Raja Dasab and
Pankaj Poddar*abc
aPhysical and Materials Chemistry Division, CSIR-National Chemical Laboratory, Dr Homi Bhabha Road, Pune 411 008, India. E-mail: p.poddar@ncl.res.in
bAcademy of Scientific and Innovative Research (AcSIR), Anusandhan Bhawan, 2 Rafi Marg, New Delhi-110 001, India
cCentre of Excellence on Surface Science, CSIR-National Chemical Laboratory, Dr Homi Bhabha Road, Pune 411 008, India
First published on 20th December 2013
Detailed ac and dc magnetic properties of orthorhombic EuMnO3 were studied using a nanocrystalline powder sample. Orthorhombic EuMnO3 nanoparticles of 45 nm average size were synthesised using a hydrothermal method. Zero field cooled (ZFC) and field cooled (FC) magnetisation shows anomalies at ∼53, 44 and 24 K attributed to paramagnetic (PM) to an incommensurate antiferromagnetic phase (ICAFM), ICAFM to a canted A-type antiferromagnetic order (cAAFM) and spin reorientation transitions, respectively. No indication of a PM to ICAFM transition was observed in either the real or imaginary part of ac magnetisation. The real part of the ac magnetisation curve showed a peak at ∼24.7 K and anomalies at ∼46.8 and 21.8 K were observed in the imaginary part of ac magnetisation. Reduction in the width of the thermal hysteresis between the field cooling and heating magnetisation curve was observed with the nanocrystallites (∼1 K) compared with the bulk phase (∼3 K) EuMnO3. Isothermal magnetisation showed a large value of the exchange bias (2799 Oe at 3 K) below the ICAFM to cAAFM transition temperature.
EuMnO3 crystallises in an orthorhombic perovskite structure with Pbnm symmetry.9 At room temperature, it is paraelectric and PM. It undergoes a phase transition from PM to ICAFM at ∼50 K.5 It undergoes a further transition from ICAFM to cAAFM ordering at ∼44 K.10 Due to this cAAFM ordering, it shows ferromagnetic-like ordering below this temperature. At ∼24 K, it shows a spin reorientation transition.10 It shows a thermal hysteresis in a field cooled heating and cooling magnetisation curve.10 Detailed study of the thermal hysteresis has not been done so far. Studies of the thermal hysteresis and the transitions are needed in order to understand the origin of the ferromagnetism. Low temperature isothermal magnetisation has also not been studied so far in EuMnO3, which could further give insight into these transitions.
Nanoparticles exhibit significant differences in their physical and chemical properties from their bulk counterparts due to their large surface to volume ratio.11,12 Therefore, it is interesting to explore the corresponding effects like multiferroic properties in the nanoparticle form in order to integrate them into nano-electronics and other applications with potential benefits. Despite the great interest to study them in the nano-regime, there are no reports on the synthesis and magnetic properties of EuMnO3 nanoparticles. In this paper, we are reporting for the first time the synthesis and magnetic properties of EuMnO3 nanoparticles. Moreover, we are showing a detailed study on the thermal hysteresis and transitions. Isothermal magnetisation shows a large value of the exchange bias below the ICAFM to cAAFM transition temperature. The possible reason for the exchange bias is also studied.
Fig. 2 (A) Transmission electron micrograph and (B) HRTEM image of orthorhombic EuMnO3 nanocrystals. |
Fig. 3 shows the temperature dependence of magnetisation in ZFC and FC modes at 500 Oe and 10000 Oe applied magnetic field. At 500 Oe applied field, the ZFC and FC magnetisation curves show bifurcation at 53 K. The ZFC magnetisation curve shows two more anomalies as humps at 44.8 and 24.7 K. At 10000 Oe applied field, the ZFC and FC magnetisation curves show bifurcation at 43 K. The ZFC curve shows a broad hump at 13 K. Above 100 K, Curie–Weiss fitting of the FC curve gave a Weiss temperature of −40 K and Curie constant, C = 4.5 K emu mol−1. The Weiss temperature is greater than the reported value of −88 K for a bulk ceramic sample.10 Below bifurcation of the ZFC and FC magnetisation curves, the FC magnetisation curve shows a steep increase in magnetisation value. As the temperature increases from 3 K, FC magnetisation (500 Oe) shows a decreasing trend and ZFC magnetisation increases very slowly, showing a maximum at 24.7 K. Further heating causes a decrease in magnetisation and again produces a maximum at 44.8 K. The increase in magnetisation below ∼53 K in FC mode is an indication of ferromagnetic interaction. The bifurcation of the ZFC and FC magnetisation curves at 53 K is due to the PM to ICAFM transition. This is in good agreement with reported values for bulk samples.5 The maximum at ∼44.8 K in the ZFC magnetisation curve can be attributed to the ICAFM to cAAFM transition. The maximum at 24.7 K in the ZFC curve can be assigned to a spin reorientation transition.10 It can be noted that, for bulk ceramic samples, ZFC magnetisation shows a decreasing trend as the temperature increases from 3 K, but in our nanocrystallite particles, the ZFC magnetisation curve showed an increasing trend. This can be explained by the large value of the Weiss temperature, −40 K, which indicates reduced strength of the frustrated antiferromagnetism. At low temperature, cAAFM dominates and gives ferromagnetic-like behaviour. As the applied field is increased, these transitions are not seen in the ZFC magnetisation curve, which shows their weak interaction strength, so a higher field can cause them to vanish completely. At 10000 Oe applied field, the ZFC and FC magnetisation curves show bifurcation at 43 K and ZFC shows a maximum at 13 K. The field dependence of these transitions were probed further and discussed below. The field cooling and heating curves (Fig. 4) at 500 Oe applied field show a thermal hysteresis between 19 and 56 K. The presence of the thermal hysteresis can be explained by competitive interaction between different spin orders. From 19–56 K, three phases of PM, ICAFM and cAAFM compete with each other during the heating and cooling cycle. So in the heating and cooling cycle, competitive interaction between the different types of spin ordering results in a thermal hysteresis. It is noteworthy that the width of the thermal hysteresis observed in the nanocrystallites (∼1 K) is lower than reported data for bulk samples (∼3 K).10 As the surface to volume ratio is higher in nanocrystallites, so surface disorder spins dominate over the bulk spin phenomenon. This is also evident from the steep increase of the FC magnetisation curve. To probe the field dependence of the transitions, we compared the ZFC magnetisation curves in Fig. 5. The spin reorientation transition at 24.7 K does not show field dependency up to 1000 Oe applied field, whereas the ICAFM to cAAFM transition varies from 48 K at 100 Oe to 45 K at 1000 Oe applied field. At 10000 Oe applied field, the ZFC magnetisation curve shows a broad hump starting from 34 K with a pronounced peak ∼12 K.
Fig. 3 ZFC and FC magnetisation curves at 500 Oe and 10000 Oe applied fields for orthorhombic EuMnO3 nanoparticles. |
Fig. 4 FC heating and cooling magnetisation curves at 500 Oe applied field for orthorhombic EuMnO3 nanoparticles. |
Fig. 5 ZFC magnetisation curves at various applied fields for orthorhombic EuMnO3 nanoparticles showing the field dependency of transitions. |
To probe further the nature of these transitions, ac magnetisation was performed in a wide temperature range at 5 Oe ac field at various frequencies. The real part of the ac magnetisation (Fig. 6A) curve showed a peak at ∼24.7 K, which is a spin reorientation transition observed in dc magnetisation. Except for this transition, none of the other transitions which were seen in the dc magnetisation data were observed in the real part of the ac magnetisation curve. The absence of a Néel transition (∼53 K) in the real part of the ac magnetisation was reported for many compounds of the same class in both the bulk and nano-regime.17,18 No frequency dependency was observed for the spin reorientation transition. The imaginary part of the ac magnetisation (Fig. 6B) shows anomalies at ∼46.8 and 21.8 K. These can be associated to ICAFM to cAAFM and spin reorientation transitions, respectively, which are in good agreement with dc magnetisation data.
To probe further the nature of the transitions, isothermal field dependent magnetisation was performed around the transition regions. The M–H curves (Fig. 7) show non linearity below the Néel temperature and no saturation was observed in the whole temperature range as expected for AFM compounds. At 25 K, the coercivity value is 1025 Oe, which increases to 2991 Oe at 3 K. The increase in coercivity value at low temperature can be due to cAAFM or surface ferromagnetic-like uncompensated spins, which become more pronounced at low temperature. A large exchange bias (Fig. 7 inset) was observed below the ICAFM to cAAFM (∼43 K) transition. At 3 K, the value of the exchange bias was ∼2799 Oe and it decreased with an increase in temperature, becoming zero at 43 K. The presence of exchange bias in nanocrystallite particles is well explained in the literature, being due to the presence of a ferromagnetic-like surface layer. In the literature for bulk EuMnO3, exchange bias is not reported. It is proposed in several previous studies that in smaller dimensions, the AFM systems may show uncompensated spins at the surface leading to net ferromagnetic-like behavior at low temperature. Moreover, due to the presence of indirect exchange interaction, the coupling is very weak and the shell-spins may not have a well-defined transition temperature. They are still part of the core lattice but due to the reduced coordination number of surface atoms, the surface spins remain disordered/canted leading to a ferromagnetic-like surface layer.19–21 An exchange bias effect was also observed in antiferromagnetic nanoparticles, BiFe0.8Mn0.2O3, La0.2Ca0.8MnO3 due to uncompensated surface spins.19,20 EuMnO3 nanoparticles were cooled from 300 K to 3 K at the desired applied field, then an isothermal measurement was recorded. The applied field while cooling will align the surface uncompensated spins, which should increase the surface ferromagnetic-like character, thereby increasing the exchange bias. The M–H loops at 3 K under various field cooled conditions are shown in Fig. 8. It was found that at 30000 Oe and 50000 Oe field cooled conditions, there was an enhanced exchange bias (∼3400 Oe) at 3 K isothermal magnetisation. At 1000 Oe field cooled, which is less than coercivity at 3 K, the exchange bias decreased to 2260 Oe compared with 2799 Oe in the zero field cooled M–H. This could be due to the fact that, at fields less than the coercive field, the AFM spin could not align in the opposite direction thereby decreasing the exchange bias. Based on the above field cooled M–H loops at 3 K, we can model a nanoparticle as a core–shell structure having an inner antiferromagnetic core and ferromagnetic-like surface layer (Fig. 8 inset). The origin of the exchange bias below ICAFM to cAAFM (∼43 K) is due to the onset of antiferromagnetic nature in the core of the nanoparticles, which is weakly coupled with an uncompensated ferromagnetic-like surface layer. The temperature dependency of the exchange bias is due to an increase in the cAAFM ordering with decreasing temperature.
Fig. 7 M–H loops for orthorhombic EuMnO3 nanoparticles at various temperatures. Inset shows temperature dependence of the exchange bias. |
Fig. 8 M–H loops of orthorhombic EuMnO3 nanoparticles at 3 K with different field cooled conditions. Inset shows schematic model of an individual orthorhombic EuMnO3 nanoparticle. |
In conclusion, we have synthesised single phase orthorhombic EuMnO3 nanoparticles with 45 nm average particle size. The ZFC and FC magnetisation curves showed three anomalies at ∼53, 44.8 and 24.7 K, which were attributed to PM to ICAFM, ICAFM to cAAFM and spin reorientation transitions, respectively. Due to competitive interactions between different spin orderings, a thermal hysteresis (∼1 K) in between 19 and 56 K was observed in field cooled heating and cooling magnetisation. Based on the field cooled M–H loop measurement, the nanoparticle was modelled as a core–shell structure. The origin of the exchange bias below the ICAFM to cAAFM (∼43 K) transition is due to the weak coupling between the antiferromagnetic-core and the ferromagnetic-like surface layer of the nanoparticles.
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