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VACUUM ULTRAVIOLET ABSORPTION SPECTRA OF RARE GASES MIXTURES

Please use this identifier to cite or link to this item: http://hdl.handle.net/1811/9795

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dc.creator Castex, Marie-Claude en_US
dc.date.accessioned 2006-06-15T13:48:46Z
dc.date.available 2006-06-15T13:48:46Z
dc.date.issued 1976 en_US
dc.identifier 1976-Sigma-R-5 en_US
dc.identifier.uri http://hdl.handle.net/1811/9795
dc.description Present address of L. W. Buxton: Department of Chemistry, The University of Illinois, Champaign-Urbana, Illinois, 61801. en_US
dc.description Author Institution: Laboratoire des Interactions Mol\'{e}culaires et des Hautes Pressions, C.N.R.S. en_US
dc.description.abstract The vacuum ultraviolet absorption spectra of Xe-rare gas and Kr-rare gas mixtures have been investigated between 1150 and 1500 {\AA}. These spectra are characterized by the appearance of band systems, often called ""satellite bands"", associated with allowed or forbidden Xe (Kr) atomic states. Quantitative absorption measurements with a double-beam Spectrophotometer as a function of pressure (p < 760 Torr) and temperature $(130^\circ K$ $<$ T $< 300^\circ K$ ) provide information on their bound or unbound diatomic molecular origin. From high resolution analysis of the spectra photographed with a ten-meter Spectrograph, information may be obtained on the excited states: the bands observed on the high energy side of the atomic transition are explained by molecular bound-free transitions. The bands observed on the low energy side arise from a minimum in the difference potential between the ground and the excited states. en_US
dc.format.extent 123411 bytes
dc.format.mimetype image/jpeg
dc.language.iso English en_US
dc.title VACUUM ULTRAVIOLET ABSORPTION SPECTRA OF RARE GASES MIXTURES en_US
dc.type article en_US