Omelyan I P, Mryglod I M, Folk R, Fenz W
Institute for Condensed Matter Physics, 1 Svientsitskii Street, UA-79011 Lviv, Ukraine.
Phys Rev E Stat Nonlin Soft Matter Phys. 2004 Jun;69(6 Pt 1):061506. doi: 10.1103/PhysRevE.69.061506. Epub 2004 Jun 16.
The phase behavior of Ising spin fluids is studied in the presence of an external magnetic field with the integral equation method. The calculations are performed on the basis of a soft mean spherical approximation using an efficient algorithm for solving the coupled set of the Ornstein-Zernike equations, the closure relations, and the external field constraint. The phase diagrams are obtained in the whole thermodynamic space including the magnetic field H for a wide class of Ising fluid models with various ratios R of the strengths of magnetic to nonmagnetic Yukawa-like interactions. The influence of varying the inverse screening lengths z(1) and z(2), corresponding to the magnetic and nonmagnetic Yukawa parts of the potential, is investigated too. It is shown that changes in R as well as in z(1) and z(2) can lead to different topologies of the phase diagrams. In particular, depending on the value of R, the critical temperature of the liquid-gas transition either decreases monotonically, behaves nonmonotonically, or increases monotonically with increasing H. The para-ferro magnetic transition is also affected by changes in R and the screening lengths. At H=0, the Ising fluid maps onto a simple model of a symmetric nonmagnetic binary mixture. For H--> infinity, it reduces to a pure nonmagnetic fluid. The results are compared with available simulations and the predictions of other theoretical methods. It is demonstrated that the mean spherical approximation appears to be more accurate compared with mean field theory, especially for systems with short ranged attraction potentials (when z(1) and z(2) are large). In the Kac limit z(1), z(2) -->+0, both approaches tend to nearly the same results.
采用积分方程方法研究了外磁场作用下伊辛自旋流体的相行为。计算基于软平均球近似,使用一种高效算法来求解耦合的奥恩斯坦 - 泽尔尼克方程、封闭关系和外场约束。对于具有各种磁相互作用与非磁汤川型相互作用强度比(R)的广泛伊辛流体模型,在包括磁场(H)的整个热力学空间中获得了相图。还研究了对应于势的磁和非磁汤川部分的逆屏蔽长度(z(1))和(z(2))变化的影响。结果表明,(R)以及(z(1))和(z(2))的变化会导致相图的不同拓扑结构。特别是,根据(R)的值,液 - 气转变的临界温度要么随(H)增加单调降低、非单调变化,要么单调增加。顺 - 铁磁转变也受到(R)和屏蔽长度变化的影响。在(H = 0)时,伊辛流体映射到对称非磁二元混合物的简单模型。当(H\to\infty)时,它简化为纯非磁流体。将结果与现有的模拟以及其他理论方法的预测进行了比较。结果表明,与平均场理论相比,平均球近似似乎更准确,特别是对于具有短程吸引势的系统(当(z(1))和(z(2))较大时)。在卡茨极限(z(1), z(2)\to +0)时,两种方法趋于几乎相同的结果。