplinary nature of research in this area, while emphasizing chemistry and chemical research tools as the unifying theme. The journal publishes broadly in the domains of high- and low-temperature geochemistry, atmospheric chemistry, marine chemistry, planetary chemistry, astrochemistry, and analytical geochemistry. ACS Earth and Space Chemistry publishes Articles, Letters, Reviews, and Features to provide flexible formats to readily communicate all aspects of research in these fields.
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