Matches in SemOpenAlex for { <https://semopenalex.org/work/W2023201888> ?p ?o ?g. }
- W2023201888 endingPage "2314" @default.
- W2023201888 startingPage "2302" @default.
- W2023201888 abstract "It is demonstrated that matrix-like spectroscopy may be carried out in the gas phase using molecular beams of clusters and the conditions under which bulk-matrix-like behavior is achieved are illustrated. At the same time, we obtain information on the structural evolution of noble gas clusters as a function of their size. Infrared spectra for SF6 attached to noble gas clusters of argon, krypton, and xenon were recorded using a free jet cluster source and a laser photofragmentation detection technique. When a dilute mixture of the chromophore in Ar and Kr is expanded at relatively low pressures, the clusters spectra show a feature characteristic of the SF6 solvated in a defective, unannealed matrix. This feature disappears at higher source pressures (larger sizes) at which the chromophore prefers to reside on the surface of the cluster. This can be demonstrated by producing neat clusters and depositing the chromophore on them. However, on producing still larger clusters, a different absorption appears which is accurately located at the same position as the main absorption in a well-annealed matrix of Ar or Kr. This behavior is related to the transition of clusters from a Mackay icosahedral structure, shown to be the most stable for smaller clusters, to the face-centered-cubic (fcc) structure which is observed in the bulk phase. This structural transition occurs at a nozzle stagnation pressure which corresponds to an average cluster size of about 2000 atoms for both Ar and Kr. Scattering studies performed on argon clusters suggest that the fcc-type clusters correspond to the largest sizes in the cluster size distribution present in the beams. A similar structural transition for xenon cluster was not established as the SF6 appears to solvate only slightly in Xe in the size range studied here." @default.
- W2023201888 created "2016-06-24" @default.
- W2023201888 creator A5004873717 @default.
- W2023201888 creator A5015711601 @default.
- W2023201888 creator A5040194464 @default.
- W2023201888 date "1995-02-08" @default.
- W2023201888 modified "2023-10-16" @default.
- W2023201888 title "Noble gas clusters as matrices for infrared spectroscopy. From small clusters to the bulk-matrix limit: SF6Ar<i>n</i>, SF6Kr<i>n</i>, and SF6Xe<i>n</i> with 100≲<i>n</i>≲10 000" @default.
- W2023201888 cites W1965258253 @default.
- W2023201888 cites W1966873215 @default.
- W2023201888 cites W1969761292 @default.
- W2023201888 cites W1978614837 @default.
- W2023201888 cites W1979990363 @default.
- W2023201888 cites W1984181592 @default.
- W2023201888 cites W1989814314 @default.
- W2023201888 cites W2004366174 @default.
- W2023201888 cites W2005776470 @default.
- W2023201888 cites W2006109315 @default.
- W2023201888 cites W2017004982 @default.
- W2023201888 cites W2017918114 @default.
- W2023201888 cites W2020257390 @default.
- W2023201888 cites W2034796623 @default.
- W2023201888 cites W2038669286 @default.
- W2023201888 cites W2040025498 @default.
- W2023201888 cites W2042642365 @default.
- W2023201888 cites W2044270257 @default.
- W2023201888 cites W2051387162 @default.
- W2023201888 cites W2052691968 @default.
- W2023201888 cites W2057985864 @default.
- W2023201888 cites W2077818116 @default.
- W2023201888 cites W2078047375 @default.
- W2023201888 cites W2078935943 @default.
- W2023201888 cites W2085447425 @default.
- W2023201888 cites W2093161296 @default.
- W2023201888 cites W2114107537 @default.
- W2023201888 cites W2128014528 @default.
- W2023201888 doi "https://doi.org/10.1063/1.468718" @default.
- W2023201888 hasPublicationYear "1995" @default.
- W2023201888 type Work @default.
- W2023201888 sameAs 2023201888 @default.
- W2023201888 citedByCount "46" @default.
- W2023201888 countsByYear W20232018882012 @default.
- W2023201888 countsByYear W20232018882013 @default.
- W2023201888 countsByYear W20232018882014 @default.
- W2023201888 countsByYear W20232018882015 @default.
- W2023201888 countsByYear W20232018882018 @default.
- W2023201888 countsByYear W20232018882022 @default.
- W2023201888 crossrefType "journal-article" @default.
- W2023201888 hasAuthorship W2023201888A5004873717 @default.
- W2023201888 hasAuthorship W2023201888A5015711601 @default.
- W2023201888 hasAuthorship W2023201888A5040194464 @default.
- W2023201888 hasConcept C113709186 @default.
- W2023201888 hasConcept C119824511 @default.
- W2023201888 hasConcept C120665830 @default.
- W2023201888 hasConcept C121332964 @default.
- W2023201888 hasConcept C121530826 @default.
- W2023201888 hasConcept C125287762 @default.
- W2023201888 hasConcept C153642686 @default.
- W2023201888 hasConcept C159985019 @default.
- W2023201888 hasConcept C164866538 @default.
- W2023201888 hasConcept C178790620 @default.
- W2023201888 hasConcept C184779094 @default.
- W2023201888 hasConcept C185592680 @default.
- W2023201888 hasConcept C192468462 @default.
- W2023201888 hasConcept C192562407 @default.
- W2023201888 hasConcept C199360897 @default.
- W2023201888 hasConcept C2777896788 @default.
- W2023201888 hasConcept C32891209 @default.
- W2023201888 hasConcept C41008148 @default.
- W2023201888 hasConcept C41999313 @default.
- W2023201888 hasConcept C521692839 @default.
- W2023201888 hasConcept C547737533 @default.
- W2023201888 hasConcept C548442186 @default.
- W2023201888 hasConcept C62520636 @default.
- W2023201888 hasConcept C75473681 @default.
- W2023201888 hasConcept C8010536 @default.
- W2023201888 hasConceptScore W2023201888C113709186 @default.
- W2023201888 hasConceptScore W2023201888C119824511 @default.
- W2023201888 hasConceptScore W2023201888C120665830 @default.
- W2023201888 hasConceptScore W2023201888C121332964 @default.
- W2023201888 hasConceptScore W2023201888C121530826 @default.
- W2023201888 hasConceptScore W2023201888C125287762 @default.
- W2023201888 hasConceptScore W2023201888C153642686 @default.
- W2023201888 hasConceptScore W2023201888C159985019 @default.
- W2023201888 hasConceptScore W2023201888C164866538 @default.
- W2023201888 hasConceptScore W2023201888C178790620 @default.
- W2023201888 hasConceptScore W2023201888C184779094 @default.
- W2023201888 hasConceptScore W2023201888C185592680 @default.
- W2023201888 hasConceptScore W2023201888C192468462 @default.
- W2023201888 hasConceptScore W2023201888C192562407 @default.
- W2023201888 hasConceptScore W2023201888C199360897 @default.
- W2023201888 hasConceptScore W2023201888C2777896788 @default.
- W2023201888 hasConceptScore W2023201888C32891209 @default.
- W2023201888 hasConceptScore W2023201888C41008148 @default.
- W2023201888 hasConceptScore W2023201888C41999313 @default.
- W2023201888 hasConceptScore W2023201888C521692839 @default.
- W2023201888 hasConceptScore W2023201888C547737533 @default.
- W2023201888 hasConceptScore W2023201888C548442186 @default.