2008
DOI: 10.1016/j.aop.2008.03.001
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Wightman function and scalar Casimir densities for a wedge with two cylindrical boundaries

Abstract: Wightman function, the vacuum expectation values of the field square and the energymomentum tensor are investigated for a massive scalar field with general curvature coupling parameter inside a wedge with two coaxial cylindrical boundaries. It is assumed that the field obeys Dirichlet boundary condition on bounding surfaces. The application of a variant of the generalized Abel-Plana formula enables to extract from the expectation values the contribution corresponding to the geometry of a wedge with a single sh… Show more

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Cited by 12 publications
(11 citation statements)
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References 61 publications
(92 reference statements)
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“…We will enforce Dirichlet boundary condition on the inner and outer cylinder. This is similar to situations studied by Nesterenko et al 15,16 for global Casimir energies for the case of one circular boundary and by Saharian et al 17,18 for the local properties of the stress energy tensor for the case of both one and two circular boundaries. The radial potentials will be semi-transparent deltafunction potentials in the angular coordinates, λ 2 δ(θ − α).…”
Section: Casimir Energy For Planes In An Annular Cavitysupporting
confidence: 88%
“…We will enforce Dirichlet boundary condition on the inner and outer cylinder. This is similar to situations studied by Nesterenko et al 15,16 for global Casimir energies for the case of one circular boundary and by Saharian et al 17,18 for the local properties of the stress energy tensor for the case of both one and two circular boundaries. The radial potentials will be semi-transparent deltafunction potentials in the angular coordinates, λ 2 δ(θ − α).…”
Section: Casimir Energy For Planes In An Annular Cavitysupporting
confidence: 88%
“…In addition to describing the physical structure of a quantum field at a given point, the energy-momentum tensor acts as the source in the Einstein equations and therefore plays an important role in modelling a self-consistent dynamics involving the gravitational field. The vacuum densities for a Robin cylindrical boundary in the Minkowski background are investigated in [36] (see also [37] for the case of two coaxial cylindrical surfaces). In Ref.…”
Section: Introductionmentioning
confidence: 99%
“…That is, we consider conducting boundaries at r = r min > 0, r = r max < ∞, θ = 0 with r min < r < r max , and θ = α with r min < r < r max , and allow the last boundary to move. This model has been studied in various ways in [6] and [7], but those works do not answer all the questions we need to ask. The divergence at r = 0 is now removed (and would be independent of α anyway).…”
Section: Discussionmentioning
confidence: 99%