Please use this identifier to cite or link to this item:
https://doi.org/10.1364/OE.14.008958
DC Field | Value | |
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dc.title | Gravitation-dependent, thermally-induced self-diffraction in carbon nanotube solutions | |
dc.contributor.author | Ji, W. | |
dc.contributor.author | Chen, W. | |
dc.contributor.author | Lim, S. | |
dc.contributor.author | Lin, J. | |
dc.contributor.author | Guo, Z. | |
dc.date.accessioned | 2014-10-16T09:27:03Z | |
dc.date.available | 2014-10-16T09:27:03Z | |
dc.date.issued | 2006-10 | |
dc.identifier.citation | Ji, 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.issn | 10944087 | |
dc.identifier.uri | http://scholarbank.nus.edu.sg/handle/10635/96745 | |
dc.description.abstract | We 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.uri | http://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1364/OE.14.008958 | |
dc.source | Scopus | |
dc.type | Article | |
dc.contributor.department | PHYSICS | |
dc.description.doi | 10.1364/OE.14.008958 | |
dc.description.sourcetitle | Optics Express | |
dc.description.volume | 14 | |
dc.description.issue | 20 | |
dc.description.page | 8958-8966 | |
dc.identifier.isiut | 000240981000005 | |
Appears in Collections: | Staff Publications |
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