2022
DOI: 10.1016/j.chemosphere.2021.132793
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Formation and growth mechanisms of polycyclic aromatic hydrocarbons: A mini-review

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Cited by 125 publications
(70 citation statements)
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“…35,36 It is important to state that we are not observing radical intermediates and many formation mechanisms are possible such as addition of phenyl and subsequent alkyl cyclization, 37 or direct addition of vinylacetylene (C 4 H 2 ). 21 The presence of 5-membered PAHs also opens the possibility of formation of curved PAHs or fullerenes since the ). Optical images taken from (i) before and (ii) after sputtering are displayed.…”
Section: Time Resolved Growth Of Flat and Curved Pahsmentioning
confidence: 99%
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“…35,36 It is important to state that we are not observing radical intermediates and many formation mechanisms are possible such as addition of phenyl and subsequent alkyl cyclization, 37 or direct addition of vinylacetylene (C 4 H 2 ). 21 The presence of 5-membered PAHs also opens the possibility of formation of curved PAHs or fullerenes since the ). Optical images taken from (i) before and (ii) after sputtering are displayed.…”
Section: Time Resolved Growth Of Flat and Curved Pahsmentioning
confidence: 99%
“…18 Flat and curved PAHs can form from smaller PAHs and can go onward to form soot particles and their mechanisms of formation have been well studied. [19][20][21] To advance this work we propose the use of the 3D OrbiSIMS depth profiling function to analyse deposits in situ on fuel injector component surfaces to establish the fate of molecules once deposited on a surface. This technique combines a low energy gas cluster ion beam to generate relatively large diagnostic secondary ions in situ for accurate identification and confirmation using the high mass resolving power (>240, 000) and MS/MS (fragmentation/structural characterization) capability of the Orbitrap™.…”
Section: Introductionmentioning
confidence: 99%
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“…Carbonaceous organic molecules especially polycyclic aromatic hydrocarbons (PAHs) are ubiquitously the key components in the astrochemical evolution of the interstellar medium (ISM) [1][2][3][4]. Understanding the chemical evolution of the Universe through the formation of the PAHs and their abundance in the astrochemical environment are one of the important aspects of astrochemistry [5,6]. The detection and isolation of the building blocks of PAHs in the laboratory by creating "space-like" environment is experimentally a daunting task.…”
Section: Introductionmentioning
confidence: 99%
“…The accuracy of numerical results depends not only on the algorithm used to solve the problem but also on the prediction of acetylene oxidation and self-decomposition reactions. The rapid development of elementary reactions of acetylene and hydrocarbon fuels in recent years has produced a large number of reaction rate coefficients with reliable precision [29]. Many general chemical reaction mechanisms for the formation of PAHs have been proposed [30][31][32][33].…”
Section: Introductionmentioning
confidence: 99%