2002
DOI: 10.1103/physrevd.66.085023
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Casimir effect in the Fulling-Rindler vacuum

Abstract: The vacuum expectation values of the energy-momentum tensor are investigated for massless scalar fields satisfying Dicichlet or Neumann boundary conditions, and for the electromagnetic field with perfect conductor boundary conditions on two infinite parallel plates moving by uniform proper acceleration through the Fulling-Rindler vacuum. The scalar case is considered for general values of the curvature coupling parameter and in an arbitrary number of spacetime dimension. The mode-summation method is used with … Show more

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Cited by 37 publications
(67 citation statements)
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“…From these expressions it follows that the coefficients u l (t) have the structure 17) with the numerical coefficients u lm . From the recurrence relations for the polynomials u l (t) (see [33]), the following recurrence formulae can be obtained for the coefficients u lm : 18) where m = 0, 1, .…”
Section: Vacuum Energy In the Rr Regionmentioning
confidence: 99%
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“…From these expressions it follows that the coefficients u l (t) have the structure 17) with the numerical coefficients u lm . From the recurrence relations for the polynomials u l (t) (see [33]), the following recurrence formulae can be obtained for the coefficients u lm : 18) where m = 0, 1, .…”
Section: Vacuum Energy In the Rr Regionmentioning
confidence: 99%
“…As a result the eigenmodes are independent of the curvature coupling parameter and, hence, the Casimir energy will not depend on this parameter. However, the local characteristics of the vacuum such as energy density and vacuum stresses depend on the parameter ζ [16,17].…”
Section: Casimir Energy For a Single Dirichlet Platementioning
confidence: 99%
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