From Rindler space to the electromagnetic energy-momentum tensor of a Casimir apparatus in a weak gravitational field
arXiv:0804.2839 · doi:10.1103/PhysRevD.78.024010
Abstract
This paper studies two perfectly conducting parallel plates in the weak gravitational field on the surface of the Earth. Since the appropriate line element, to first order in the constant gravity acceleration g, is precisely of the Rindler type, we can exploit the formalism for studying Feynman Green functions in Rindler spacetime. Our analysis does not reduce the electromagnetic potential to the transverse part before quantization. It is instead fully covariant and well suited for obtaining all components of the regularized and renormalized energy-momentum tensor to arbitrary order in the gravity acceleration g. The general structure of the calculation is therefore elucidated, and the components of the Maxwell energy-momentum tensor are evaluated up to second order in g, improving a previous analysis by the authors and correcting their old first-order formula for the Casimir energy.
10 pages
References in corpus (5)
- How Does Casimir Energy Fall?
- Energy-momentum tensor for a Casimir apparatus in a weak gravitational field
- Relativistic mechanics of Casimir apparatuses in a weak gravitational field
- How does Casimir energy fall? II. Gravitational acceleration of quantum vacuum energy
- Holographic dark energy and late cosmic acceleration
Cited by in corpus (20)
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- Recent Developments in the Casimir Effect
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- Casimir effect in Extended Theories of Gravity
- Casimir effect of two conducting parallel plates in a general weak gravitational field
- Casimir effect in a weak gravitational field and the spacetime index of refraction
- Electromagnetic Casimir effect and the spacetime index of refraction
- Null Second Order Corrections to Casimir Energy in Weak Gravitational Field
- Local and Global Casimir Energies: Divergences, Renormalization, and the Coupling to Gravity
- Energy-momentum tensor for a scalar Casimir apparatus in a weak gravitational field: Neumann conditions
- Casimir effect for curved boundaries in Robertson-Walker spacetime
- Quasi-local Casimir energy and vacuum buoyancy in a weak gravitational field
- Null second order corrections to Casimir energy in weak gravitational field: The Schwinger's approach
- How Does Quantum Vacuum Energy Accelerate?
- Vacuum fluctuation force on a rigid Casimir cavity in de Sitter and Schwarzschild-de Sitter spacetime
- Casimir densities for a boundary in Robertson-Walker spacetime
- Quasi-local stress-tensor formalism and the Casimir effect
- Quantum vacuum under mixed boundary conditions: the case for curved spacetime
- Towards obtaining Green functions for a Casimir cavity in de Sitter spacetime