PHYSICAL REVIEW B VOLUME 60, NUMBER 1 1 JULY 1999-I Tetragonal equilibrium states of iron P. M. Marcus and V. L. Moruzzi IBM Research Division, T.J. Watson Research Center, Yorktown Heights, New York 10598 S.-L. Qiu Department of Physics, Alloy Research Center, Florida Atlantic University, Boca Raton, Florida 33431-0991 ~Received 6 January 1999! First-principles total-energy calculations on tetragonal Fe show that the ferromagnetic and antiferromagnetic phases have tetragonal equilibrium states with c/a.1, the fcc value. The bulk layers of an epitaxial film of Fe on Cu~001!, which are almost fcc with the Cu lattice constant, are shown to be stable in the antiferromagnetic phase, but inherently unstable in the ferromagnetic phase. The structure of tetragonal equilibrium antiferromagnetic Fe is estimated to be a53.47 Å, c53.75 Å. @S0163-1829~99!04125-9# I. INTRODUCTION The electronic structure of bulk Fe is especially interesting because of the rich variety of states it exhibits. Thus, Fe exists in both bcc and fcc structures and has many magnetic phases. This work examines the behavior of Fe in the more general case of tetragonal atomic structure and looks for metastable equilibrium tetragonal states of Fe in various magnetic phases. The results show the existence of noncubic tetragonal equilibrium states in both the ferromagnetic ~FM! and antiferromagnetic ~AF! phases with comparable energies. First-principles calculations of fcc Fe based on the KohnSham equations1 indicate that the lowest energy state is nonmagnetic ~NM! with lattice constant a53.44 Å ~WignerSeitz radius r WS52.54 a.u.). The FM and AF energy and moment curves of Ref. 1, Fig. 2, which include the type-I AF phase @alternating moments on ~001! planes#, have been verified many times.2–4 Figure 1 is a calculation using the augmented spherical wave method of Ref. 1, but now based on a four-atom cell ~two adjacent bcc cells!, which gives the calculation greater stability, especially near phase transitions. The second-order phase transition to the AF phase from the NM phase is found to occur at a slightly expanded r WS ~0.4%! than the NM minimum, as shown by the position of the abrupt rise of the local moment of the AF phase. Figure 1 applies to the bulk layers of Fe films of 5–10 atomic layers grown in coherent epitaxy on Cu~001! at room temperature, since the bulk layers are very nearly fcc at the Cu lattice constant5 a53.61 Å, r WS52.67 a.u. with c/a50.98. Although Fig. 1 shows the NM phase has the minimum energy state of fcc Fe at a53.44 Å, it is wrong to think of this state as the lowest equilibrium state of Fe near the fcc structure. A simple symmetry argument based on Fig. 1 shows that the energy E of the AF phase can be reduced below the fcc NM minimum by tetragonal deformation. The minimum energy NM and AF states of fcc Fe are nearly degenerate, but the E of the AF state will vary linearly with tetragonal deformation @ DE}D(c/a) # since the AF state does not have cubic symmetry, whereas the NM state does have cubic symmetry, hence will be flat under tetragonal deformation @ DE}„D(c/a)…2 # . Then in one direction of te0163-1829/99/60~1!/369~4!/$15.00 PRB 60 tragonal deformation the E of the AF state E AF will go below the E of the NM state E NM. Later it is shown that increase of c/a by 8% lowers E AF by about 4 mRy/atom, whereas E NM has a minimum at c/a 51 and actually increases when c/a changes from 1. Hence epitaxial tensile strain exerted by Cu~001! on the Fe film strains the tetragonal equilibrium state nearly into constrained fcc Fe at the Cu lattice constant and the fcc calculation of Fig. 1 applies. Thus at r WS52.67 a.u. Fig. 1 shows the AF phase below the FM phase by about 3 mRy/atom and below the NM phase by about 4 mRy/atom, in agreement FIG. 1. Energies (E2E 0 ) mRy per atom relative to the energy minimum and magnetic moments per atom in Bohr magnetons m B of the nonmagnetic ~NM!, high-spin ferromagnetic ~FM!, and type-I antiferromagnetic ~AF! phases of fcc Fe as functions of WignerSeitz radius r WS . Calculated with a four-atom cell, the augmented spherical wave method and the fixed spin-moment procedure from the spin-polarized Kohn-Sham equations. 369 ©1999 The American Physical Society 370 P. M. MARCUS, V. L. MORUZZI, AND S.-L. QIU PRB 60 FIG. 3. Relative energy per atom (E2E 0 ) of Fe relative to FM energy at the experimental volume V511.53 Å 3 as a function of c/a, where a5a 8 & is the fct basal plane lattice constant. The NM ~h!, FM ~circle!, and AF ~3! points are from the first-principles calculations of Peng and Jansen ~Ref. 11!. The curves are interpolated between the calculated points to show the two minima in the AF and FM curves, particularly the tetragonal minima at 1.08 ~AF! and 1.20 ~FM! that give equilibrium states. FIG. 2. ~a! Constant energy contours ~small dashes!, two energy minima ~•! and saddle point ~3! of vanadium V on the tetragonal plane, coordinates c/a 8 and V/V 0 , where a 8 is the body-centeredtetragonal basal plane lattice constant and V 0 is the bcc reference volume 12.57 Å3. The dashed lines bound the region of inherent instability and the full line is the epitaxial Bain path ~EBP! of states produced by isotropic epitaxial strain on the equilibrium states at the two minima. ~b! Energy per atom E(c/a) along the EBP ~full line! and E(c/a) at volume V51.04V 0 ~dashed line!. The plots show that c/a 8 is the same at the minima and saddle points of the two curves and E is slightly greater at the minima of the dashed curve. of FM Fe, but without the complications of separating the other phases that occur in Fe. Figure 2~a! shows contour lines ~short dashes! on which E(a,c) is constant in the tetragonal plane which has coordinates c/a 8 and V/V 0 ; a 8 and c are tetragonal lattice constants @a 8 is the lattice constant of the square cross section of a body-centered-tetragonal ~bct! description, and a5a 8 & is the lattice constant for a face-centered-tetragonal ~fct! description#. Figure 2 uses the bct description; Figs. 3 and 4 use the fct description. V is the volume per atom5c/a 8 2 /2 5ca 2 /4, and V 0 is the reference volume—for vanadium V 0 is the bcc value 12.57 Å3. The contour lines in Fig. 2~a! show there are two minima with measurements which show6 the bulk of the film to be AF. Section II uses the theory of tetragonal structures in Refs. 7 and 8 to deduce the metastable tetragonal equilibrium structures of both AF and FM Fe from first-principles calculations and elastic and structural measurements. In Sec. III the stability of the AF phase and instability of the FM phase of Fe on Cu~001! are shown. Problems that need further study are indicated. II. DETERMINATION OF TETRAGONAL EQUILIBRIUM STATES Finding the tetragonal equilibrium states of Fe requires knowledge of some features of tetragonal structure which are discussed in detail in Ref. 7. Figure 2 illustrates the characteristic behavior of tetragonal states by showing the behavior of nonmagnetic tetragonal vanadium. Figure 2~a! is adapted from Ref. 7 ~Fig. 1! by the addition of the energy curves in Fig. 2~b!; both figures are based on the first-principles calculations of tetragonal states in Ref. 8. The tetragonal behavior of V is described here because it is very close to the behavior FIG. 4. Part of the tetragonal plane of Fe showing the LEED point ~3!, the EBP in linear elastic approximation, slope 21.92 Å3, ~full line! and tetragonal equilibrium state of AF Fe at c/a51.08, V511.34 Å 3 ~circle!. Assuming the FM phase has the same equilibrium V at c/a51.20 ~h! and that the FM EBP has the same slope as the AF EBP, then the FM EBP is the dashed line through the FM equilibrium point. The FM EBP intersects the line on the tetragonal plane on which a53.61 Å ~slope a 3 /4511.76 Å 3 ) at the point c/a51, V511.76 Å 3 ~n!, hence the FM Fe phase on Cu~001! is fcc with the Cu lattice constant. PRB 60 TETRAGONAL EQUILIBRIUM STATES OF IRON of E ~•! and a saddle point ~3!. These are general features of tetragonal structures.8,9 The minima are the equilibrium states of vanadium V; the lower minimum is at the bcc state, hence the ground state is bcc. The higher minimum is a noncubic equilibrium state at c/a 8 51.78 which has actually been observed when stabilized by coherent epitaxy of V on Ni~001! and on Cu~001!.10 Around the minima are states of constrained stability, such as those constrained by epitaxy. The solid line which passes through the minima and the saddle point is the epitaxial Bain path ~EBP!, which gives all the constrained states of V produced by isotropic epitaxial ~two-dimensional! strain on the equilibrium states. A point on the EBP for Fe will describe the structure of the bulk layers of an Fe film epitaxial on Cu~001!. However, as will be shown, the magnetic phase must be specified. Reference 7 shows that the region between the two lines of long dashes in Fig. 2~a!, in which the saddle point is central, contains inherently unstable tetragonal states. Such states cannot be stabilized by applied stresses, in contrast to the constrained states around the minima mentioned above, which are outside this unstable region. This behavior of tetragonal states will be used later to determine the stabilities of the magnetic states of Fe on Cu~001!. Reference 7 also gives a formula for the slope of the EBP, which will be used later; at cubic points it is S dV d ~ c/a ! D 52 EBP 2 ~ 122 n ! V , ~ 11 n !~ c/a ! ~1! where n is the Poisson ratio of the cubic material ~for stresses along a cubic axis!. In Fig. 2~b! the solid curve is the energy per atom along the EBP, E EBP(c/a), and the dashed curve is the energy per atom at a constant V51.04V 0 as a function of c/a, E V (c/a). This V is about 2% higher than the equilibrium V at c/a 8 51.78. Determination of the Fe tetragonal equilibrium states requires the feature shown in Fig. 2~b!, namely that the c/a values of the minima and of the saddle points of the two curves coincide. This correspondence of the c/a values is due to c/a and V being orthogonal coordinates at cubic stationary points and nearly orthogonal at noncubic stationary points @Ref. 7, Eq. ~7!#. Also note that the E values at the minima of E V (c/a) are only slightly higher than at the minima of E EBP(c/a), since E is flat around the minima. The available information on the energies of tetragonal Fe from first principles consists of the work of Peng and Jansen,11 who calculated some values of E V (c/a) for the AF, FM, and NM phases of E. They used the full-potential linearized plane wave method including relativistic corrections and solved the spin-polarized Kohn-Sham equations with the von Barth–Hedin exchange correlation interaction, but without nonlocal corrections like the generalized gradient approximation ~GGA!. Also they used the experimental volume per atom of the bulk of the Fe film on Cu~001!, V 511.53 Å 3 . Their results, replotted from Table I of Ref. 11, FM are shown in Fig. 3. The E AF V (c/a) and E V (c/a) curves are notably different. Both show the characteristic two minima of tetragonal structures. The FM curve resembles E V (c/a) for vanadium with the ground state at the bcc structure and the second minimum at large c/a 8 51.70 (c/a51.20). The fragment of E NM V (c/a) is enough to show a minimum at 371 c/a51, the fcc point, as anticipated in Sec. I. The AF curve has a minimum at c/a51.08, also as anticipated in Sec. I. Thus these constant-volume energy curves locate an equilibrium state of the AF phase at c/a51.08, c/a 8 51.53, and of the FM phase at c/a51.20, c/a 8 51.70. However the values of V, hence of a and c separately, of the equilibrium states are not yet known. To find V for the equilibrium state of the AF phase we use the structure measured by quantitative low-energy electron diffraction ~LEED! analysis5 of Fe on Cu~001!, which gives the bulk structure of the film as a53.61 Å, c53.54 Å, thereby giving a point at c/a50.98, V511.53 Å 3 on the EBP of AF Fe. Then we use Eq. ~1! at the fcc point to find the slope of the EBP as 21.92 Å3, on using the measured Poisson ratio12 of g-Fe n 50.44 and V511.50 Å 3 ~slightly smaller at c/a51 compared to V at c/a50.98) to draw the EBP shown in Fig. 4. At c/a51.08 the EBP has V 511.34 Å 3 , hence a53.47 Å, c53.75 Å at the tetragonal AF equilibrium point. An estimate of a and c for the tetragonal FM equilibrium state, where no LEED structure is available, can be made with the plausible assumption that the equilibrium value of V is the same as that for the AF phase, 11.34 Å3. Then with c/a51.20 the FM equilibrium tetragonal lattice constants are a53.35 Å, c54.02 Å. For both the AF and FM phases we have used the minima of E V (c/a) at a V 2% larger than the equilibrium V’s to find the c/a of the equilibrium states, the same volume difference as was illustrated for V in Fig. 2~b!. III. DISCUSSION Section II shows that enough information is now available to make a reasonable estimate of the structures of the metastable tetragonal equilibrium states of both the AF and FM phases of Fe. First-principles total-energy calculations were combined with measured epitaxial film lattice constants and measured elastic constants of g-Fe. To check these structures in a consistent calculation free of the various assumptions used, requires direct evaluation from first principles of the EBP’s of Fe in the AF, FM, and NM phases, as was done for FM Co in Ref. 13. The AF phase with equilibrium in-plane lattice constant a53.47 Å requires a 4% isotropic epitaxial tensile strain to be grown epitaxially on Cu~001!, producing a nearly fcc Fe lattice at the Cu lattice constant, a53.61 Å, r WS52.67 a.u. Hence, the fcc calculation of Fig. 1 applied to the bulk of the film on Cu~001! shows that the AF phase is lowest in energy, consistent with observations on the films.6 The existence of a nearly fcc Fe lattice at the Cu lattice constant a Cu is thus a happy coincidental result of a Cu 53.61 Å. An exact fcc Fe lattice would be produced on a substrate with a53.58 Å, since the AF EBP of Fe in Fig. 4 shows V511.50 Å 3 5a 3 /4 at c/a51. Note that diamond has a53.57 Å and epitaxial Fe films have been shown to grow well on diamond~001!.14 However no magnetic measurements were made on the films, The FM equilibrium phase at a53.35 Å requires a 7.8% tensile strain to be epitaxial on Cu~001!. The EBP of FM Fe is drawn as a straight line in Fig. 4 ~long dashes! through the point c/a51.20, V511.34 Å 3 assuming the same slope as the AF phase, i.e., assuming the same Poisson ratio. At c/a 372 P. M. MARCUS, V. L. MORUZZI, AND S.-L. QIU 51 the FM phase then has V511.75 Å 3 , which gives a5c 53.61 Å, hence the FM phase is even closer to fcc than the AF phase. Although both phases are seen to be fcc on Cu~001!, Fig. 3 shows an important difference between the AF and FM films on Cu~001!. Namely, the FM phase has cubic symmetry at the fcc point ~in a collinear description!. At a structure with cubic symmetry the energy has an extremum, hence change of the energy is second order, i.e., flat, with respect to deformations of the structure. Therefore E FM V (c/a) by symmetry is flat at the fcc point in a collinear description. Moreover, the flat shown in Fig. 3 at the fcc point is actually a maximum at c/a51. Then, as noted in Sec. II, the E EBP also has a maximum at c/a51 and E FM(a,c) has a saddle point at c/a51. This means that the FM phase of Fe on Cu~001! is in the middle of the unstable region and is inherently unstable. However, the AF phase, which has ~001! planes with alternating moments, does not have cubic symmetry at the fcc point, since the @001# direction is then different from the @100# and @010# directions. Hence, the AF EBP varies linearly at c/a51 ~and also at 0.98!, and the saddle point is far removed at c/a50.71. Thus, the AF phase of Fe on Cu~001! is a constrained stable state. Note also in Fig. 3 that the AF energy at c/a50.98 is about 4 mRy/atom above the minimum E at c/a51.08, as was noted in Sec. I. This difference in the stability of the AF phase compared to the FM phase of Fe films on Cu~001! is consistent with the observation that AF films grow easily to 10 layers, whereas FM films do not grow thicker than 4 layers, which then have no bulk layers.15 If a substrate could be found with a closer 1 V. L. Moruzzi, P. M. Marcus, and J. Kübler, Phys. Rev. B 39, 6957 ~1989!. 2 T. Asada and K. Terakura, Phys. Rev. B 46, 13 599 ~1992!. 3 T. Kraft, P. M. Marcus, and M. Scheffler, Phys. Rev. B 49, 11 511 ~1994!. 4 M. Uhl, L. M. Sandratski, and J. Kübler, Phys. Rev. B 50, 291 ~1994!. 5 S. H. Lu, J. Quinn, D. Tian, F. Jona, and P. M. Marcus, Surf. Sci. 209, 364 ~1989!; H. Landskron, G. Schmidt, K. Heinz, K. Müller, C. Stuhlmann, U. Beckers, M. Wuttig, and H. Ibach, ibid. 256, 115 ~1991!; M. Wuttig and J. Thomassen, ibid. 282, 237 ~1993!. 6 Dongqi Li, M. Freitag, J. Pearson, Z. Q. Qiu, and S. D. Bader, Phys. Rev. Lett. 73, 3112 ~1994!; R. D. Ellerbock, A. Fuest, A. Schatz, W. Keune, and R. A. Brand, ibid. 74, 3053 ~1995!. 7 P. M. Marcus and P. A. Alippi, Phys. Rev. B 57, 1971 ~1998!. 8 V. L. Sliwko, P. Mohn, K. Schwarz, and P. Blaha, J. Phys.: Condens. Matter 8, 799 ~1996!. 9 P. J. Craievich, M. Weinert, J. M. Sanchez, and R. E. Watson, Phys. Rev. Lett. 72, 3076 ~1994!; Phys. Rev. B 55, 787 ~1997!. 10 ~V/Ni! Y. Tian, F. Jona, and P. M. Marcus, Phys. Rev. B 58, PRB 60 to 3.35 Å, the FM phase might be stabilized, although Fig. 3 shows its minimum energy is 3 mRy/atom higher than the AF minimum. When Fe is grown epitaxially on substrates with c/a sufficiently below 1 to be outside the unstable region, the FM state is a constrained stable state of bcc Fe and is more stable than the AF state, as is shown in Fig. 3. This strained state of bcc Fe was found to occur for Fe/Rh~001! ~Ref. 16! (c/a50.82), for Fe/Cu3Fe(001) ~Ref. 17! (c/a 50.72), for Fe/Ag~001! ~Ref. 18! (c/a50.70), and for Fe/ Pd~001! ~Ref. 19! (c/a50.79). Recent work has shown that fcc Fe at the Cu lattice constant has additional magnetic phases with still lower energies than the AF phase shown in Fig. 1. Thus a noncollinear spin-spiral magnetic phase has been found,4 which branches off below the AF phase. Also, an AF phase with a longer period ~moment sequence ↑↑↓↓ on four successive layers! has been found.20 It remains to be seen whether tetragonal deformation of these phases brings them below the energy minimum at c/a51.08 of the simple ~type-I! AF phase considered here. ACKNOWLEDGMENTS P.M.M. thanks M. Scheffler of the Fritz-Haber Institute, Berlin, Germany and J. Kirschner of the Mikrostrukturphysik Institute, Halle, Germany for hospitality during the writing of this paper. P.M.M. and V.L.M. thank IBM for providing facilities. S.-L.Q. is grateful to NSF for research funds ~Contract Nos. DMR-9120120 and 9500654!. Some of the calculations were carried out using the computational resources provided by the MDRCF, which is funded jointly by the NSF and FAU. 14 051 ~1998!; ~V/Cu! Y. Tian, F. Jona, and P. M. Marcus ~unpublished!. 11 S. S. Peng and H. J. F. Jansen, J. Appl. Phys. 69, 6132 ~1991!. 12 J. Zarestky and C. Stassis, Phys. Rev. 35, 4500 ~1957!. 13 P. Alippi, P. M. Marcus, and M. Scheffler, Phys. Rev. Lett. 78, 3892 ~1997!. 14 H. A. Hoff, G. L. Waytena, J. W. Glesener, V. G. Harris, and D. P. Pappas, Surf. Sci. 326, 252 ~1995!. 15 S. Müller, P. Bayer, C. Reischl, K. Heinz, B. Feldmann, H. Zillgen, and M. Wuttig, Phys. Rev. Lett. 74, 765 ~1994!. 16 A. M. Begley, S. K. Kim, F. Jona, and P. M. Marcus, Phys. Rev. B 48, 1786 ~1993!. 17 B. Schirmer, B. Feldmann, and M. Wuttig, Phys. Rev. B 58, 4984 ~1998!. 18 H. Li, Y. S. Li, J. Quinn, D. Tian, J. Sokolov, F. Jona, and P. M. Marcus, Phys. Rev. B 42, 9195 ~1990!. 19 J. Quinn, Y. S. Li, H. Li, D. Tian, F. Jona, and P. M. Marcus, Phys. Rev. B 43, 3959 ~1991!. 20 M. van Schilfgarde, V. P. Antropov, and B. N. Harmon, J. Appl. Phys. 79, 4799 ~1996!; V. P. Antropov, M. I. Katsnelson, B. N. Harmon, M. van Schilfgarde, and D. Kusnezov, Phys. Rev. B 54, 1019 ~1996!.
© Copyright 2026 Paperzz