ENERGY DENSITY AND PRESSURE IN POWER-WALL MODELS
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Publication:2919252
DOI10.1142/S0217751X12600093zbMath1247.81597MaRDI QIDQ2919252
Jef Wagner, Stephen A. Fulling, Kimball A. Milton
Publication date: 2 October 2012
Published in: International Journal of Modern Physics A (Search for Journal in Brave)
Model quantum field theories (81T10) Perturbative methods of renormalization applied to problems in quantum field theory (81T15) Electromagnetic interaction; quantum electrodynamics (81V10)
Related Items (3)
Renormalization for a scalar field in an external scalar potential ⋮ Local Casimir effect for a scalar field in presence of a point impurity ⋮ Curved space quantum field theory of the 1970S elucidates boundary Casimir energy today
Cites Work
- Calculating vacuum energies in renormalizable quantum field theories: A new approach to the Casimir problem
- Static negative energies near a domain wall
- VACUUM ENERGY DENSITY AND PRESSURE NEAR BOUNDARIES
- Vacuum stress and closed paths in rectangles, pistons and pistols
- Systematics of the relationship between vacuum energy calculations and heat-kernel coefficients
- Casimir's spheres near the Coulomb limit: energy density, pressures and radiative effects
- Casimir energies of spherical plasma shells
- PERTURBATIVE CASIMIR ENERGIES OF SPHERES: TOWARDS RE-ORIENTING AND AGENDA
- Casimir effects for a flat plasma sheet: I. Energies
- Casimir effects for a flat plasma sheet: II. Fields and stresses
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