Elastic and magnetic effects on the infrared phonon spectra of MnF{}_{2}

Elastic and magnetic effects on the infrared phonon spectra of MnF

Abstract

We measured the temperature dependent infrared reflectivity spectra of MnF between 4 K and 600 K. We show that the phonon spectrum undergoes a clear renormalization at . The ab-initio calculation we performed on this compound accurately predicts the magnitude and the direction of the changes in the phonon parameters across the antiferromagnetic transition, showing that they are mainly induced by the magnetic order. In this material, we found that the dielectric constant is mostly from phonon origin. The large change in the lattice parameters with temperature seen by X-ray diffraction as well as the A phonon softening below indicate that magnetic order induced distortions in MnF are compatible with the ferroelectric instabilities observed in TiO, FeF and other rutile-type fluorides. This study also shows the anomalous temperature evolution of the lower energy mode in the paramagnetic phase, which can be compared to that of the phonon seen by Raman spectroscopy in many isostructural materials. This was interpreted as being a precursor of a phase transition from rutile to CaCl structure which was observed under pressure in ZnF.

pacs:
63.20.kk, 78.30.-j, 63.20.dk, 75.85.+t, 63.20.-e

I Introduction

In magnetoelectric multiferroic materials, ferroelectricity coexists with a magnetic order. Based on the origin and strength of the coupling between the ferroelectric and the magnetic order parameters, these materials can be divided up into two general classes.Khomskii (2009) In type-I multiferroics, such as BiFeO,Smolenskii and Chupis (1959); Kiselev et al. (1963) ferroelectric and (anti)ferromagnetic transitions are independent and weakly coupled. In type-II multiferroics, such as TbMnO,Kimura et al. (2003) ferroelectricity is a consequence of the magnetic ordering and a strong magneto-electric coupling is present. In the latter compounds, the interaction between magnetic ordering and the lattice may generate the structural distortions leading to the appearance of a permanent electrical polarization. Although the microscopic origins for this magnetoelectric coupling are still under debate, the appearance of an electrical dipole moment has important consequences on the polar, infrared active, phonon spectra. Very few studies of the phonon changes in these type-II multiferroics exist to date. Nevertheless, Schmidt et al.Schmidt et al. (2009) showed that in TbMnO phonon parameters are renormalized by about 1–2% and that the changes are linked to rather than the ferroelectric transition.

Before tackling the structurally complex type-II multiferroics, it is interesting to see the effect of magnetic ordering on the infrared phonon response. Several infrared studies on spinels,Wakamura and Arai (1988); Rudolf et al. (2007); Sushkov et al. (2005) showed that the magnetic ordering leads to infrared phonon splitting. However, the phonon splitting has systematically been attributed to the magnetic frustration present in these compounds, a vision supported by ab-initio calculations.Fennie and Rabe (2006) Previous studies on antiferromagnetic MnO (Ref. Rudolf et al., 2008) and CoO (Ref. Kant et al., 2008) showed a strong phonon renormalization at . However, both materials also undergo a structural phase transition from cubic to rhombohedral (MnO) or tetragonal (CoO) at . These phase transitions make it harder to separate what is the pure magnetic effect on phonons from what is due to the structural symmetry change.

In this perspective, manganese fluoride (MnF) emerges as a system of choice, once it is a very well characterized commensurate antiferromagnet with  K.Katsumate (2000) Its simple paramagnetic rutile structureStout and Reed (1954) (/mnm or D) remains the same below , where the spins align antiferromagnetically along the axis. Hence effects on the phonon spectra have a magnetic origin.

Temperature dependent Raman spectra of MnF show phonon frequency changes at .Lockwood and Cottam (1988) As this material has an inversion center, Raman active phonons are not infrared active and vice versa. Therefore, detailed knowledge of infrared phonons in MnF is paramount to grasp changes that would affect dielectric ordering below . We expect that these data on MnF help to set a baseline to understand the effect on phonons of the magnetic transitions in type-II multiferroic materials.

To date, only the room temperature infrared phonon spectra have been measured for MnF.Weaver et al. (1974) According to dilatometric measurementsGibbons (1959) MnF lattice parameters are renormalized across the antiferromagnetic transition. This magnetostrictive effect is the hallmark of the coupling between dipole excitations and magnetic order in this compound.

Although MnF is a classical antiferromagnet, it is closely related to multiferroic materials. Its isostructural compound TiO is a quantum paraelectric (incipient ferroelectric) as determined by infrared,Gervais and Piriou (1974a) Raman and dielectric measurements,Samara and Peercy (1973) as well as ab-initio calculations.Montanari and Harrison (2004) Similar responses, in particular renormalization of the phonon spectra, were observed in other rutile fluorides such as FeF,Lockwood et al. (1983) ZnF,Giordano and Sauvajol (1988) and NiF.Lockwood (2002)

In this paper we show a detailed, temperature-dependent infrared study of the phonon spectra in MnF along the -plane and the -axis. Our results show that the phonon spectra have marked changes at . The infrared data are complemented by low temperature X-ray diffraction and ab-initio calculations. First principles calculations predict the proper phonon frequencies for both directions and find the correct frequency shifts at . Our results show that the dielectric constant of MnF is mostly from phonon origin. The large change in the lattice parameters with temperature and phonon softening in the antiferromagnetic phase suggest that MnF distortions are compatible with the ferroelectric instabilities observed in TiO,Montanari and Harrison (2004) FeF,Lockwood et al. (1983) and ZnF.Giordano and Sauvajol (1988)

Ii Methods

The MnF single crystal used in this experiment was grown by the Czochralski method. X-ray and infrared measurements were done on different platelets cut from the same bulk and containing and planes. The sample for optical measurements was polished with a 15 wedge to avoid interference fringes from the back surface reflectance. The measured faces for both optical samples were polished with 1m diamond powder to a mirror like surface. Typical sample surface sizes are  mm. Their antiferromagnetic transition was measured on a Quantum Design MPMS-5 squid magnetometer with a magnetic field of 1000 gauss. Figure 1 shows the magnetic susceptibility () measured with the field applied parallel and perpendicular to the c axis. The curve shows a classical antiferromagnetic ordering behavior where decreases below reaching a vanishingly small value at  K. This indicates a negligible amount of impurities in this sample. When , is dominated by a spin canting response below .

Figure 1: (color online) Magnetic susceptibility of MnF measured with gauss. The solid (blue) line is the data for and the dashed (red) line is obtained for . The diagram represents the lattice and magnetic structure of the rutile tetragonal phase, where  Å and  Å.

We measured the infrared reflectivity spectra near normal incidence at 31 different temperatures between 4 K and 300 K, on the plane sample with the electric field of light parallel and perpendicular to the direction ( axis). To determine the absolute reflectivity, we used an in situ gold overfilling technique.Homes et al. (1993) The sample is attached to a cold finger of an ARS Helitran cryostat and we measure its reflectivity with respect to a reference stainless mirror for all temperatures. We then evaporate a thin layer of gold on the sample producing a mirror with the same surface quality and shape as the sample. The reflectivity of this gold mirror is measured, at several temperatures, against the same stainless steel reference and the infrared spectrum is obtained by dividing the uncoated sample by its coated version. Finally, we multiply the result by the absolute reflectivity of gold to get the absolute reflectivity of the sample. The accuracy of the absolute reflectivity is better than 1% and the relative error between different temperatures is of the order of 0.1%. The far infrared (10–700 ) data were collected with a Bruker IFS113v interferometer. Higher frequency spectra (500–7500 ) were obtained with a Bruker IFS66v spectrometer. In the overlapping region the spectra agree within 0.5%.

We also measured the reflectivity of the sample, in the (100–700 ) range, at high temperatures (300–600 K) with a TS-1500 Linkam hot stage. No polarization was used in these measurements as and are equivalent axes. An Al mirror served as a reference. As no in situ gold evaporation was used above room temperature, the data were corrected so that 300 K measurements in the cryostat and in the hot stage match.

X-ray diffraction measurements were carried out on the National Synchrotron Light Source beamline X21. A Si(111) double-crystal monochromator was used to set the incident energy of the beam to 11.5 or 13.5 keV, and a Pt-coated mirror focused the beam down to (vertical) by (horizontal) mm. The MnF crystals were inserted in an Oxford superconducting magnet, which is mounted on a 2-circle diffractometer with a horizontal scattering geometry. A LiF(200) analyzer was used, and two parallel reflections were measured for both and plane samples to obtain the and c lattice parameters.

These measurements were complemented with ab-initio density functional (DFT) calculations. In order to study the effects of the magnetic order on the phonon parameters, we performed the geometry optimization and phonon calculations for two different spin configurations. The first one is a true ferromagnetic (FM) configuration with all spins aligned. The second configuration is a pseudo-antiferromagnetic (AFM) configuration where nearest neighbor spins are anti-aligned, as shown in Fig. 1 (up-down configuration). This configuration is only pseudo-antiferromagnetic since it is not an eigenfunction of the total spin operator. The true antiferromagnetic state is a superposition of the up-down and down-up configurations, as well as quantum fluctuations on them. Such a correct calculation is unfortunately not feasible for an infinite system. The calculations were done using the CRYSTAL06 package.Dovesi et al. (2006) Three different functionals were used for the calculations, namely LDA, and two hybrid functionals B3LYPBecke (1993) and B1PW.Bilc et al. (2008) An atomic basis set of valence 2- qualityMartin and Sundermann (2001) and small core pseudopotentialsPseudo : Dolg et al. (1987) were used for the Mn ions and an all electrons basis of 3- quality was used for the F ions.Prencipe et al. (1995) As usual, the LDA functional underestimates the lattice parameters by a few percent while the two other functionals slightly overestimate them. The best fit is reached for the B1PW functional with an error of 0.2% in the direction and 1% in the direction. All ab-initio results further presented in the paper will thus refer to the B1PW functional.

Iii Results

The solid lines in the top panel of Fig. 2 show the infrared reflectivity at selected temperatures with the electric field of light lying on the -plane. These spectra show three clear phonon peaks. The solid lines in the bottom panel are the reflectivity for and show a single phonon along this direction. The infrared modes found agree with group theory predictions. Indeed, the irreducible representation decomposition for the rutile structure is . Four of these modes are Raman active — , , and  — and four are IR active — . The modes are degenerate and represent the plane spectra. From low to high frequencies, we define these modes as , , and . The mode has symmetry and is the only phonon along the axis.

Figure 2: (color online) Reflectivity with light polarized in the -plane (top panel) and along the -axis (bottom panel) for MnF. The solid lines are experimental results and the dotted lines are Lorentz fits using Eq. 1. In each panel, the dashed line is the reflectivity predicted by ab-initio calculations. These curves were generated by plugging into Eq. 1 the first principles values for and and using the values obtained from the experimental fits at 5K. The ab-initio values come from the AFM calculation.

To extract quantitative information from these data, we simulated the spectra with a multiple Lorentz oscillator model for the dielectric function:

(1)

where is the contribution from electronic transitions to the dielectric function, and each phonon is described by a resonance frequency , an oscillator strength , and damping . The reflectivity at normal incidence is given by .

Typical fitting results are shown as dotted lines in both panels of Fig. 2. Overall, the model reproduces the data very well. However, modes and , as well as at high temperatures, have structures that cannot be reproduced by the Lorentz model. This structure is likely related to a breakdown of the harmonic approximationSun et al. (2008) and/or two-phonon absorption,Benoit and Giordano (1988) even though we cannot rule out the presence of a small symmetry breaking lattice distortion. Nevertheless, in general, the parameters obtained through a Lorentz modeling of the data assuming a symmetry are a very good first approximation.

To ascertain that this is the case with our data, we also used Kramers-Kronig transformations, which are model independent. These transformations require knowledge of the reflectivity in the full spectral range, from zero to infinity. As our measurement range is limited, we extrapolated the low frequency range as a constant reflectivity. For high frequencies we used a constant up to 80 000  followed by a free-electron approximation (). The 80 000  limit was chosen to avoid unphysical negative values (albeit within error bars) in the imaginary part of the dielectric function ().

In Fig. 3 we compare Kramers-Kronig results to Lorentz fit parameters. The left panel shows for the mode. For clarity, each curve was normalized by its maximum value and shifted vertically by an amount proportional to its temperature. The peak in happens at the phonon resonance frequency. The squares are the frequencies obtained from the Lorentz fits to the data. Although a small difference in frequency is seen, both methods give the same temperature dependence and magnitude of the changes in the phonon features. The right panel presents the same comparison for the lone phonon. This figure shows that, even though Eq. 1 neglects anharmonic effects, its outcoming parameters are representative of the physical properties of MnF. We also checked that comparison of the Lorentz fits to other methods such as four-parameter simulationsGervais and Piriou (1974b) and multi-oscillator fitsKuzmenko (2005) give the same results. Henceforth we will discuss our results using the Lorentz oscillator model alone.

Figure 3: (color online) The left panel shows spectra obtained by Kramers-Kronig transformation (solid curves) for phonon and the right panel for phonon . For clarity, each curve was normalized by its maximum value then shifted vertically by a value proportional to its temperature (the curves are placed so that their maxima coincide with the temperature scale shown). The squares are frequencies obtained from the Lorentz fits and are shown in a temperature vs. frequency plot. In a perfect agreement between Lorentz and Kramers-Kronig analysis, each square would sit exactly on the maximum of a curve.

We performed ab-initio calculations to predict the values of infrared active phonon frequencies and oscillator strengths. The results of these calculations for the infrared active modes are shown as dashed lines in both panels of Fig. 2. For reference, the results for all modes are given in the appendix. The ab-initio frequencies are between 2 and 12% higher than the measured ones. Except for the very weak phonon, the predicted strenghs are underestimated by 4% to 35%. Nevertheless, the calculated spectra describe very well the overall phonon response. Table 1 summarizes the fitting parameters produced by Eq. 1 at 5 K, 100 K and 300 K. It also shows the ab-initio results for and in the FM and AFM configurations defined in Sec. II.

5K 100K 300K AFM FM
Table 1: Lorentz fit parameters at 5 K, 100 K and 300 K and ab-initio results for the phonon frequencies and oscillator strengths. Units for and are . FM and AFM configurations are defined in Sec. II. Fitted values for are 2.16 for the -plane and 2.25 along the axis.

X-ray diffraction results are presented on Fig 4 where we plot the relative change of both lattice parameters as a function of temperature. We also plot in this figure the relative change in the unit cell volume given by . The lattice parameter, as expected, increases monotonically with temperature. The AFM transition has a clear effect on this parameter which shows a kink at . The most striking feature of this plot is the anomalous behavior of the lattice parameter which increases with decreasing temperature and shows absolutely no feature at . Despite the anomalous axis behavior, the total volume of the lattice still increases with increasing temperature. It is also worth mentioning that no change was observed on lattice parameters when a 3 T magnetic field is applied.

Figure 4: (color online) Relative changes in and lattice parameters measured by x-ray diffraction. We also show the resulting relative variation of the unit-cell volume (open triangles).

Iv Discussion

As a general rule, a crystalline lattice will contract upon cooling the sample. At a magnetic transition further modifications of the crystalline parameters are induced by the magnetic energy change. Indeed, following the classical work of Baltensperger and Helman Baltensperger and Helman (1968) one can derive the modification of the lattice parameters induced by the magnetic ordering (at a given temperature below ) by the minimization of the free energy (). Below , the entropy term of the free energy is negligible and can be written as the sum of the magnetic () and the elastic () energies. A Taylor’s expansion of as a function of the lattice parameters and yields

(2)

where are the lattice parameters at in the antiferromagnetic phase. Naming the lattice parameters at the same temperature in an hypothetic paramagnetic phase, one gets

(3)

and thus

(4)

The elastic energy per unit cell can be estimated following the classical way of Ref. Baltensperger and Helman, 1968:

(5)

where is the unit cell volume and the compressibility coefficient.

Figure 5 and Tab. 2 show the definitions for the local quantification axes (, and ) of each Mn atom in the unit cell framework. The local Mn plane is defined by the in-plane (equatorial) fluorine atoms of the distorted octahedra (shown as the thick line in Fig. 5), which have the strongest metal-ligand interactions. Note that the two manganese atoms of the unit cell have different local quantification axes. Using this definition, the magnetic energy can be expressed as

(6)

It is important to notice that in the case of MnF, where the interactions are antiferromagnetic, both and are negative. can be decomposed into its main superexchange coupling. Using the local quantification axes defined in Fig. 5 and Tab. 2, we determined the superexchange coupling paths and their associated perturbative contributions pictured in Tab. 3. The sum of these terms leads to:

(7)

and represent the apical and equatorial Mn–F distances. is the angle Mn–F–Mn. Although the absolute values of the coefficients are difficult to determine, we can estimate their relative values. We found . Therefore the last two terms in Eq.7 dominate the value of .

Direction in the unit cell framework
Local axes Mn Mn
Table 2: Local quantification axes of the two Mn atoms in the unit cell. The unit cell framework is expressed in terms of its main , and directions, whereas , and refer to the local Mn quantification axes.
Figure 5: (color online) Structure of MnF highlighting the two possible orientations for the MnF coordination octahedra. The thick dark lines connect the in-plane F atoms. The local quantification axes orientations for Mn and Mn atoms are shown as black arrows. The lattice coordinates framework is defined by the arrows labeled , and .
AFM coupling path contribution scales as
( order perturbation)
Table 3: Main AFM coupling paths between adjacent Mn atoms. The Mn orbitals are written in terms of their local axes (see Tab. 2 and Fig. 5) and the F orbitals in terms of Mn local axes. The vertical and horizontal axes in pictures correspond to the and lattice directions, respectively.

We can use the above equations to obtain a rough evaluation of the derivatives in Eq. 4. We find that the first derivatives are of the same sign and order of magnitude. This is also the case for and . On the contrary, is nearly an order of magnitude larger than the other second derivative and of opposite sign. The reason is that only in the latter term magnetic and elastic contributions do not contribute with opposite signs. These estimations lead to a very weak value for , while is much larger and of opposite sign, in agreement with the x-ray measurements shown in Fig. 4.

As the atoms get closer to each other, the interaction forces between them get stronger and, in the harmonic approximation, so does the spring constant () between ions. As phonon frequencies follow ( being a reduced mass), in a first approximation we expect them to follow the thermal evolution of the unit cell volume. Figure 4 shows that the volume of the MnF lattice increases with temperature. Therefore, we expect phonon frequencies to decrease with increasing temperature. Figures 6 and 7 show the thermal evolution of phonon frequencies for MnF. Phonons and show the expected frequency softening with increasing temperature over the whole measured range. Phonon also behaves conventionally, but only above .

Figure 6: (color online) Evolution of the ab plane phonon frequencies with temperature. The red arrows indicate the ab-initio predictions for the change in frequencies (numerically indicated as the values) upon formation of an antiferromagnetic order. The shaded area is the antiferromagnetic phase. For each vibration mode, we represent the atomic motions of manganese and fluorine ions. The dotted lines are guides to the eye showing the high temperature extrapolations of the phonons behavior in the absence of magnetic ordering.
Figure 7: (color online) Evolution of the axis phonon frequency with temperature. The red arrow indicates the value of the change in frequency when the antiferromagnetic order appears, as predicted by ab-initio calculations. The shaded area is the antiferromagnetic phase. The atomic motions of manganese and fluorine ions are given for this vibration mode. The dotted line is a guide to the eye showing the high temperature extrapolation of the phonon behavior in the absence of magnetic ordering.

Phonon , on the other hand, has an anomalous thermal evolution as its frequency softens with decreasing temperature. This behavior is analogous to that reported for the mode seen by Raman spectroscopy in MnF (Ref. Lockwood and Cottam, 1988) and other rutile type fluorides such as ZnF,Giordano and Sauvajol (1988) FeF,Lockwood et al. (1983) NiF,Lockwood (2002) and MgF.Perakis et al. (1999) This mode seems to be more influenced by the parameter rather than the whole unit cell volume. The unconventional lattice parameters thermal evolution and this anomalous phonon behavior are strong indications of large lattice instabilities.

The existence of these lattice instabilities is emphasized by Raman scattering under pressure. In ZnF the softening of the Raman mode with decreasing temperature is also observed by applying pressure at room temperature. This pressure induced phonon softening is a precursor of a phase transition from rutile to a CaCl structure at 4.5 GPa.Perakis et al. (2005) Brillouin scattering measurementsYamaguchi et al. (1992) showed that MnF also undergoes a phase transition at 1.49 GPa, whose nature was inconclusive. Since the transition in ZnF is accompanied by an orthorhombic distortion of the lattice, we can interpret the mode softening in MnF as a precursor of a (incipient) phase transition. Further insight on this transition is given by measurements of the elastic properties in rutiles. MelcherMelcher (1970) showed that the elastic constant in MnF has one anomaly at and another, unrelated to magnetism, at lower temperatures. RimaiRimai (1977) observed a similar low temperature accident in the non magnetic rutile ZnF and concluded that it was representative of a structural instability compatible with ferroelectricity. Hence, although only new measurements will be able to settle the issue, it is reasonable to expect that the high pressure transition in MnF is of (incipient) ferroelectric character.

Figures 6 and 7 show that at the AFM transition, there is a clear renormalization of the phonon spectra. Mode shows an additional increase in its frequency below . This is an effect compatible with the magnetostrictive kink observed in the lattice volume, which decreases faster below . There is no noticeable change in the behavior of phonon . A puzzling behavior is observed for phonons and . The phonon softening instability observed in mode stops at and the frequency of this phonon increases notably with the appearance of the AF phase. Conversely, the thermal evolution of mode reverses, and this phonon shows a frequency softening below , which is at odds with the lattice volume evolution. As no lattice parameter show a sign change in their thermal behavior at , the sign change in the slope of the thermal evolution of these two phonon modes is likely due to effects other than conventional magnetostriction, such as exchange between ions.

To grasp further insight on this phonon behavior, we can look into ab-initio results. The paramagnetic phase is not accessible to ab-initio calculations. We considered that the average of calculations in the AFM and FM configurations are representative of the paramagnetic phase. The difference in the phonon frequencies between the AFM and “paramagnetic” calculations are indicated by the vertical arrows in Figs. 6 and 7. It is remarkable that not only do ab-initio calculations predict the correct magnitude for the phonon frequency shifts, but also they find the proper sign for these changes. It is important to remark that ab-initio calculations are done at 0 K. Hence, its predictions for phonon changes are not due to lattice modifications but are representative of a direct coupling of the phonons to the magnetic ordering, without the need of mediation by elastic lattice distortions.

Ab-initio calculations also yield the normal mode eigenvectors. One can thus analyze the effect of the displacements associated with these phonon modes on the magnetic coupling constant. The infrared active normal modes are shown in Figs. 6 and 7. The thermal evolution of all phonons in the paramagnetic phase, including the anomalous softening when lowering the temperature of the mode is probably dominated by the elastic energy. Indeed, the same behavior is observed in the Raman spectra of the mode of MgF (Ref. Perakis et al., 1999) and the infrared response of the mode of ZnF (Ref. Giordano and Sauvajol, 1987), both non magnetic fluorides, isostructural to MnF.

In order to understand the sign change in the thermal evolution of phonons and below , we have to look at the free energy . In the AFM phase, the dominant term in the changes of the free energy of the system is the magnetic energy , given by Eq. 6. Thus, minimization of goes through the minimization of . Let us look into the contribution coming from phonons and to this term. The mode corresponds to a large displacement in the and directions of the F atoms bridging two MnF octahedra. Let us define as the magnetic coupling between the Mn atom and the Mn atoms located at the crystallographic positions and ; as the coupling between Mn and the Mn atoms located at and ; and as the coupling between Mn and the Mn atoms located at , , and . Under a phonon displacement of amplitude , the magnetic energy is modified as follows

(8)

is the value of the magnetic exchange with the atoms in their equilibrium position. We should stress, again, that both and the spin correlation terms are negative because of the AFM interaction. Using the perturbative expressions of Tab. 3 one can show that does not depend on the displacement , that , and that . In the AFM phase the magnetic energy must be minimized, and thus, the modulus of the first factor of Eq. 8 must increase. As the second derivative and have opposite signs, increasing the modulus of the first factor implies that the oscillation amplitude must decrease. In a equivalent view, one can note that the second derivative term acts as a correction to the full harmonic potential of the phonon. For phonon it introduces a positive correction to the effective phonon spring constant, i.e. the phonon hardens, as observed in Fig. 6.

A similar analysis also explains why the mode softens when the temperature decreases in the AFM phase. The mode corresponds to displacements with opposite signs of the Mn and F atoms along the direction (see Fig 7). We define as the magnetic coupling between the Mn atom and the Mn atoms located at , , , ; and as the coupling between the Mn atom and the Mn atoms located at , , , . Under a displacement of amplitude , the magnetic energy is modified as

(9)

Using again a rough evaluation of the perturbative expression of one finds that , and . Because the second derivative and here have the same sign, an increase of the displacement amplitude diminishes the value of . In the full harmonic potential perspective, here the correction to the effective phonon spring constant is negative, leading to the phonon softening, in agreement with Fig. 7.

Our infrared data allow us to link the magnetic ordering to changes in the dielectric constant of MnF. The optical dielectric constant is given by . In the absence of any microwave excitations, it should be equal to the static value obtained from electrical measurements. Our reflectivity data do not show any extra excitation below the phonons down to 10  (300 GHz). Figure 8 compares the static dielectric constants, measured by SeehraSeehra et al. (1986) at  kHz, with the zero frequency limit of our optical data. The left panel shows the -plane dielectric constant, and the right panel the axis response. The solid squares are the “static” values from SeehraSeehra et al. (1986) (vertically shifted by -1, for clarity) and the open circles are the optical dielectric constants. On the left panel, we also show the thermal variation of the oscillator strength for the lowest energy mode (solid triangles, right-hand scale). Note that both scales in this figure cover the same variation in values of . It is then clear that all the temperature variations in the optical dielectric constant come from the phonon. This figure also shows that, within 15%, the static dielectric constant is build from phonon and higher frequency excitations. The static and optical dielectric constants agree very well below . In the paramagnetic phase, there is a growing difference between these two values. Along the -axis both values increase with temperature but the static dielectric constant increases faster. In the -plane the difference is also qualitative. The static dielectric constant increases with temperature, whereas the optical value decreases. These discrepancies may be due to a difference in the quality of the sample, but are more likely linked to ionic conduction contributions to the dielectric constant in the radiofrequency range, a common effect on fluorides.Ure (1957); Samara and Peercy (1979) Nevertheless, in both polarizations, , measured by both techniques, shows a kink at .

Figure 8: (color online) The left panel shows the plane dielectric constant measured utilizing dielectric techniques by SeehraSeehra et al. (1986) (open squares) and zero frequency optical extrapolation (solid circles). The right panel shows the same quantities for the axis. For clarity, the dielectric measurement was shifted by -1. The blue arrows are the ab-initio predictions for changes in upon appearance of the antiferromagnetic order. The right-hand scale in the left panel shows the contribution to the dielectric constant (solid stars) and the red arrow is the ab-initio prediction for the change in . Note that right and left scales in this panel span the same range in values of , indicating that all the in-plane changes come from the mode.

We can estimate the ab-initio zero frequency dielectric constant from the calculated oscillator strengths. We made the same comparison between a “paramagnetic” and AFM configurations, as we did for the phonon frequencies. The predicted changes are shown as the vertical arrows in Fig. 8. The predicted ab-initio jump upon magnetic ordering is of the same order of magnitude as the values measured. More important, we find the correct sign for the changes in both cases. The AFM order tends to decrease the dielectric constant in the -plane while it is increased along the -axis.

The panorama in MnF points towards instabilities that favor a ferroelectric order. Ferroelectricity is not a common property of fluorides. However, several compounds (ZnF, NiF and FeF) show lattice instabilities that indicate the appearance of an incipient ferroelectric order. Our x-ray data indicate that lattice instabilities are indeed present in MnF. Infrared measurements show that the -axis phonon softens upon formation of the antiferromagnetic order. This softening goes together with an increase of the dielectric constant along this direction. These effects are indicative of a possible incipient ferroelectric behavior in MnF. In this scenario the differences between static and phononic dielectric constants observed in Fig. 8 above 100 K could also be related to zero frequency ferroelectric fluctuations. However, dielectric constant measurements at high frequencies as well as phonon dynamic measurements under pressure and/or magnetic field are necessary to confirm (or refuse) this picture. In any case, understanding the phonon changes induced by the magnetic ordering in MnF should bring new insights on the magneto-electric coupling in multiferroic materials.

V Conclusions

In this paper we presented a detailed temperature dependent infrared study of the phonon renormalization observed at in MnF. We showed that the phonon temperature dependence and the lattice parameter changes across the antiferromagnetic transition are well reproduced by ab-initio calculations, implying that the magnetic order dominates the changes observed at T. We find that phonons along the axis and the tetragonal plane have opposite changes at as predicted by the first principles results. Our results show that the dielectric constant of MnF is mostly from phonon origin. Relaxation effects on the plane contribute strongly to the dielectric constant in the paramagnetic phase. The large change in the lattice parameters with temperature and the phonon softening in the antiferromagnetic phase suggest that MnF distortions induced by the magnetic order are compatible with the ferroelectric instabilities observed in TiO and FeF and other fluorides. We suggest that the phase transition observed at 1.49 GPa (Ref. Yamaguchi et al., 1992) could be of ferroelectric order and so, MnF would qualify as an incipient multiferroic.

Acknowledgment

We thank Prof. J.-Y. Gesland for providing us with the MnF crystal used in this study. RLM acknowledges an invited “Joliot chair” at ESPCI and RPSML acknowledges an invited scientist position from FAPEMIG. This work was partially funded by the Brazilian agencies CNPq and FAPEMIG. The collaboration between ESPCI and UFMG was supported by the CNRS PICS 4905. Use of the NSLS was supported by the U.S. Dept. of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886. Structure diagrams were produced using VESTA software.Momma and Izumi (2008) The ab-initio calculations were performed at the IDRIS and CRIHAN computational centers under projects number 1842 (IDRIS) and 2007013 (CRIHAN).

Appendix

In this paper, we limited our discussion of ab-initio calculations to the four infrared active modes only. For completeness, Table 4 gives the results of calculations for all modes (infrared, Raman and silent) in both FM and pseudo-AFM configurations. These calculations are compared to the experimental values determined at 5 K for the infrared (this work) and Raman active modes (Ref. Lockwood and Cottam, 1988).

. ab-initio Experimental Symmetry Activity FM AFM This work Ref. Lockwood and Cottam,1988
Raman
- IR - Raman IR IR - Raman IR Raman

Table 4: Ab-initio point optical phonons frequencies (in ) for the FM and pseudo-AFM phases. The experimental values were taken at 5 K from the present work (IR) and from Ref. Lockwood and Cottam, 1988 (Raman)

References

  1. D. Khomskii, Physics 2, 20 (2009).
  2. G. A. Smolenskii and I. E. Chupis, Usp. Fiz. Nauk. 137, 415 (1959).
  3. S. V. Kiselev, R. P. Oserov, and G. S. Zhdanov, Sov. Phys. Dokl. 7, 742 (1963).
  4. T. Kimura, T. Goto, H. Shintani, K. Ishizaka, T. Arima, and Y. Tokura, Nature 426, 55 (2003).
  5. M. Schmidt, C. Kant, T. Rudolf, F. Mayr, A. A. Mukhin, A. M. Balbashov, J. Deisenhofer, and A. Loidl, Eur. Phys. J. B 71, 411 (2009).
  6. K. Wakamura and T. Arai, J. Appl. Phys. 63, 5824 (1988).
  7. T. Rudolf, C. Kant, F. Mayr, J. Hemberger, V. Tsurkan, and A. Loidl, New J. Phys. 9, 76 (2007).
  8. A. B. Sushkov, O. Tchernyshyov, W. Ratcliff II, S. W. Cheong, and H. D. Drew, Phys. Rev. Lett. 94, 137202 (2005).
  9. C. J. Fennie and K. M. Rabe, Phys. Rev. Lett. 95, 205505 (2006).
  10. T. Rudolf, C. Kant, F. Mayr, and A. Loidl, Phys. Rev. B 77, 024421 (2008).
  11. C. Kant, T. Rudolf, F. Schrettle, F. Mayr, J. Deisenhofer, P. Lunkenheimer, M. V. Eremin, and A. Loidl, Phys. Rev. B 78, 245103 (2008).
  12. K. Katsumate, J. Phys.: Condens. Matt. 12, R589 (2000).
  13. J. W. Stout and S. A. Reed, J. Am. Chem. Soc. 76, 5279 (1954).
  14. D. J. Lockwood and M. G. Cottam, J. Appl. Phys. 64, 5876 (1988).
  15. J. H. Weaver, C. A. Ward, G. S. Kovener, and R. Alexander, J. Phys. Chem. Solids 35, 1625 (1974).
  16. D. F. Gibbons, Phys. Rev. 115, 1194 (1959).
  17. F. Gervais and B. Piriou, Phys. Rev. B 10, 1642 (1974a).
  18. G. A. Samara and P. S. Peercy, Phys. Rev. B 7, 1131 (1973).
  19. B. Montanari and N. M. Harrison, J. Phys. Condens. Matt. 16, 273 (2004).
  20. D. J. Lockwood, R. S. Katiyar, and V. C. Y. So, Phys. Rev. B 28, 1983 (1983).
  21. J. Giordano and J. L. Sauvajol, Phys. Stat. Sol. (b) 147, 537 (1988).
  22. D. J. Lockwood, Low Temp. Phys. 28, 505 (2002).
  23. C. C. Homes, M. Reedyk, D. A. Crandles, and T. Timusk, Appl. Opt. 32, 2976 (1993).
  24. R. Dovesi, V. R. Saunders, C. Roetti, R. Orlando, C. M. Zicovich-Wilson, F. Pascale, B. Civalleri, K. Doll, N. M. Harrison, I. J. Bush, et al., CRYSTAL06 User’s manual (University of Torino, 2006).
  25. A. D. Becke, J. Chem. Phys. 98, 5648 (1993).
  26. D. I. Bilc, R. Orlando, R. Shaltaf, G. M. Rignanese, J. Íñiguez, and P. Ghosez, Phys. Rev. B 77, 165107 (2008).
  27. J. Martin and A. Sundermann, J. Chem. Phys. 114, 3408 (2001), diffuse orbitals with exponents samller than 0.15 were omitted as usual in infinite systems.
  28. M. Pseudo : Dolg, U. Wedig, H. Stoll, and H. Preuss, J. Chem. Phys. 86, 866 (1987).
  29. M. Prencipe, A. Zupan, R. Dovesi, R. Aprà , and V. R. Saunders, Phys. Rav. B 51, 3391 (1995).
  30. T. Sun, P. B. Allen, D. G. Stahnke, S. D. Jacobsen, and C. C. Homes, Phys. Rev. B 77, 134303 (2008).
  31. C. Benoit and J. Giordano, J. Phys. C: Solid State Phys. 21, 5209 (1988).
  32. F. Gervais and B. Piriou, J. Phys. C 7, 2374 (1974b).
  33. A. B. Kuzmenko, Rev. Sci. Instrum. 76 (2005).
  34. W. Baltensperger and J. S. Helman, Helv. Phys. Acta 41, 668 (1968).
  35. A. Perakis, E. Sarantopoulou, Y. S. Raptis, and C. Raptis, Phys. Rev. B 59, 775 (1999).
  36. A. Perakis, D. Lampakis, Y. C. Boulmetis, and C. Raptis, Phys. Rev. B 72, 144108 (2005).
  37. M. Yamaguchi, T. Yagi, and N. Hamaya, J. Phys. Soc. Japan 61, 3883 (1992).
  38. R. L. Melcher, Phys. Rev. B 2, 733 (1970).
  39. D. S. Rimai, Phys. Rev. B 16, 4069 (1977).
  40. J. Giordano and J. L. Sauvajol, J. Phys. C: Solid State Phys. 20, 1547 (1987).
  41. M. S. Seehra, R. E. Helmick, and G. Srinivasan, J. Phys. C: Solid State Phys. 19, 1627 (1986).
  42. R. W. Ure, J. Chem. Phys. 26, 1363 (1957).
  43. G. A. Samara and P. S. Peercy, J. Phys. Chem. Solids 40, 509 (1979).
  44. K. Momma and F. Izumi, J. Appl. Crystallogr. 41, 653 (2008).
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