{"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, Brandi J. West, 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, Brandi J. West, 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}
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.
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.