Spherical Casimir pistons
arXiv:1102.1946 · doi:10.1088/0264-9381/28/15/155018
Abstract
A piston is introduced into a spherical lune Casimir cavity turning it into two adjacent lunes separated by the (hemispherical) piston. On the basis of zeta function regularisation, the vacuum energy of the arrangement is finite for conformal propagation in space-time. For even spheres this energy is independent of the angle of the lune. For odd dimensions it is shown that for all Neumann, or all Dirichlet, boundary conditions the piston is attracted or repelled by the nearest wall if d=3,7,... or if d=1,5,..., respectively. For hybrid N-D conditions these requirements are switched. If a mass is added, divergences arise which render the model suspect. The analysis, however, is relatively straightforward and involves the Barnes zeta function. The extension to finite temperatures is made and it is shown that for the 3,7,... series of odd spheres, the repulsion by the walls continues but that, above a certain temperature, the free energy acquires two minima symmetrically placed about the mid point.
10 pages. Finite temperature results added
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Cited by in corpus (6)
- Conical Casimir Pistons with Hybrid Boundary Conditions
- Casimir Pistons with General Boundary Conditions
- The Casimir Effect for Generalized Piston Geometries
- Some Developments of the Casimir Effect in -Cavity of -Dimensional Spacetime
- Quantum revivals in free field CFT
- The Casimir Effect for Thick Pistons