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Phys. Rev. B 77, 115409 (2008) [22 pages]

Thermodynamic Casimir effects involving interacting field theories with zero modes

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Daniel Grüneberg and H. W. Diehl
Fachbereich Physik, Universität Duisburg-Essen, D-47048 Duisburg, Germany

Received 22 October 2007; published 6 March 2008

Systems with an O(n) symmetrical Hamiltonian are considered in a d-dimensional slab geometry of macroscopic lateral extension and finite thickness L that undergo a continuous bulk phase transition in the limit L. The effective forces induced by thermal fluctuations at and above the bulk critical temperature Tc, (thermodynamic Casimir effect) are investigated below the upper critical dimension d*=4 by means of field-theoretic renormalization-group methods for the case of periodic and special-special boundary conditions, where the latter correspond to the critical enhancement of the surface interactions on both boundary planes. As shown previously [ Europhys. Lett. 75 241 (2006)], the zero modes that are present in Landau theory at Tc, make conventional renormalization-group-improved perturbation theory in 4−ϵ dimensions ill-defined. The revised expansion introduced there is utilized to compute the scaling functions of the excess free energy and the Casimir force for temperatures TTc, as functions of LLξ, where ξ is the bulk correlation length. Scaling functions of the L-dependent residual free energy per area are obtained, whose L→0 limits are in conformity with previous results for the Casimir amplitudes ΔC to O(ϵ3∕2) and display a more reasonable small-L behavior inasmuch as they approach the critical value ΔC monotonically as L→0. Extrapolations to d=3 for the Ising case n=1 with periodic boundary conditions are in fair agreement with Monte Carlo results. In the case of special-special boundary conditions, extrapolations to d=3 are hampered by the fact that the one-loop result for the inverse finite-size susceptibility becomes negative for some values of L when ϵ≳0.83.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.77.115409
DOI:
10.1103/PhysRevB.77.115409
PACS:
05.70.Jk, 68.35.Rh, 11.10.Hi, 68.15.+e