Please use this identifier to cite or link to this item: https://doi.org/10.1364/OE.14.008958
DC FieldValue
dc.titleGravitation-dependent, thermally-induced self-diffraction in carbon nanotube solutions
dc.contributor.authorJi, W.
dc.contributor.authorChen, W.
dc.contributor.authorLim, S.
dc.contributor.authorLin, J.
dc.contributor.authorGuo, Z.
dc.date.accessioned2014-10-16T09:27:03Z
dc.date.available2014-10-16T09:27:03Z
dc.date.issued2006-10
dc.identifier.citationJi, W., Chen, W., Lim, S., Lin, J., Guo, Z. (2006-10). Gravitation-dependent, thermally-induced self-diffraction in carbon nanotube solutions. Optics Express 14 (20) : 8958-8966. ScholarBank@NUS Repository. https://doi.org/10.1364/OE.14.008958
dc.identifier.issn10944087
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/96745
dc.description.abstractWe report the observation of thermally-induced self-diffraction in carbon nanotube (CNT) solutions under the influence of the gravity. We present a theoretical model in which CNTs are assumed to obey the Boltzmman distribution law. Under the approximations of small temperature rise and a very narrow distribution of CNT masses, the model simulation is consistent with the data measured at low laser powers. An immediate application of such a gravitation-dependent characteristic is the optical measurement for molecular weights of CNTs. ©2006 Optical Society of America.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1364/OE.14.008958
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentPHYSICS
dc.description.doi10.1364/OE.14.008958
dc.description.sourcetitleOptics Express
dc.description.volume14
dc.description.issue20
dc.description.page8958-8966
dc.identifier.isiut000240981000005
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