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dc.contributor.authorHorsley, S. A. R.
dc.contributor.authorArtoni, M.
dc.contributor.authorLa Rocca, G. C.
dc.date.accessioned2013-08-05T16:01:02Z
dc.date.available2013-08-05T16:01:02Z
dc.date.issued2012-11
dc.identifier62958688
dc.identifier334f48db-bfd1-494a-882c-89a4ee847df0
dc.identifier000310708700023
dc.identifier84870167749
dc.identifier.citationHorsley , S A R , Artoni , M & La Rocca , G C 2012 , ' Radiation pressure on a moving body : beyond the Doppler effect ' , Journal of the Optical Society of America B : Optical Physics , vol. 29 , no. 11 , pp. 3136-3140 . https://doi.org/10.1364/JOSAB.29.003136en
dc.identifier.issn0740-3224
dc.identifier.urihttps://hdl.handle.net/10023/3920
dc.descriptionThe Engineering and Physical Sciences Research Council (EPSRC) provided financial support for this research.en
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.
dc.format.extent5
dc.format.extent312286
dc.language.isoeng
dc.relation.ispartofJournal of the Optical Society of America B : Optical Physicsen
dc.subjectElectromagnetic-wavesen
dc.subjectReflectionen
dc.subjectTransmissionen
dc.subjectFrictionen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleRadiation pressure on a moving body : beyond the Doppler effecten
dc.typeJournal articleen
dc.contributor.sponsorEPSRCen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1364/JOSAB.29.003136
dc.description.statusPeer revieweden
dc.identifier.grantnumberEP/H027610/1en


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