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dc.contributor.authorHorsley, S.A.R.
dc.contributor.authorArtoni, M.
dc.contributor.authorLa Rocca, G.C.
dc.date.accessioned2013-07-12T13:38:17Z
dc.date.issued2012-10-24
dc.description.abstractThe dependence of macroscopic radiation pressure on the velocity of the object being pushed is commonly attributed to the Doppler effect. This need not be the case, and here we highlight velocity-dependent radiation pressure terms that have their origins in the mixing of s and p polarizations brought about by the Lorentz transformation between the lab and the material rest frame, rather than in the corresponding transformation of frequency and wavevector. The theory we develop may be relevant to the nano-optomechanics of moving bodies.en_GB
dc.identifier.citationVol. 29 (11), pp. 3136 - 3140en_GB
dc.identifier.doi10.1364/JOSAB.29.003136
dc.identifier.urihttp://hdl.handle.net/10871/11727
dc.language.isoenen_GB
dc.publisherOptical Society of Americaen_GB
dc.titleRadiation pressure on a moving body: Beyond the Doppler effecten_GB
dc.typeArticleen_GB
dc.date.available2013-07-12T13:38:17Z
dc.identifier.issn0740-3224
dc.descriptionCopyright © 2012 Optical Society of Americaen_GB
dc.descriptionThis paper was published in Journal of the Optical Society of America B and is made available as an electronic reprint with the permission of OSA. The paper can be found at the following URL on the OSA website: http://www.opticsinfobase.org/josab/abstract.cfm?uri=josab-29-11-3136. Systematic or multiple reproduction or distribution to multiple locations via electronic or other means is prohibited and is subject to penalties under law.en_GB
dc.identifier.eissn1520-8540
dc.identifier.journalJournal of the Optical Society of America B: Optical Physicsen_GB


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