连续加氢对多环芳烃离子的单分子化学影响如何?

Q2 Physics and Astronomy
Malick Diedhiou, Brandi J. West, Paul M Mayer
{"title":"连续加氢对多环芳烃离子的单分子化学影响如何?","authors":"Malick Diedhiou,&nbsp;Brandi J. West,&nbsp;Paul M Mayer","doi":"10.1016/j.molap.2020.100071","DOIUrl":null,"url":null,"abstract":"<div><p><span>Hydrogenated polycyclic aromatic hydrocarbons (PAHs) have been proposed to contribute to the formation of interstellar H</span><sub>2</sub><span> by acting as a surface catalyst for the adsorption of hydrogen atoms and desorption of H</span><sub>2</sub><span><span> molecules. In the present study, imaging photoelectron<span> photoion coincidence (iPEPICO) spectroscopy and tandem mass spectrometry were employed to examine the unimolecular </span></span>chemistry of four hydrogenated polycyclic aromatic hydrocarbon ions: 9,10-dihydroanthracene (DHA</span><sup>+•</sup>) and 1,2,3,4,5,6,7,8-octahydroanthracene (OHA<sup>+•</sup>), having opposite patterns of hydrogenation, and 1,2,3,4-tetrahydrophenanthrene (THP<sup>+•</sup>) and 1,2,3,4,9,10-hexahydrophenanthrene (HHP<sup>+•</sup>). DHA<sup>+•</sup> exhibits the same reactions previously observed for 1,2-dihydronaphthalene and 9,10-dihydrophenanthrene, namely competing loss of H<sup>•</sup> and CH<sub>3</sub><sup>•</sup>. However, the energy required for H<sup>•</sup><span>-loss, as predicted by RRKM modeling of the iPEPICO results, was lower than the latter ions, presumably due to charge delocalization across the central ring upon dehydrogenation. OHA</span><sup>+•</sup><span> behaves similarly to ionized tetralin, displaying losses of H</span><sup>•</sup>, CH<sub>3</sub><sup>•</sup>, C<sub>2</sub>H<sub>4</sub> and C<sub>3</sub>H<sub>5</sub><sup>•</sup><span><span> in its collision induced dissociation (CID) </span>mass spectra, but under iPEPICO conditions CH</span><sub>3</sub><sup>•</sup>-loss is not observed. THP<sup>+•</sup> and HHP<sup>+•</sup> have aspects of both DHA<sup>+•</sup> and OHA<sup>+•</sup> chemistries, displaying losses of H<sup>•</sup>, CH<sub>3</sub><sup>•</sup>, C<sub>2</sub>H<sub>4</sub> and C<sub>3</sub>H<sub>5</sub><sup>•</sup>. RRKM modeling produced minimum energies for all observed reaction channels, which were also computationally explored at the B3LYP/6–31+G(d,p) level of theory. The results indicate that small PAH ions may not be effective surfaces for the catalytic formation of H<sub>2</sub> in the ISM, but rather sources of small hydrocarbons.</p></div>","PeriodicalId":44164,"journal":{"name":"Molecular Astrophysics","volume":"19 ","pages":"Article 100071"},"PeriodicalIF":0.0000,"publicationDate":"2020-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/j.molap.2020.100071","citationCount":"3","resultStr":"{\"title\":\"How does successive hydrogen addition to PAH ions impact their unimolecular chemistry?\",\"authors\":\"Malick Diedhiou,&nbsp;Brandi J. West,&nbsp;Paul M Mayer\",\"doi\":\"10.1016/j.molap.2020.100071\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p><span>Hydrogenated polycyclic aromatic hydrocarbons (PAHs) have been proposed to contribute to the formation of interstellar H</span><sub>2</sub><span> by acting as a surface catalyst for the adsorption of hydrogen atoms and desorption of H</span><sub>2</sub><span><span> molecules. In the present study, imaging photoelectron<span> photoion coincidence (iPEPICO) spectroscopy and tandem mass spectrometry were employed to examine the unimolecular </span></span>chemistry of four hydrogenated polycyclic aromatic hydrocarbon ions: 9,10-dihydroanthracene (DHA</span><sup>+•</sup>) and 1,2,3,4,5,6,7,8-octahydroanthracene (OHA<sup>+•</sup>), having opposite patterns of hydrogenation, and 1,2,3,4-tetrahydrophenanthrene (THP<sup>+•</sup>) and 1,2,3,4,9,10-hexahydrophenanthrene (HHP<sup>+•</sup>). DHA<sup>+•</sup> exhibits the same reactions previously observed for 1,2-dihydronaphthalene and 9,10-dihydrophenanthrene, namely competing loss of H<sup>•</sup> and CH<sub>3</sub><sup>•</sup>. However, the energy required for H<sup>•</sup><span>-loss, as predicted by RRKM modeling of the iPEPICO results, was lower than the latter ions, presumably due to charge delocalization across the central ring upon dehydrogenation. OHA</span><sup>+•</sup><span> behaves similarly to ionized tetralin, displaying losses of H</span><sup>•</sup>, CH<sub>3</sub><sup>•</sup>, C<sub>2</sub>H<sub>4</sub> and C<sub>3</sub>H<sub>5</sub><sup>•</sup><span><span> in its collision induced dissociation (CID) </span>mass spectra, but under iPEPICO conditions CH</span><sub>3</sub><sup>•</sup>-loss is not observed. THP<sup>+•</sup> and HHP<sup>+•</sup> have aspects of both DHA<sup>+•</sup> and OHA<sup>+•</sup> chemistries, displaying losses of H<sup>•</sup>, CH<sub>3</sub><sup>•</sup>, C<sub>2</sub>H<sub>4</sub> and C<sub>3</sub>H<sub>5</sub><sup>•</sup>. RRKM modeling produced minimum energies for all observed reaction channels, which were also computationally explored at the B3LYP/6–31+G(d,p) level of theory. The results indicate that small PAH ions may not be effective surfaces for the catalytic formation of H<sub>2</sub> in the ISM, but rather sources of small hydrocarbons.</p></div>\",\"PeriodicalId\":44164,\"journal\":{\"name\":\"Molecular Astrophysics\",\"volume\":\"19 \",\"pages\":\"Article 100071\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-06-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.1016/j.molap.2020.100071\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Molecular Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S2405675820300099\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Molecular Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S2405675820300099","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 3

摘要

氢化多环芳烃(PAHs)作为表面催化剂,吸附氢原子和解吸H2分子,参与星际H2的形成。本研究采用成像光电子光离子符合(iPEPICO)光谱和串联质谱法研究了4种氢化多环芳烃离子的单分子化学性质:9,10-二氢蒽(DHA+•)和氢化方式相反的1,2,3,4,5,6,7,8-八氢蒽(OHA+•),1,2,3,4-四氢菲(THP+•)和1,2,3,3,4,9,10 -六氢菲(HHP+•)。DHA+•表现出与1,2-二氢萘和9,10-二氢菲相同的反应,即H•和CH3•的竞争性损失。然而,正如iPEPICO结果的RRKM模型所预测的那样,H•损失所需的能量低于后一种离子,可能是由于脱氢时电荷在中心环上的离域。OHA+•在碰撞诱导解离(CID)质谱中表现出H•、CH3•、C2H4和C3H5•的损失,但在iPEPICO条件下没有观察到CH3•损失。THP+•和HHP+•具有DHA+•和OHA+•的化学性质,表现为H•、CH3•、C2H4和C3H5•的损失。RRKM模型为所有观察到的反应通道产生了最小能量,并在理论的B3LYP/ 6-31 +G(d,p)水平上进行了计算探索。结果表明,在ISM中,小的多环芳烃离子可能不是催化生成H2的有效表面,而是小碳氢化合物的来源。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

How does successive hydrogen addition to PAH ions impact their unimolecular chemistry?

How does successive hydrogen addition to PAH ions impact their unimolecular chemistry?

Hydrogenated polycyclic aromatic hydrocarbons (PAHs) have been proposed to contribute to the formation of interstellar H2 by acting as a surface catalyst for the adsorption of hydrogen atoms and desorption of H2 molecules. In the present study, imaging photoelectron photoion coincidence (iPEPICO) spectroscopy and tandem mass spectrometry were employed to examine the unimolecular chemistry of four hydrogenated polycyclic aromatic hydrocarbon ions: 9,10-dihydroanthracene (DHA+•) and 1,2,3,4,5,6,7,8-octahydroanthracene (OHA+•), having opposite patterns of hydrogenation, and 1,2,3,4-tetrahydrophenanthrene (THP+•) and 1,2,3,4,9,10-hexahydrophenanthrene (HHP+•). DHA+• exhibits the same reactions previously observed for 1,2-dihydronaphthalene and 9,10-dihydrophenanthrene, namely competing loss of H and CH3. However, the energy required for H-loss, as predicted by RRKM modeling of the iPEPICO results, was lower than the latter ions, presumably due to charge delocalization across the central ring upon dehydrogenation. OHA+• behaves similarly to ionized tetralin, displaying losses of H, CH3, C2H4 and C3H5 in its collision induced dissociation (CID) mass spectra, but under iPEPICO conditions CH3-loss is not observed. THP+• and HHP+• have aspects of both DHA+• and OHA+• chemistries, displaying losses of H, CH3, C2H4 and C3H5. RRKM modeling produced minimum energies for all observed reaction channels, which were also computationally explored at the B3LYP/6–31+G(d,p) level of theory. The results indicate that small PAH ions may not be effective surfaces for the catalytic formation of H2 in the ISM, but rather sources of small hydrocarbons.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Molecular Astrophysics
Molecular Astrophysics ASTRONOMY & ASTROPHYSICS-
自引率
0.00%
发文量
0
期刊介绍: Molecular Astrophysics is a peer-reviewed journal containing full research articles, selected review articles, and thematic issues. Molecular Astrophysics is a new journal where researchers working in planetary and exoplanetary science, astrochemistry, astrobiology, spectroscopy, physical chemistry and chemical physics can meet and exchange their ideas. Understanding the origin and evolution of interstellar and circumstellar molecules is key to understanding the Universe around us and our place in it and has become a fundamental goal of modern astrophysics. Molecular Astrophysics aims to provide a platform for scientists studying the chemical processes that form and dissociate molecules, and control chemical abundances in the universe, particularly in Solar System objects including planets, moons, and comets, in the atmospheres of exoplanets, as well as in regions of star and planet formation in the interstellar medium of galaxies. Observational studies of the molecular universe are driven by a range of new space missions and large-scale scale observatories opening up. With the Spitzer Space Telescope, the Herschel Space Observatory, the Atacama Large Millimeter/submillimeter Array (ALMA), NASA''s Kepler mission, the Rosetta mission, and more major future facilities such as NASA''s James Webb Space Telescope and various missions to Mars, the journal taps into the expected new insights and the need to bring the various communities together on one platform. The journal aims to cover observational, laboratory as well as computational results in the galactic, extragalactic and intergalactic areas of our universe.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信