Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/28
Title: Critical Casimir effect in the Ising strips with standard normal and ordinary boundary conditions and the grain boundary
Authors: Borjan, Zoran 
Keywords: Casimir effect;Distant-wall corrections;Grain boundary;Ising strip
Issue Date: 15-Sep-2016
Journal: Physica A: Statistical Mechanics and its Applications
Abstract: 
We consider critical Casimir force in the Ising strips with boundary conditions defined by standard normal and ordinary surface universality classes containing also the internal grain boundary. Using exact variational approach of Mikheev and Fisher we have elaborated on behaviors of Casimir amplitudes Δ++(g), ΔOO(g) and Δ+O(g), corresponding to normal-normal, ordinary-ordinary and mixed normal-ordinary boundary conditions, respectively, with g as a strength of the grain boundary. Closed analytic results describe Casimir amplitudes Δ++(g) and ΔOO(g) as continuous functions of the grain boundary's strength g, changing the character of the Casimir force from repulsive to attractive and vice versa for certain domains of g. Present results reveal a new type of symmetry between Casimir amplitudes Δ++(g) and ΔOO(g). Unexpectedly simple constant result for the Casimir amplitude Δ+O(g)=π/12 we have comprehensively interpreted in terms of equilibrium states of the present Ising strip as a complex interacting system comprising two sub-systems. Short-distance expansions of energy density profiles in the vicinity of the grain boundary reveal new distant-wall correction amplitudes that we examined in detail. Analogy of present considerations with earlier more usual short-distance expansions near one of the (N), (O) and (SB) boundaries, as well as close to surfaces with variable boundary conditions refers to the set of scaling dimensions appearing in the present calculations but also to the discovery of the de Gennes-Fisher distant wall correction amplitudes.
URI: https://physrep.ff.bg.ac.rs/handle/123456789/28
ISSN: 0378-4371
DOI: 10.1016/j.physa.2016.04.002
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