Helmholtz Free Energy in the Two-Dimensional Ising Model with Defects

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY
V. V. Binkovskii, S. D. Mostovoy
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引用次数: 0

Abstract

The influence of point defects of the vacancy type on the thermodynamic properties of the two-dimensional Ising model is investigated in the paper. The main attention is paid to the comparison of two approaches to the description of the system: the traditional analysis of the internal energy \(E\) and a more complete analysis of the Helmholtz free energy \(F\) and entropy \(S\). Using Monte Carlo methods—the Metropolis algorithm and the Wang–Landau algorithm—the temperature dependences of the changes in the indicated quantities upon the introduction of defects are calculated. It is established that the interaction of defects has the character of attraction with an effective radius of \(d\approx 3\). It is shown that in the phase transition region, the free energy behaves as a continuous monotonically decreasing function of temperature, whereas the internal energy exhibits a singularity caused by the behaviour of the entropy. The possible dynamics of defects is investigated by comparing the energy of different configurations; a tendency towards defect clustering at temperatures above the critical one is observed. A comparative analysis of the accuracy and computational efficiency of both approaches is carried out.

含缺陷二维Ising模型中的亥姆霍兹自由能
研究了空位型点缺陷对二维Ising模型热力学性质的影响。重点比较了两种描述系统的方法:传统的内能分析\(E\)和更完整的亥姆霍兹自由能分析\(F\)和熵分析\(S\)。利用蒙特卡罗方法- Metropolis算法和Wang-Landau算法-计算了缺陷引入时指示量变化的温度依赖性。建立了缺陷相互作用具有吸引力的特征,有效半径为\(d\approx 3\)。结果表明,在相变区,自由能表现为温度的连续单调递减函数,而内能表现为熵的奇异性。通过比较不同构型的能量,研究了缺陷可能的动力学特性;在临界温度以上观察到缺陷聚集的趋势。对比分析了两种方法的精度和计算效率。
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来源期刊
Moscow University Physics Bulletin
Moscow University Physics Bulletin PHYSICS, MULTIDISCIPLINARY-
CiteScore
0.70
自引率
0.00%
发文量
129
审稿时长
6-12 weeks
期刊介绍: Moscow University Physics Bulletin publishes original papers (reviews, articles, and brief communications) in the following fields of experimental and theoretical physics: theoretical and mathematical physics; physics of nuclei and elementary particles; radiophysics, electronics, acoustics; optics and spectroscopy; laser physics; condensed matter physics; chemical physics, physical kinetics, and plasma physics; biophysics and medical physics; astronomy, astrophysics, and cosmology; physics of the Earth’s, atmosphere, and hydrosphere.
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