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Critical Casimir forces for O(n) systems with long-range interaction in the spherical limit
1Institute of Solid State Physics-BAS, 72 Tzarigradsko Chaussée, 1784 Sofia, Bulgaria. chamati@issp.bas.bg
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|February 9, 2005
Summary
We analyzed the thermodynamic Casimir force and free energy in a d-dimensional spherical model. The Casimir force is always attractive for sigma >= 1, with its behavior depending on temperature and film thickness.
Area of Science:
- Statistical Mechanics
- Condensed Matter Physics
- Critical Phenomena
Background:
- The Casimir effect describes a physical force arising from quantum fluctuations.
- Understanding thermodynamic Casimir forces is crucial for systems near critical points.
- Long-ranged interactions significantly influence system behavior at criticality.
Purpose of the Study:
- To present exact results for thermodynamic Casimir force and excess free energy.
- To investigate these quantities in a d-dimensional spherical model with power-law interactions.
- To analyze behavior near and above/below the critical temperature in a film geometry.
Main Methods:
- Utilized the d-dimensional spherical model with power-law decaying interactions (r^{-d-sigma}).
- Analyzed film geometry under periodic boundary conditions.
- Derived and investigated the universal finite-size scaling function for the Casimir force.
Main Results:
- Derived exact results for thermodynamic Casimir force and excess free energy.
- The Casimir force is shown to be universally attractive for sigma >= 1.
- Identified distinct force dependencies on film thickness (L) based on temperature relative to T(c).
Conclusions:
- The excess free energy is always negative and increases with temperature and magnetic field.
- The Casimir force is always attractive for sigma >= 1, indicating surface attraction.
- The force exhibits complex behavior at T(c), depending on sigma and magnetic field.