Phys. Rev. E 79, 041103 (2009) [16 pages]Casimir force in O(n) systems with a diffuse interfaceReceived 23 June 2008; revised 25 November 2008; published 3 April 2009 We study the behavior of the Casimir force in O(n) systems with a diffuse interface and slab geometry ∞d−1×L, where 2<d<4 is the dimensionality of the system. We consider a system with nearest-neighbor anisotropic interaction constants J∥ parallel to the film and J⊥ across it. We argue that in such an anisotropic system the Casimir force, the free energy, and the helicity modulus will differ from those of the corresponding isotropic system, even at the bulk critical temperature, despite that these systems both belong to the same universality class. We suggest a relation between the scaling functions pertinent to the both systems. Explicit exact analytical results for the scaling functions, as a function of the temperature T, of the free energy density, Casimir force, and the helicity modulus are derived for the n→∞ limit of O(n) models with antiperiodic boundary conditions applied along the finite dimension L of the film. We observe that the Casimir amplitude ΔCasimir(d∣J⊥,J∥) of the anisotropic d-dimensional system is related to that of the isotropic system ΔCasimir(d) via ΔCasimir(d∣J⊥,J∥)=(J⊥∕J∥)(d−1)∕2ΔCasimir(d). For d=3 we derive the exact Casimir amplitude ΔCasimir(3,∣J⊥,J∥)=[Cl2(π∕3)∕3−ζ(3)∕(6π)](J⊥∕J∥), as well as the exact scaling functions of the Casimir force and of the helicity modulus Υ(T,L). We obtain that βcΥ(Tc,L)=(2∕π2)[Cl2(π∕3)∕3+7ζ(3)∕(30π)](J⊥∕J∥)L−1, where Tc is the critical temperature of the bulk system. We find that the contributions in the excess free energy due to the existence of a diffuse interface result in a repulsive Casimir force in the whole temperature region. © 2009 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevE.79.041103
DOI:
10.1103/PhysRevE.79.041103
PACS:
05.20.−y, 05.50.+q, 75.10.Hk
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