Phys. Rev. E 78, 011124 (2008) [9 pages]Casimir energies: Temperature dependence, dispersion, and anomaliesReceived 18 February 2008; revised 5 May 2008; published 25 July 2008 Assuming the conventional Casimir setting with two thick parallel perfectly conducting plates of large extent with a homogeneous and isotropic medium between them, we discuss the physical meaning of the electromagnetic field energy Wdisp when the intervening medium is weakly dispersive but nondissipative. The presence of dispersion means that the energy density contains terms of the form d[ωε(ω)]∕dω and d[ωμ(ω)]∕dω. We find that, as Wdisp refers thermodynamically to a nonclosed physical system, it is not to be identified with the internal thermodynamic energy U following from the free energy F, or the electromagnetic energy W, when the last-mentioned quantities are calculated without such dispersive derivatives. To arrive at this conclusion, we adopt a model in which the system is a capacitor, linked to an external self-inductance L such that stationary oscillations become possible. Therewith the model system becomes a nonclosed one. As an introductory step, we review the meaning of the nondispersive energies, F, U, and W. As a final topic, we consider an anomaly connected with local surface divergences encountered in Casimir energy calculations for higher space-time dimensions, D>4, and discuss briefly its dispersive generalization. This kind of application is essentially a generalization of the treatment of Alnes et al. J. Phys. A 40 F315 (2007) to the case of a medium-filled cavity between two hyperplanes. © 2008 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevE.78.011124
DOI:
10.1103/PhysRevE.78.011124
PACS:
05.30.−d, 42.50.Lc, 11.10.Wx, 78.20.Ci
See AlsoComment: Finn Ravndal, Comment on “Casimir energies: Temperature dependence, dispersion, and anomalies”, Phys. Rev. E 79, 053101 (2009). |
