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Monte Carlo study of the metamagnet Ising model in a random and uniform field

Abstract

Monte Carlo simulation has been used to determine the phase diagram of a metamagnet Ising model in the presence of a random and uniform magnetic field. The model consists of a spin-1/2 metamagnet in which the nearest neighbor and next nearest neighbor spin interactions are antiferromagnetic (J1 < 0) and ferromagnetic (J2 > 0), respectively. We used a bimodal probability distribution for the random magnetic field. We have calculated the staggered magnetization and the fourth-order Binder cumulants in order to obtain the critical points. The phase diagram in the uniform field versus temperature plane presents continuous and first-order transition lines. The phase transition lines, together with the critical and tricritical points, have been obtained for several random field values.

Random field; Monte Carlo simulation; Tricritical point


Monte Carlo study of the metamagnet Ising model in a random and uniform field

A. Weizenmann; M. Godoy; A. S. de Arruda

Departamento de Física, Universidade Federal de Mato Grosso, 78060-900, Cuiabá, Mato Grosso, Brazil

ABSTRACT

Monte Carlo simulation has been used to determine the phase diagram of a metamagnet Ising model in the presence of a random and uniform magnetic field. The model consists of a spin-1/2 metamagnet in which the nearest neighbor and next nearest neighbor spin interactions are antiferromagnetic (J1 < 0) and ferromagnetic (J2 > 0), respectively. We used a bimodal probability distribution for the random magnetic field. We have calculated the staggered magnetization and the fourth-order Binder cumulants in order to obtain the critical points. The phase diagram in the uniform field versus temperature plane presents continuous and first-order transition lines. The phase transition lines, together with the critical and tricritical points, have been obtained for several random field values.

Keywords: Random field; Monte Carlo simulation; Tricritical point

I. INTRODUCTION

Random field and disordered magnetic systems have been a considerable source of research in the last years [1]. The random field Ising model (RFIM) has been one of the most interesting research topics in theoretical physics (Condensed Matter) in the last fifteen years and it occupies an important position within the physics of disordered systems [2, 3]. Basically, there are two types of disorder in the spin models: disorder bonds (type I) and randomness in the strength of the applied magnetic field (type II). The Spin Glass models, which result from the type I disorder, have been very sucessfull [4]. RFIM, in which the disorder is coupled directly to the external applied magnetic field (type II), has been shown very hard to handle. Although RFIM has deserved many investigations from both experimental and theoretical points of view [3], no significant progress has been achieved to fully understand the nature of the phase transitions and critical behavior. On the other hand, questions such as the lower critical dimension [5, 6] and the existence of a static phase transition have already been solved from the theoretical point of view. However, questions such as the existence of the tricritical point [7-11] are still open. The relevance of RFIM is due to the fact that it is the simplest model used to describe the essential physics of a rich class of experimentally accessible disordered systems, which includes: i) structural phase transitions in random alloys [12], ii) commensurate charge-density-wave systems with impurity pinning [13, 14], iii) binary fluid mixtures in random porous media [15], iv) melting of intercalates in layered compounds such as TiS2 [16], v) frustration introduced by the disorder in interacting many body systems, besides explaining several aspects of electronic transport in disordered insulators [17] and vi) systems near the metal-insulator transition [18, 19]. In the last ten years, the physics of the hysteresis, of the avalanche behavior and of the origin of self-organized criticality [20] have been modelled employing the non-equilibrium behavior of the RFIM. In particular, a new class of problems, such as self-generated glassy behavior, has been studied through the non-disordered model with infinitesimal random field [21]. Recently, random magnetic fields have been considered in metamagnet systems of Ising type. In these systems, only the competition between the ferromagnetic and antiferromagnetic ordering are interesting. However, the application of a random and uniform magnetic field can yield the appearance of new phenomena and a richer critical behavior becomes possible. This is in fact the subject of the present work.

The plan of the paper is as follows. The model and the simulation background are given in section II while the results are discussed in section III.

II. MODEL AND SIMULATION

The Hamiltonian model for the spin-1/2 Ising metamagnet can be written as

where the first and second sum run over all pairs of spin nearest neighbors ( á ij ñ ) and next nearest neighbors ( á ik ñ ), respectively, on a simple square lattice with N spins and si = ±1. J1 < 0 (antiferromagnetic) represents the nearest neighbor spin interactions and J2 > 0 (ferromagnetic) represents the next nearest neighbor spin interactions. h is the strength of the external uniform magnetic field and the random magnetic fields hi in the last sum are governed by the bimodal distribution

where hr is the strength of the random field.

To study this system we employed Monte Carlo simulation techniques [22]. We consider a square lattice of linear size L, with values of L ranging from L = 16 to L = 128, and we applied periodic boundary conditions. We prepared the system with the spins randomly distributed on the lattice. Each trial change of a spin state on the lattice is accepted according to the Metropolis prescription, w(a®a¢) = min[1,exp(-bDE)], where DE is the local energy change (E-Ea) resulting from changing the state of a random selected spin from a to a¢ state, and b = 1/kBT. To reach the equilibrium state we take, for guarantee, at least 2×105 MCs (Monte Carlo steps) for all the lattice sites we studied. Then, we take more 3×105 MCs to estimate the average values of the quantities of interest. Here, 1 MCs means L2 trials for change the state of a spin of the lattice.

We calculated the sublattice magnetizations per spin

and

The transition lines of the phase diagram were obtained from the staggered magnetization, defined as mS = (m1-m2)/2. We also calculated the reduced fourth-order Binder cumulants [23]

associated with the staggered magnetization. From the crossing point of the cumulants for different lattice sizes we determined the critical points of the model [23]. In the above expressions denotes the average over the disorder and á ¼ ñ denotes the thermal average. The average over the disorder was done using Nsamp = 100 independent samples for lattices in the range 16 < L < 128.

III. RESULTS

We present in Fig. 1 the phase diagram of the model in the plane external uniform field h versus temperature T, for three selected values of the random field hr. The phase diagram displays continuous phase transition lines which end at a tricritical point at low temperatures. The solid curves joining the square are continuous phase transition lines while the dashed lines represent first-order transitions. Circles represent the positions of the tricritical points. The points in the continuous transition lines were obtined by considering the common point where the cumulants for different lattice sizes cross. As an example, we show in Fig. 2 a typical case for hr = 0 and h = 1.0. On the other hand, the first-order transition lines were estimated by observing the discontinuity in the staggered magnetization at the transition point. An example of this is given in Fig. 3. We found the tricritical points for the following random fields (see Fig. 1): (a) hr = 0.0 (Tt = 2.52, ht = 3.90), (b) hr = 0.5 (Tt = 2.40, ht = 3.80) and (c) hr = 1.0 (Tt = 2.30, ht = 3.30). For h = 0 and different values of hr the phase diagram presents different values for the critical temperature. The result shown in (Fig. 1) is qualitatively similar to that obtained by the use of a mean-field calculation [24].




In Fig. 3 we show the behavior of the staggered magnetization ms as a function of the external uniform field h. For the set values of temperatures T = 1.5, T = 2.0, and for a random field hr = 0.0, we observe that the staggered magnetizations are discontinuous, clearly indicating the existence of a first-order phase transition. On the other hand, for the temperature T = 3.0, we can observe that a staggered magnetization vanishes continuously with the increase of the uniform field h, indicating the existence of a continuous phase transition. From the crossing of the analytical continuation of the first- and second-order lines we estimate the location of the tricritical points shown in Fig. 1.

In summary, the present Monte Carlo simulations for a metamagnet Ising model in a random and uniform field show that the phase diagram in the plane uniform field h versus temperature present continuous and first-order transition lines separated by tricritical points.

Acknowledgments

The authors acknowledge the financial support given by the Brazilian agencies CAPES, CNPq and FAPEMAT.

[1] D. P. Belanger, Braz. J. Phys. 30 682 (2000).

[2] D. P. Belanger, in Spin Glasses and Random Fields, edited by A. P. Young (World Scientific, Singapore, 1998); R. J. Birgeneau, J. Magn. Magn. Mater. 177, 1 (1998).

[3] Y. Shapir, in Recent Progress in Random Magnets, edited by D. H. Ryan (World Scientific, Singapore, 1992), pp. 309-334.

[4] J. R. L. de Almeida and D. J. Thouless, J. Phys. A 11, 983 (1978).

[5] J. Z. Imbrie, Phys. Rev. Lett. 53 1747 (1984).

[6] Y. Imry and S. K. Ma, Phys. Rev. Lett. 35 1399 (1975).

[7] A. S. de Arruda, W. Figueiredo, R. M. Sebastianes, and V. K. Saxena, Phys. Rev. B 39 4409 (1989).

[8] A. S. de Arruda and W. Figueiredo, Mod. Lett. B 11 (21,22) 973 (1997).

[9] D. F. de Albuquerque and A. S. de Arruda, Physica A 316 13 (2002).

[10] D. C. Mattis, Phys. Rev. Lett. 55 3009 (1985).

[11] A. Aharohy, Phys. Rev. B 18 3318 (1978).

[12] J. R. Childress and C. L. Chien, Phys. Rev. B 43, 8089 (1991).

[13] D. S. Fisher, Phys. Rev. Lett. 50, 1486 (1983).

[14] D. S. Fisher, Phys. Rev. B 31, 1396 (1985).

[15] J. V. Maher, W. I. Goldburg, D. W. Pohlm and M. Lanz, Phys. Rev. Lett. 53, 60 (1984).

[16] R. M. Suter, M. W. Shafer, P. M. Hornm and P. Dimon, Phys. Rev. B 26, 1495 (1982).

[17] A. L. Efros and B. L. Shklovskii, J. Phys. C 8, L49 (1975).

[18] T. R. Kirkpatrick and D. Belitz, Phys. Rev. Lett. 73, 862 (1994).

[19] A. A. Pastor and V. Dobrosavljevi\'c, Phys. Rev. Lett. 83, 4642 (1999).

[20] A. A. Pastor, V. Dobrosavljevi\'c, and M. L. Horbach, Phys. Rev. B 66 014413 (2002).

[21] M. Mezard, Physica A 265, 352 (1999).

[22] D. P. Landau and K. Binder, A Guide to Monte Carlo Simulations in Statistical Physics (Cambridge University Press, United Kingdom, 2000).

[23] K. Binder and D. W. Heermann, Monte Carlo Simulation in Statistical Physics. An Introduction, 3rd ed. (Springer, Berlin, 1997).

[24] S. Galam, C. S. O. Yokoi, and S. R. Salinas, Phys. Rev. B 57, 8370 (1998).

Received on 30 September, 2005

  • [1] D. P. Belanger, Braz. J. Phys. 30 682 (2000).
  • [2] D. P. Belanger, in Spin Glasses and Random Fields, edited by A. P. Young (World Scientific, Singapore, 1998);
  • R. J. Birgeneau, J. Magn. Magn. Mater. 177, 1 (1998).
  • [3] Y. Shapir, in Recent Progress in Random Magnets, edited by D. H. Ryan (World Scientific, Singapore, 1992), pp. 309-334.
  • [4] J. R. L. de Almeida and D. J. Thouless, J. Phys. A 11, 983 (1978).
  • [5] J. Z. Imbrie, Phys. Rev. Lett. 53 1747 (1984).
  • [6] Y. Imry and S. K. Ma, Phys. Rev. Lett. 35 1399 (1975).
  • [7] A. S. de Arruda, W. Figueiredo, R. M. Sebastianes, and V. K. Saxena, Phys. Rev. B 39 4409 (1989).
  • [8] A. S. de Arruda and W. Figueiredo, Mod. Lett. B 11 (21,22) 973 (1997).
  • [9] D. F. de Albuquerque and A. S. de Arruda, Physica A 316 13 (2002).
  • [10] D. C. Mattis, Phys. Rev. Lett. 55 3009 (1985).
  • [11] A. Aharohy, Phys. Rev. B 18 3318 (1978).
  • [12] J. R. Childress and C. L. Chien, Phys. Rev. B 43, 8089 (1991).
  • [13] D. S. Fisher, Phys. Rev. Lett. 50, 1486 (1983).
  • [14] D. S. Fisher, Phys. Rev. B 31, 1396 (1985).
  • [15] J. V. Maher, W. I. Goldburg, D. W. Pohlm and M. Lanz, Phys. Rev. Lett. 53, 60 (1984).
  • [16] R. M. Suter, M. W. Shafer, P. M. Hornm and P. Dimon, Phys. Rev. B 26, 1495 (1982).
  • [17] A. L. Efros and B. L. Shklovskii, J. Phys. C 8, L49 (1975).
  • [18] T. R. Kirkpatrick and D. Belitz, Phys. Rev. Lett. 73, 862 (1994).
  • [19] A. A. Pastor and V. Dobrosavljevi\'c, Phys. Rev. Lett. 83, 4642 (1999).
  • [20] A. A. Pastor, V. Dobrosavljevi\'c, and M. L. Horbach, Phys. Rev. B 66 014413 (2002).
  • [21] M. Mezard, Physica A 265, 352 (1999).
  • [22] D. P. Landau and K. Binder, A Guide to Monte Carlo Simulations in Statistical Physics (Cambridge University Press, United Kingdom, 2000).
  • [23] K. Binder and D. W. Heermann, Monte Carlo Simulation in Statistical Physics. An Introduction, 3rd ed. (Springer, Berlin, 1997).
  • [24] S. Galam, C. S. O. Yokoi, and S. R. Salinas, Phys. Rev. B 57, 8370 (1998).

Publication Dates

  • Publication in this collection
    16 Oct 2006
  • Date of issue
    Sept 2006

History

  • Received
    30 Sept 2005
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