Casimir effect in a weak gravitational field and the spacetime index of refraction
arXiv:1003.0614 · doi:10.1103/PhysRevD.85.044060
Abstract
In a recent paper [arXiv:0904.2904] using a conjecture it is shown how one can calculate the effect of a weak stationary gravitational field on vacuum energy in the context of Casimir effect in an external gravitational field treated in 1+3 formulation of spacetime decomposition.. In this article, employing quntum field theory in curved spacetime, we explicitly calculate the effect of a weak static gravitational field on virtual massless scalar particles in a Casimir apparatus. It is shown that, as expected from the proposed conjecture, both the frequency and renormalized energy of the virtual scalar field are affected by the gravitational field through its index of refraction. This could be taken as a strong evidence in favour of the proposed conjecture. Generalizations to weak {\it stationary} spacetimes and virtual photons are also discussed.
11 pages, RevTex, typos corrected (combined with arXiv:0904.2904 published in PRD)
References in corpus (5)
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- Energy-momentum tensor for a Casimir apparatus in a weak gravitational field
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- From Rindler space to the electromagnetic energy-momentum tensor of a Casimir apparatus in a weak gravitational field
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- General relativistic analogs of Poisson's equation and gravitational binding energy
- Null second order corrections to Casimir energy in weak gravitational field: The Schwinger's approach
- Static and stationary dark fluid universes: A gravitoelectromagnetic perspective
- Papapetrou field as the gravitoelectromagnetic field tensor in stationary spacetimes
- Quantum vacuum under mixed boundary conditions: the case for curved spacetime