Fluctuation-induced forces in periodic slabs: Breakdown of epsilon expansion at the bulk critical point and revised field theory

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Published 14 June 2006 2006 EDP Sciences
, , Citation H. W. Diehl et al 2006 EPL 75 241 DOI 10.1209/epl/i2006-10090-0

0295-5075/75/2/241

Abstract

Systems described by n-component ϕ4 models in a d − 1×L slab geometry of finite thickness L are considered at and above their bulk critical temperatureTc,. The renormalization-group improved perturbation theory commonly employed to investigate the fluctuation-induced forces ("thermodynamic Casimir effect") in d = 4 − epsilon bulk dimensions is re-examined. It is found to be ill-defined beyond two-loop order because of infrared singularities when the boundary conditions are such that the free propagator in slab geometry involves a zero-energy mode at bulk criticality. This applies to periodic boundary conditions and the special-special ones corresponding to the critical enhancement of the surface interactions on both confining plates. The field theory is reorganized such that a small-epsilon expansion results which remains well behaved down to Tc,. The leading contributions to the critical Casimir amplitudes Δper and Δsp,spbeyond two-loop order are ∼ (u*)(3 − epsilon)/2, whereu* = O(epsilon) is the value of the renormalized ϕ4 coupling at the infrared-stable fixed point. Besides integer powers of epsilon, the small-epsilon expansions of these amplitudes involve fractional powers epsilonk/2, with k ⩾ 3, and powers of ln epsilon. Explicit results to order epsilon3/2 are presented for Δper and Δsp,sp, which are used to estimate their values at d = 3.

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10.1209/epl/i2006-10090-0