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dc.contributor.authorHorsley, S. A. R.
dc.contributor.authorSimpson, W. M. R.
dc.date.accessioned2014-08-18T08:31:02Z
dc.date.available2014-08-18T08:31:02Z
dc.date.issued2013-07-22
dc.identifier136327250
dc.identifier1debe25c-204e-4b59-8d20-b0291223cdc8
dc.identifier000322111800014
dc.identifier84880592312
dc.identifier.citationHorsley , S A R & Simpson , W M R 2013 , ' Cutoff dependence of the Casimir force within an inhomogeneous medium ' , Physical Review. A, Atomic, molecular, and optical physics , vol. 88 , no. 1 , 013833 . https://doi.org/10.1103/PhysRevA.88.013833en
dc.identifier.issn1050-2947
dc.identifier.urihttps://hdl.handle.net/10023/5178
dc.descriptionS.A.R.H. thanks the EPSRC for financial support, and the Weizmann Institute for their hospitality. W.M.R.S. thanks SUPA and the Weizmann Institute for their financial support.en
dc.description.abstractWe consider the ground-state energy of the electromagnetic field in a piston geometry. In the idealized case, where the piston and the walls of the chamber are taken as perfect mirrors, the Casimir pressure on the piston is finite and independent of the small-scale physics of the media that compose the mirrors; the Casimir energy of the system can be regularized and is cutoff independent. Yet we find that, when the body of the piston is filled with an inhomogeneous dielectric medium, the Casimir energy is cutoff dependent, and the value of the pressure is thus inextricably dependent on the detailed behavior of the mirror and the medium at large wave vectors. This result is inconsistent with recent proposals for regularizing Casimir forces in inhomogeneous media.
dc.format.extent5
dc.format.extent427941
dc.language.isoeng
dc.relation.ispartofPhysical Review. A, Atomic, molecular, and optical physicsen
dc.subject42.50.Lcen
dc.subject31.30.jhen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleCutoff dependence of the Casimir force within an inhomogeneous mediumen
dc.typeJournal articleen
dc.contributor.sponsorEPSRCen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1103/PhysRevA.88.013833
dc.description.statusPeer revieweden
dc.identifier.grantnumberEP/H027610/1en


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