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dc.creatorBucaro, J. A.en_US
dc.creatorLitovitz, T. A.en_US
dc.date.accessioned2006-06-15T13:27:38Z
dc.date.available2006-06-15T13:27:38Z
dc.date.issued1971en_US
dc.identifier1971-Sigma-21en_US
dc.identifier.urihttp://hdl.handle.net/1811/8835
dc.description$^{*}$This research was supported by the Atomic Energy Commission. $^{\dagger}$Present address: Naval Research Laboratory, Washington, D.C.""en_US
dc.descriptionAuthor Institution: Department of Physics, The Catholic University of Americaen_US
dc.description.abstractMeasurements of light scattered in the Rayleigh wing were made over the range from 5 to $500 cm^{-1}$ in $CCI_{4}$, $C_{6}H_{12}$, $C_{5}H_{12}$, $CH_{3}OH$, $C_{2}H_{5}OH$, $H_{2}O$, $NH_{3}$ and $CHCl_{3}$. These data when compared with earlier data on Ar, Xe, and SnBr, indicate that in all of these liquids there is present the essentially exponential frequency dependence typical of collision induced effects. A calculation of the spectrum for large frequency shifts based on a binary interaction picture employing a Lennard-Jones potential and a short range electronic overlap distortion model agrees well with the experimental results in liquid argon. Further, assuming that molecular frame distortion is proportional to the interaction force, a similar calculation yields excellent agreement for the molecular systems. It is concluded that isolated binary interactions are mainly responsible for the spectral density in the wings of the Rayleigh Spectrum.en_US
dc.format.extent109300 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleRAYLEIGH SCATTERING: COLLISIONAL MOTIONS IN $LIQUIDS^{*}$en_US
dc.typearticleen_US


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