1 Introduction

Abstract

The phase transition to ferromagnetic order in itinerant ferromagnetic superconductor UGe as function of pressure shows change of phase transition order. At low temperature and high pressure the transition is of first order and at pressure of about 1.42 GPa the order changes to second. On the basis of Landau expansion of free energy up to the sixth order in magnetization we calculate the phase diagram taking into account the magneto-elastic interaction as the mechanism responsible for this change.
We propose a simple Stoner-like dependence of the Curie temperature on the pressure and present the results for measurable thermodynamic quantities as the entropy jump at the first order phase transition.

Some remarks on the magnetic phase diagram of ferromagnetic superconductor UGe

Diana V. Shopova

Collective Phenomena laboratory, G. Nadjakov Institute of Solid State Physics,

Bulgarian Academy of Sciences, BG-1784 Sofia, Bulgaria.

E-mail: sho@issp.bas.bg
Key words: Ginzburg-Landau theory, superconductivity, ferromagnetism, magnetization.
PACS: 74.20.De, 74.20.Rp, 74.40-n, 74.78-w.

1 Introduction

The coexistence of ferromagnetism and bulk superconductivity in Uranium-based intermetallic compound, UGe [1, 2] has been a subject of intensive research since its discovery. The experimental results show that the UGe is an itinerant ferromagnet with orthorhombic symmetry and can be well described as uniaxial ferromagnet of Ising type. The superconducting phase exists entirely within the ferromagnetic domain at low temperature and pressure interval between 1.0 1.5 GPa. At T=0 and ambient pressure UGe orders ferromagnetically through second order phase transition with Curie temperature of T = 52 K. There are two distinct ferromagnetic phases usually denoted by FM2 and FM1 with different magnitude of magnetic moments. With increasing pressure,the magnetic ground state switches from a highly polarized phase (FM2, M 1.5 B) to a weakly polarized phase (FM1, M 0.9 B) at pressure of P 1.2 GPa. When the pressure is increased the order of transition from paramagnetic to FM1 changes from second to first at the tricritical point T on the T(P) diagram, and at some critical pressure P, the ferromagnetic order disappears. Detailed description of P-T phase diagram of UGe can be found in [3]; schematic illustration is given in Fig. 1.

Figure 1: An illustration of phase diagram of UGe: FM1 - high-pressure ferromagnetic phase, FM2 - low-pressure ferromagnetic phase, SC-phase of coexistence of ferromagnetism and superconductivity. and are the respective magnetic phase transition lines; is tricritical point; is the critical pressure, at which the ferromagnetic order disappears.

The steep drop of T(P) to zero at the critical pressure P in UGe is generally agreed to be an evidence of first order phase transition to the paramagnetic phase, see for example [4, 5] and is of great interest as a candidate for quantum critical point  [6]. Recently Mineev [7] reexamined the development of instability with respect to the continuous type of transition from paramagnetic phase to FM1 on the basis of magneto-elastic mechanism, treating it in mean-field approach. The influence of pressure on magnetic fluctuations close to the critical point leads only to weak first-order transition at P in contradiction to the experimental results, [5]. Mineev made an estimate of the theoretical results with the experimentally obtained parameters for UGe and concluded that most likely the order of the phase transition is changed from second to first because the coefficient before the fourth order term in Landau expansion of the free energy may become negative due to interaction of magnetic and elastic degrees of freedom.
In this paper we shall study within the phenomenological Landau energy the effect of pressure and compressibility on the phase transition order from paramagnetic phase to FM1 in UGe by including a sixth order term in the Landau expansion of the magnetic free energy and considering the possible change with the pressure of the sign of parameter at the forth order in magnetization.

2 Landau free energy

In previous papers [8, 9] we derived and applied Ginzburg-Landau free energy of UGe in the following form:

(1)

where, f is the free energy density describing pure superconducting system:

(2)

with the superconducting order parameter, and are the standard Landau parameters; the terms with and represent the anisotropy of spin triplet Cooper pairs and crystal anisotropy, respectively. The ferromagnetic energy density up to the forth order in magnetization is denoted by f

(3)

where , and . f stands for the interaction between superconducting and magnetic order parameters:

(4)

The pressure effect in (1) was included phenomenologically only through the linear dependence of temperature of ferromagnetic transition on pressure. This simple free energy gives surprisingly good general results in description of UGe phase diagram and its comparison to the experimental data. The temperature of transition to the phase of coexistence of superconductivity and ferromagnetism in UGe is always lower than the Curie temperature, a fact that confirms the idea of superconductivity that is triggered by the spontaneous magnetization M. That is why the detailed description of the purely magnetic phase transitions is very important for the construction of the total phase diagram. The most substantial deviations from the experimental for UGe given by the free energy (1) are two: the first is concerned with the overestimation of the critical pressure where the superconductivity appears for the first time when lowering the temperature, which is represented by a maximum on the phase diagram - see Fig.1. This is likely due to the fact that magnetic free energy, (3) does not properly describe the whole magnetic phase diagram of UGe, especially the presence of two magnetic phases, as the phase transition between the two magnetic phases is at pressure, very close to the pressure of superconducting transition. This problem is widely discussed in the literature and needs additional studies. Another feature that is lacking in the description by free energy (1) is the change of order from second to first of the transition from paramagnetic to ferromagnetic ordering of FM1.
Taking into account the arguments of Mineev [7] about the instability of second order transition to ferromagnetic ordering in UGe due to the strong dependence of Curie temperature on pressure which may lead to change of the sign of in (3) from to positive to negative, we will consider in detail this effect. Moreover, the neutron scattering experiments of lattice expansion [10] show that the magnetoelastic coupling in UGe is strong with substantial influence on the phase transitions.
We expand the magnetic part of Ginzburg-Landau energy to sixth order in magnetization and take into account the lowest order of interaction between the magnetic and elastic degrees of freedom. As UGe is highly anisotropic uniaxial ferromagnet without loss of generality we may write that . In the absence of shear deformation magnetic part of free energy will become:

(5)

The variable is the relative volume change, M is the magnetization, is the bulk modulus. We assume that the parameters and do not depend on temperature and pressure, so and , where and . The dependence of is given by the relation . The term is the coupling energy between magnetization and the relative volume change with coupling parameter . Similar form of the magnetic free energy is proposed in [11], where a first order phase transition due to effect of compressibility is discussed for transition metals Ni, Fe, Co.
We minimize the energy (5) with respect to relative volume change in absence of shear deformation, and obtain:

(6)

Thus the coupling of magnetic and elastic degrees of freedom modifies the coefficient in front of the fourth order term in (6) and it may become negative if:

The coupling parameter is the slope of volume dependence [12], or , and using the relation , it can be written in the form:

(7)

Therefore, in certain range of temperatures and pressures the ferromagnetic ordering may occur through first order phase transition from the disordered phase. This depends crucially on the steepness of the function , which is measured by the derivative of with respect to pressure. The experiments [13] show, for example, that the Stoner-Wohlfarth theory for weak itinerant ferromagnets can fairly well describe the behavior of magnetization with pressure in low-pressure ferromagnetic phase, denoted in Fig. 1 as FM2. There the pressure derivative will take the form:

(8)

and is connected to the microscopic model used for calculation of Eq.(8). From the above relation it is straightforwardly seen that the dependence of on pressure will be proportional to , where is the critical pressure of disappearance of ferromagnetism. This Stoner dependence of on pressure renormalizes the parameter in front of the forth order term in magnetization in (6) in the following way:

(9)

where . It is obvious that can become negative which leads to instability of second order phase transition, but the above relation can hardly be applied to the description of the first order phase transition from paramagnetic to FM1 phase as close to , the parameter from (9) becomes divergent and grows in unlimited way. So Stoner-Wohlfarth theory can hardly be directly applied to the description of the first order phase transition in its original form. Here we will use the interpolation approach, proposed in [15] for the dependence of Curie temperature of the second-order phase transition on pressure, which is a solution of the following equation:

(10)

In the above equation and ; the dimensionless variable, , is defined by with the critical pressure, at which the ferromagnetic ordering disappears. The quantity is the measure that accounts for the spin fluctuations with respect to the single particle Stoner excitations. The limit gives the Stoner dependence of the critical temperature on pressure, and means that the spin fluctuations determine .

3 Results and discussion

The experiments show that for and the phase transition from paramagnetic phase to FM1 phase is of second order, and using that, we can write the free energy (6) in dimensionless form:

(11)

where, is the magnetization at , ; and . The dimensionless critical temperature, , obtained from equation (10) will be:

(12)

The parameter in front of the forth order term of the free energy (11) becomes:

(13)

where and is the specific heat jump of the second order phase transition at . For pressures in the interval , the parameter . The equality is fulfilled for pressure of the tricritical point and there . For UGe the tricritical pressure according to the different experimental data, namely GPa and GPa.
The equation of state for free energy (11) will be:

(14)

with one stable solution:

(15)

existing for . It is seen from the above relation that for , the magnetization will be positive at and its jump at will be:

The equilibrium temperature for the first order phase transition is determined in the standard way by finding the minimum of free energy (11) or , with given by Eq. (15). With the help of equation of state, (14) we obtain for the equilibrium energy:

(16)

For

(17)

and paramagnetic and FM1 phase coexist. In the interval of temperatures , the FM1 phase is stable. For UGe the calculations with the experimental data available, give that which according to [15] means that the Stoner mechanism is prevailing with corrections from spin fluctuations. The numerical estimate of with this value of gives that the equilibrium temperature of first order phase transition is K at the measured critical pressure of GPa. The dimensionless latent heat , at the first-order transition temperature , see Eq. (17), is given by . At the critical pressure , the numerical value of is 0.11.
The crucial point in the description of the first-order phase transition from paramagnetic to FM1 phase is the explicit dependence of Curie temperature on pressure. Recently in [16], the pressure coefficient of Curie temperature is calculated from microscopic model numerically. The results show that depends in a complex way on two terms coming from the derivatives of Fermi temperature and exchange integral with pressure, respectively. But these results cannot be applied directly in phenomenological analysis. More theoretical calculations are needed in this respect as the first order of the phase transition is also important for the understanding of phase of coexistence of superconductivity and ferromagnetism.

4 Conclusion

The presented phenomenological analysis shows that the account of compressibility to the lowest order in the relative volume change can explain the first order phase transition between FM1 and paramagnetic phase in UGe. The use of phenomenological interpolation relation derived in [15] adequately describes qualitatively the first order phase transition. In order to properly understand the nature of the this transition, more precise microscopic calculation are needed for the dependence of Curie temperature on pressure in the high-pressure ferromagnetic phase of UGe.

References

  1. S. S. Saxena, P. Agarwal, K. Ahilan, F. M. Grosche, R. K. W. Haselwimmer, M.J. Steiner, E. Pugh, I. R. Walker, S.R. Julian, P. Monthoux, G. G. Lonzarich, A. Huxley. I. Sheikin, D. Braithwaite, and J. Flouquet, Nature (London) 406 (2000) 587.
  2. A. Huxley, I. Sheikin, E. Ressouche, N. Kernavanois, D. Braithwaite, R. Calemczuk, and J. Flouquet, Phys. Rev. B 63 (2001) 144519.
  3. Dai Aoki, Frédéric Hardy, Atsushi Miyake, Valentin Taufour, Tatsuma D. Matsuda, Jacques Flouquet, Comptes Rendus Physique 12 (2011) 573.
  4. C. Plfleider and A. D. Huxley, Phys. Rev. Letters 89 (2002) 147005
  5. Christian Pfleiderer, Rev. Mod. Phys. 81 1551–1624 (2009)
  6. Hisashi Kotegawa, Valentin Taufour, Dai Aoki, Georg Knebe, and Jacques Flouquet, J. Phys. Soc. Jpn. 80 (2011) 083703
  7. V. P. Mineev, Journal of Physics: Conference Series 400 (2012) 032053
  8. M. G. Cottam, D. V. Shopova and D. I. Uzunov, Phys. Lett. A 373 (2008) 152
  9. D. V. Shopova and D. I. Uzunov, Phys. Rev. B 79 (2009) 064501
  10. D A Sokolov, R Ritz, C Peiderer, T Keller and A D Huxley, Journal of Physics: Conference Series 273 (2011) 012085
  11. Sen Yang, Xiaobing Ren and Xiaoping Song, Phys. Rev. B 78 (2008) 174427
  12. C. P. Bean and D. S. Rodbell, Phys. rev. 126 (1962) 104
  13. N. Aso, G. Motoyama, Y. Uwatoko, S. Ban, S. Nakamura, T. Nishioka, Y. Homma, Y. Shiokawa, K. Hirota, and N.K. Sato, Phys.Rev. B 29 (2006) 054512
  14. E. P. Vohlfarth, Physica B+C 91 (1977) 305
  15. P. Mohn and E. P. Wohlfarth, Journal de Physique,Colloque C8, 49 (1988) 83
  16. R Konno and N Hatayama, J. Phys: Conf. Series 400 (2012) 032041
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
107435
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description