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Energy dependence of infrared emission from azulene C–H stretching vibrations
dc.contributor.authorShi, Jichunen_US
dc.contributor.authorBernfeld, Dianeen_US
dc.contributor.authorBarker, John R.en_US
dc.date.accessioned2010-05-06T22:10:06Z
dc.date.available2010-05-06T22:10:06Z
dc.date.issued1988-05-15en_US
dc.identifier.citationShi, Jichun; Bernfeld, Diane; Barker, John R. (1988). "Energy dependence of infrared emission from azulene C–H stretching vibrations." The Journal of Chemical Physics 88(10): 6211-6218. <http://hdl.handle.net/2027.42/70442>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/70442
dc.description.abstractNew data are described on the energy dependence of infrared fluorescence (IRF) from the C–H stretch modes (∼3050 cm−1) of vibrationally excited azulene (C10H8). An optoacoustic method was used to measure the absorbed laser energy and determine the number of excited molecules, while time‐resolved infrared emission was recorded. The experimental uncertainties of ∼5% are much smaller than in previous work and the agreement between the experiments and the theory for the IRF intensity is excellent for total vibrational energies from 14 000 to 33 000 cm−1.en_US
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dc.format.extent560934 bytes
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dc.format.mimetypeapplication/pdf
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleEnergy dependence of infrared emission from azulene C–H stretching vibrationsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, Space Physics Research Laboratory, University of Michigan, Ann Arbor, Michigan 48109‐2143en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/70442/2/JCPSA6-88-10-6211-1.pdf
dc.identifier.doi10.1063/1.454459en_US
dc.identifier.sourceThe Journal of Chemical Physicsen_US
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dc.owningcollnamePhysics, Department of


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