Vacuum energy density and pressure near a soft wall
arXiv:1512.09121 · doi:10.1103/PhysRevD.93.105010
Abstract
Perfectly conducting boundaries, and their Dirichlet counterparts for quantum scalar fields, predict nonintegrable energy densities. A more realistic model with a finite ultraviolet cutoff yields two inconsistent values for the force on a curved or edged boundary (the "pressure anomaly"). A still more realistic, but still easily calculable, model replaces the hard wall by a power-law potential; because it involves no a posteriori modification of the formulas calculated from the theory, this model should be anomaly-free. Here we first set up the formalism and notation for the quantization of a scalar field in the background of a planar soft wall, and we approximate the reduced Green function in perturbative and WKB limits (the latter being appropriate when either the mode frequency or the depth into the wall is sufficiently large). Then we display numerical calculations of energy density and pressure for the region outside the wall, which show that the pressure anomaly does not occur there. Calculations inside the wall are postponed to later papers, which must tackle regularization and renormalization of divergences induced by the potential in the bulk region.
21 pages, 12 figures; v2 has improved graphics, more references, minor corrections, two new coauthors
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- Local Casimir Effect for a Scalar Field in Presence of a Point Impurity
- Renormalization for a Scalar Field in an External Scalar Potential
- Local Neumann semitransparent layers: resummation, pair production and duality
- Vacuum energy density and pressure inside a soft wall
- Disordered Bose-Einstein condensate in hard walls trap
- Vacuum energy, the Casimir effect, and Newton's non-constant
- Scarf for Lifshitz
- Thermodynamics of the scalar radiation in the presence of a reflecting plane wall