We compute the Casimir stress on a perfectly conducting cylindrical shell, due to quantum field fluctuations (zero-point energy) in both the interior and exterior regions, using a Green's dyadic formulation for the field strengths. To obtain a finite answer, a frequency cutoff must be inserted, but
Casimir self-stress on a perfectly conducting spherical shell
โ Scribed by Kimball A. Milton; Lester L. DeRaad Jr.; Julian Schwinger
- Publisher
- Elsevier Science
- Year
- 1978
- Tongue
- English
- Weight
- 690 KB
- Volume
- 115
- Category
- Article
- ISSN
- 0003-4916
No coin nor oath required. For personal study only.
โฆ Synopsis
The Casimir stress on a perfectly conducting uncharged sphere, due to occurrence of fluctuations in the electromagnetic field, is calculated using a source theory formulation. Two independent methods are employed: we compute (1) the total Casimir energy inside and outside the sphere, and (2) the radial component of the stress tensor on the surface. It is necessary to exercise care in allowing the field points to overlap; a correct limiting procedure supplies a "cutoff" in the frequency integration. In spite of numerous technical improvements, the result of Boyer, that the self-stress is repulsive (and not attractive as Casimir hoped), is confirmed unambiguously. The magnitude of the Casimir energy of a sphere of radius a is found, by numerical and analytic techniques, to be E = (fic/2a)(0.09235), also in agreement with the very recent result of Balian and Duplantier.
๐ SIMILAR VOLUMES
The Casimir self-stress, due to fluctuations of the electromagnetic field, for a solid dielectric ball is calculated using a formalism previously employed for the reevaluation of the repulsive Casimir stress on a conducting spherical shell. Even after volume energy subtractions are performed, the re
We show within the Hamiltonian formalism the existence of classical relativistic mechanics of N scalar particles interacting at a distance which satisfies the requirements of Poincare invariance, separability, world-line invariance and Einstein causality. The line of approach which is adopted here u
Starting from the tensor product of N irreducible positive energy representations of the Poincare group describing N free relativistic particles with arbitrary spins and positive masses, we construct an interacting positive energy representation by modifying the total 4-momentum operator. We first m