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dc.contributor.authorSandra Schröteren_US
dc.contributor.authorApiwat Wijaikhumen_US
dc.contributor.authorAndrew R. Gibsonen_US
dc.contributor.authorAndrew Westen_US
dc.contributor.authorHelen L. Daviesen_US
dc.contributor.authorNicolas Minesien_US
dc.contributor.authorJames Dedricken_US
dc.contributor.authorErik Wagenaarsen_US
dc.contributor.authorNelson De Oliveiraen_US
dc.contributor.authorLaurent Nahonen_US
dc.contributor.authorMark J. Kushneren_US
dc.contributor.authorJean Paul Boothen_US
dc.contributor.authorKari Niemien_US
dc.contributor.authorTimo Gansen_US
dc.contributor.authorDeborah O'Connellen_US
dc.date.accessioned2018-11-29T07:38:00Z-
dc.date.available2018-11-29T07:38:00Z-
dc.date.issued2018-01-01en_US
dc.identifier.issn14639076en_US
dc.identifier.other2-s2.0-85054103811en_US
dc.identifier.other10.1039/c8cp02473aen_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85054103811&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/62642-
dc.description.abstract© the Owner Societies. Atmospheric pressure plasmas are sources of biologically active oxygen and nitrogen species, which makes them potentially suitable for the use as biomedical devices. Here, experiments and simulations are combined to investigate the formation of the key reactive oxygen species, atomic oxygen (O) and hydroxyl radicals (OH), in a radio-frequency driven atmospheric pressure plasma jet operated in humidified helium. Vacuum ultra-violet high-resolution Fourier-transform absorption spectroscopy and ultra-violet broad-band absorption spectroscopy are used to measure absolute densities of O and OH. These densities increase with increasing H2O content in the feed gas, and approach saturation values at higher admixtures on the order of 3 × 1014 cm−3 for OH and 3 × 1013 cm−3 for O. Experimental results are used to benchmark densities obtained from zero-dimensional plasma chemical kinetics simulations, which reveal the dominant formation pathways. At low humidity content, O is formed from OH+ by proton transfer to H2O, which also initiates the formation of large cluster ions. At higher humidity content, O is created by reactions between OH radicals, and lost by recombination with OH. OH is produced mainly from H2O+ by proton transfer to H2O and by electron impact dissociation of H2O. It is lost by reactions with other OH molecules to form either H2O + O or H2O2. Formation pathways change as a function of humidity content and position in the plasma channel. The understanding of the chemical kinetics of O and OH gained in this work will help in the development of plasma tailoring strategies to optimise their densities in applications.en_US
dc.subjectChemistryen_US
dc.subjectPhysics and Astronomyen_US
dc.titleChemical kinetics in an atmospheric pressure helium plasma containing humidityen_US
dc.typeJournalen_US
article.title.sourcetitlePhysical Chemistry Chemical Physicsen_US
article.volume20en_US
article.stream.affiliationsUniversity of Yorken_US
article.stream.affiliationsCNRS Centre National de la Recherche Scientifiqueen_US
article.stream.affiliationsSOLEIL Synchrotronen_US
article.stream.affiliationsUniversity of Michigan, Ann Arboren_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsUniversity of Manchesteren_US
article.stream.affiliationsLaboratoire d'Energetique Moleculaire et Macroscopique, Combustionen_US
Appears in Collections:CMUL: Journal Articles

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