Fixed-Magnetization Ising Model with a Slowly Varying Magnetic Field

Abstract The motivation for this paper is the analysis of the fixed-density Ising lattice gas in the presence of a gravitational field. This is seen as a particular instance of an Ising model with a slowly varying magnetic field in the fixed magnetization ensemble. We first characterize the typical magnetization profiles in the regime in which the contribution of the magnetic field competes with the bulk energy term. We then discuss in more detail the particular case of a gravitational field and the arising interfacial phenomena. In particular, we identify the macroscopic profile and propose several conjectures concerning the interface appearing in the phase coexistence regime. The latter are supported by explicit computations in an effective model. Finally, we state some conjectures concerning equilibrium crystal shapes in the presence of a gravitational field, when the latter contributes to the energy only to surface order.

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Publication Details

Journal
Journal of Statistical Physics
Published
2024-10-14
DOI
https://doi.org/10.1007/s10955-024-03346-0
Citations
1
Primary Topic
Theoretical and Computational Physics
Type
article
Field-Weighted Citation Impact
0.31

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article

Fixed-Magnetization Ising Model with a Slowly Varying Magnetic Field

Yvan Velenik, Yacine Aoun, Sébastien Ott
1 citations
Journal of Statistical Physics
Theoretical and Computational Physics
0.31
article

Fixed-Magnetization Ising Model with a Slowly Varying Magnetic Field

Yvan Velenik, Yacine Aoun, Sébastien Ott
article en
1 citations

Abstract

Abstract The motivation for this paper is the analysis of the fixed-density Ising lattice gas in the presence of a gravitational field. This is seen as a particular instance of an Ising model with a slowly varying magnetic field in the fixed magnetization ensemble. We first characterize the typical magnetization profiles in the regime in which the contribution of the magnetic field competes with the bulk energy term. We then discuss in more detail the particular case of a gravitational field and the arising interfacial phenomena. In particular, we identify the macroscopic profile and propose several conjectures concerning the interface appearing in the phase coexistence regime. The latter are supported by explicit computations in an effective model. Finally, we state some conjectures concerning equilibrium crystal shapes in the presence of a gravitational field, when the latter contributes to the energy only to surface order.

Journal of Statistical PhysicsVol. 191(10)
University of Geneva (CH), École Polytechnique Fédérale de Lausanne (CH)
National Science Foundation, National Centres of Competence in Research SwissMAP, Université de Genève
Affordable and clean energy
Openalex Percentile: Top 43%
Theoretical and Computational Physics
0.31
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