Numerical evaluation of the Casimir interaction between cylinders
- 1. Departamento de Fisica Juan Jose Giambiagi, FCEyN UBA, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellon I, 1428 Buenos Aires (Argentina)
Description
We numerically evaluate the Casimir interaction energy for configurations involving two perfectly conducting eccentric cylinders and a cylinder in front of a plane. We consider in detail several special cases. For quasiconcentric cylinders, we analyze the convergence of a perturbative evaluation based on sparse matrices. For concentric cylinders, we obtain analytically the corrections to the proximity force approximation up to second order, and we present an improved numerical procedure to evaluate the interaction energy at very small distances. Finally, we consider the configuration of a cylinder in front of a plane. We first show numerically that, in the appropriate limit, the Casimir energy for this configuration can be obtained from that of two eccentric cylinders. Then we compute the interaction energy at small distances, and compare the numerical results with the analytic predictions for the first order corrections to the proximity force approximation.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.78.085009;
- arXiv
- arXiv:0808.3368v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 78
- Journal Issue
- 8
- Journal Page Range
- p. 085009-085009.11
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41005066
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- APPROXIMATIONS; CASIMIR EFFECT; COMPARATIVE EVALUATIONS; COMPUTERIZED SIMULATION; CONFIGURATION; CONVERGENCE; CORRECTIONS; CYLINDERS; DISTANCE; FORECASTING; INTERACTIONS; NUMERICAL SOLUTION
- Descriptors DEC
- CALCULATION METHODS; EVALUATION; MATHEMATICAL SOLUTIONS; SIMULATION
Optional Information
- Notes
- (c) 2008 The American Physical Society