Attractive or repulsive nature of Casimir force in D -dimensional Minkowski spacetime
Journal Article
·
· Physical Review, D (Particles Fields); (USA)
- Centro Brasileiro de Pesquisas Fisicas, Rua Dr. Xavier Sigaud 150, 22290 Rio de Janeiro, Brazil (BR)
- Instituto de Matematica Pura e Aplicada, Estrada Dona Castorina 110, 22460 Rio de Janeiro, (Brazil)
- Centro Brasileiro de Pesquisas Fisicas, Rua Dr. Xavier Sigaud 150, 22290 Rio de Janeiro, (Brazil)
The dependence of Casimir energy (associated with a massless scalar field) on spacetime dimensionality ({ital D}) is shown to be strongly entangled with the type of geometric bounds and the kind of macroscopic boundary conditions imposed on the field. In the case of a massless scalar field satisfying Dirichlet boundary conditions in the presence of a hyperparallelepipedal cavity with {ital p} sides of finite length {ital L} and {ital D}{minus}{ital p}{minus}1 sides with length much greater than {ital L}, a new compact integral formula, more suitable to analyze the nature of the Casimir force, is obtained. The force is attractive if {ital p} is odd or for very large even values of {ital p}, irrespective of {ital D}. For each small even {ital p} there exists a critical spacetime dimension {ital D}{sub {ital c}}({ital p}) such that the force is repulsive if {ital D}{lt}{ital D}{sub {ital c}} and attractive otherwise. As a consequence, the instability of the semiclassical Abraham-Lorentz-Casimir model of the electron is proved to depend on the spacetime dimensionality.
- OSTI ID:
- 5845741
- Journal Information:
- Physical Review, D (Particles Fields); (USA), Journal Name: Physical Review, D (Particles Fields); (USA) Vol. 43:4; ISSN PRVDA; ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
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