Published March 15, 2010 | Version v1
Journal article

Casimir force at a knife's edge

  • 1. Department of Physics, Middlebury College, Middlebury, Vermont 05753 (United States)
  • 2. Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)
  • 3. Laboratoire de Physique Theorique et Modeles Statistiques, CNRS UMR 8626, Batiment 100, Universite Paris-Sud, 91405 Orsay cedex (France)
  • 4. Institut fuer Theoretische Physik, Universitaet zu Koeln, Zuelpicher Strasse 77, 50937 Koeln (Germany)
  • 5. Center for Theoretical Physics and Laboratory for Nuclear Science, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)

Description

The Casimir force has been computed exactly for only a few simple geometries, such as infinite plates, cylinders, and spheres. We show that a parabolic cylinder, for which analytic solutions to the Helmholtz equation are available, is another case where such a calculation is possible. We compute the interaction energy of a parabolic cylinder and an infinite plate (both perfect mirrors), as a function of their separation and inclination, H and θ, and the cylinder's parabolic radius R. As H/R→0, the proximity force approximation becomes exact. The opposite limit of R/H→0 corresponds to a semi-infinite plate, where the effects of edge and inclination can be probed.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
81
Journal Issue
6
Journal Page Range
p. 061701-061701.5
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42005782
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
ANALYTICAL SOLUTION; APPROXIMATIONS; CASIMIR EFFECT; COMPUTERIZED SIMULATION; CYLINDERS; EQUATIONS; INCLINATION; INTERACTIONS; PLATES
Descriptors DEC
CALCULATION METHODS; MATHEMATICAL SOLUTIONS; SIMULATION

Optional Information

Notes
(c) 2010 The American Physical Society