Abstract
The present study investigates the influence of iron (Fe) doping on the martensitic transformation and magnetic properties of Ni50−xMn37Sn13Fex(x = 0.5, 1, 1.5) magnetic shape memory alloys in ribbon form. The ribbons were prepared using arc-melting followed by melt-spinning processes and were characterized using X-ray diffraction, scanning electron microscopy, differential scanning calorimetry, and vibrating sample magnetometry. Our findings demonstrate that the addition of Fe shifts the martensitic transformation to lower temperatures and increases the Curie point of the austenitic phase, \(T_{c}^{\text A}\), leading to an enhanced magnetism in the austenitic phase. Moreover, a significant increase in the magnetization jump \((\Delta M)\) is observed, from \( 3.3\;{\text{emu\ g}}^{-1} \) for \(x=1\) to \(17 \, {\text{emu\ g}}^{-1} \) for \(x=1.5\) under a \(50 \, \text {Oe}\) applied magnetic field. The structural transformations are also found to be sensitive to the external applied magnetic field. The isothermal magnetization curves exhibit the exchange bias effect, which confirms the coexistence of antiferromagnetic and ferromagnetic coupling in the samples. Furthermore, the exchange bias effect increases with the Fe content.
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Introduction
Non-stoichiometric NiMn-X (X=Sn, In, Ga, and Sb) ferromagnetic shape memory alloys have attracted considerable attention in recent years due to their multifunctional properties, such as Exchange Bias (EB) [1,2,3], memory shape effect [4], magnetocaloric effect [5, 6], magnetoresistance [7, 8], and elastocaloric effect [9]. These alloys undergo a first-order reversible martensitic transformation from the ferromagnetic cubic austenite phase to the weak magnetic martensitic phase with lower symmetry (tetragonal, modulated monoclinic, or orthorhombic) upon cooling. This magneto-structural transition is associated with an abrupt change in magnetization, which affects the magnetic entropy change \((\Delta S_{M})\) [5]. Due to these interesting properties, these alloys are potential candidates for magnetic refrigeration devices, sensors, and actuation devices [10, 11]. The magnetism in these alloys is mainly attributed to the Mn magnetic moment, and their magnetic properties strongly depend on the Mn-Mn inter-atomic distances, which are relatively large, resulting in indirect exchange interactions via the conduction electrons [12, 13]. The transformation temperatures and magnetic properties are highly sensitive to the chemical composition of the alloy and fourth-element doping. Transition metal doping, such as with Fe and Co, has been found to be highly effective in tuning the transformation temperatures and enhancing the magnetic properties [14,15,16]. Previous researches have indicated that replacement of Mn or Ni by Fe or Co can enhance the magnetic properties and tune the transformation temperatures of these alloys [15,16,17,18]. In Mn-rich Heusler \(Mn_{50}Ni_{41}In_{9}\) ribbon materials, substituting Mn with \(1\, at\%\) Fe caused both martensitic and magnetic transition temperatures to decrease by about \(33\, K\). Increasing Fe content to \(2\, at\%\) resulted in a slight increase in the two transitions and a large overlap. Further increasing Fe to \(3\%\) caused the magnetic transition in the austenite phase to vanish [19]. Ghosh and Mandal [20] investigated Mn-rich Mn-Ni-Fe-Sn Heusler alloys by substituting Fe for Ni and Mn. They found that replacing Ni with Fe decreased the martensitic transition temperature, but substitution of Mn with Fe increased this temperature. They also observed a large magnetic entropy change and high refrigerant capacities with a small percentage of Fe doping (\(2\, at\%\) ). In recent studies, substitution of Ni with \(1.1\, at\% \) of Fe in \(Ni_{50}Mn_{38}Sn_{12}\) alloy resulted in a magnetization jump \(\Delta M\) of \(36.7 \,A \, m^{2}\ kg^{-1}\), almost twice as large as that in the undoped alloy \((19.7 \, A \, m^{2}\ kg^{-1})\) [21]. In \(Ni_{42}Mn_{49}Sn_{9}\) alloy, replacing Ni with Fe enhanced the magnetization, reaching a maximum value of \(49 \, A \, m^{2}\ kg^{-1}\) for \(4\, at\%\) Fe, and decreasing the martensitic transformation temperature [15]. The addition of Co or Fe as the fourth element in Ni-Mn-Sn based alloys can lead to the precipitation of the \(\gamma \) phase [15, 22,23,24], which causes chemical composition segregation and adversely affects the magneto-structural properties [25]. However, the fast kinetics of crystallization associated with melt spinning can suppress the formation of the \(\gamma \) phase [26]. Moreover, melt spinning facilitates the fabrication of textured samples with enhanced mechanical properties. The specific geometry of the resulting ribbons offers distinct advantages for the development of magnetocaloric materials, as it facilitates efficient heat exchange with the heat transfer fluid within a magnetocaloric device, enabling rapid thermal transfer [27, 28]. From a technological standpoint, the use of melt spinning is attractive because it obviates the need for expensive heat treatment stages. Fe or Co has been added as a fourth element in several studies involving Ni-Mn-Sn-based ribbons [18, 29,30,31,32]. In the present work, we perform a systematic investigation of the effect of Fe doping and applied magnetic field on the martensitic transformation and magnetic properties of \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5,\, 1,\, 1.5)\) melt-spun ribbons.
Experimental
Non-stoichiometric \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5,\, 1,\, 1.5)\) Heusler alloys were synthesized by arc melting high purity elements (\(> 99.9 \,at\%\)) under an argon atmosphere. To ensure homogeneity, the constituent elements were melted four times. The obtained ingots were then induction-melted in a quartz tube in a melt-spinning system, and ejected into an argon environment onto the polished surface of a copper wheel rotating at a linear speed of \( 48\, m\ s^{-1}\). The microstructural morphology and chemical composition of the resulting melt-spun ribbons were examined using a scanning electron microscope (SEM) equipped with an X-ray energy dispersive spectroscopy (EDS) microanalysis system. The melt-spinning technique offers advantages for ribbon production, including compositional homogeneity and a polycrystalline texture with a small grain size, which can facilitate martensitic phase nucleation [33]. The structure and properties of the ribbons depend on several factors, including the velocity of the rotating wheel and ejection conditions [34]. To ensure consistency, all samples in this work were produced using the same melt-spinning conditions. The crystallographic structure of the ribbons at room temperature was determined using X-ray diffraction (XRD) with \(Cu K \alpha \) radiation (\(\lambda = 0.154060 \, nm\)), a step size of \(2\theta = 0.02^{\circ }\), and a counting time of \(15\,s\). The XRD patterns were analyzed using the MAUD program [35] based on the Rietveld method [36]. The austenite-martensite structural transformations were studied using differential scanning calorimetry (DSC). Cyclic experiments were performed under a liquid nitrogen atmosphere with a cooling and heating rate of \(10\, K\ min^{-1}\) to determine the thermal characteristics of the ribbons. Thermomagnetic measurements were conducted using a vibrating sample magnetometer (VSM-VersaLab, QD) with zero-field-cooling (ZFC), field-cooling (FC), and field-heating (FH) protocols over a temperature range of \(50\, K\) to \(400 \, K\) and an applied magnetic field up to \(50 \, kOe\).
Results and discussions
Microstructure
Figure 1 shows typical SEM micrographs of the free surface [(a), (b) and (c)] and the fracture cross section [(d), (e) and (f)] of \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5,\, 1,\, 1.5)\) Heusler alloys ribbons. The free surface of the ribbons exhibits a granular microstructure, characterized by nearly equiaxed grains. Additionally, a distinct twin-variants relief of the martensitic substructure is clearly observed for \(x=0.5\) alloys in fig 1 (a) (will be confirmed as the modulated 10M structure by XRD measurements). On the other hand, the fracture cross section of all ribbons demonstrates a consistent columnar structure oriented perpendicular to the ribbon plane, indicating that heat dissipation during the rapid solidification process induces directional growth of the crystalline phase [37, 38]. The grain sizes and the ribbon thickness were around 2 and \(11\, \mu m\) respectively. The chemical composition of the obtained samples was verified using EDS microanalysis, with the results presented in Table 1. As shown, the chemical composition of all the ribbons closely matches the nominal values.
XRD
The XRD patterns at room temperature of the obtained ribbons are presented in fig 2. The XRD patterns of the \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} ( 1,\, 1.5)\) samples show the presence of peaks corresponding to the austenite phase. However, for the \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5)\) composition, in addition to the characteristic peaks of the austenite phase, there are additional peaks that may correspond to the martensitic phase (observed in fig 1 (a)). The XRD patterns were refined using the MAUD program based on the Rietveld analysis. For \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 1,\, 1.5)\) ribbons, the Rietveld refinement was obtained by generating theoretical patterns of the cubic \(L2_{1}\) structure that correspond to the austenite phase. However, for the \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5)\) ribbon, the Rietveld refinement was obtained with the cubic \(L2_{1}\) structure and the modulated 10M structure, with phase percentages of \(80\%\) and \(20\%\), respectively. This indicates the coexistence of the austenite and martensite phases at room temperature in the \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5)\) ribbon (observed in Fig. 1a). The 10M modulated martensite is one of the three possible crystallographic structures of the martensite phase, consisting of five cells of the monoclinic \(L1_{0}\) put together with some distortion between the different layers. This martensite structure was also observed in \(Ni_{50}Mn_{38}Sb_{12}\) [39], \(Ni_{50}Mn_{36}Fe_{1}In_{13}\) and \(Ni_{50}Mn_{35}Fe_{2}In_{13}\) [40]. The Rietveld refinement results presented in Table 2 show a small decrease in the lattice parameter, a, of the austenite phase with the increase of Fe concentration. This slight decrease could be attributed to the smaller atomic radius of Fe than that of Ni. A similar lattice shrinkage was reported in Fe-doped Ni-Mn-In melt-spun ribbons [41]. Based on the XRD results, it appears that the increase of Fe doping stabilizes the austenite phase at room temperature. The average crystallite size, representing the coherent diffraction domain, also shows notable differences. For the \(x = 0.5\) composition, the \(L2_{1}\) phase exhibits a crystallitte size of \(113\pm 2 \, nm\), while the 10M phase shows a significantly smaller size of \(55\pm 2 \, nm\). For the \(x = 1\) and \(x = 1.5\) compositions, which consist only of the austenite \(L2_{1}\) phase, the crystalline sizes are \(142\pm 3 \, nm\) and \(139 \pm 2 \, nm\), respectively. These values indicate that the crystallite size increases with Fe doping from \(x = 0.5\) to \(x = 1\), but slightly decreases for \(x = 1.5\). The larger crystallite sizes observed for the \(x = 1\) and \(x = 1.5\) compositions suggest that Fe doping promotes the growth of larger crystallites in these alloys. In contrast, the presence of two phases (\(L2_1\) and 10M) in the \(x = 0.5\) composition results in significantly different crystallite sizes for each phase, with the 10M phase showing much smaller crystallites. This disparity in crystalline size can be attributed to the distinct growth mechanisms and stability of the different phases. The nanometric scale of the crystallites observed in these alloys can be attributed to the rapid solidification process inherent in the melt-spinning method used for samples preparation.
DSC
DSC curves, shown in Fig. 3, indicate a first-order reversible martensitic transformation (MT) in all samples. The curves display exothermic and endothermic peaks related to the forward and reverse martensitic transformation, respectively. The start \((M_{S}, A_{S})\) and finish \((M_{F}, A_{F})\) MT characteristic temperatures were determined as the intersection of the tangents of each peak with the baseline. The results are presented in Table 3. \(M_{S}\) was found to decrease with increasing Fe content for all ribbons, \(M_{s}\) values were \(329\, K, 255\, K\), and \(205\, K\) for \(x=0.5, 1, 1.5\), respectively. The other characteristic transformation temperatures, \(M_{f}\), \(A_{s}\), \(A_{f}\), and the martensitic transformation temperature \(T_{M}\), defined as \((M_{S} + A_{F})/2\), also shifted toward lower temperatures as the Fe content increased. The decrease in transformation temperatures was most significant in the \(Ni_{47}Mn_{37}Sn_{13}Fe_{1.5}\, (x=1.5)\) alloy, indicating that Fe strengthens the stability of the cubic austenite parent phase. This behavior has been observed in other Ni-Mn-Sn ferromagnetic alloys and was attributed to the electron valence concentration (e/a), which has a linear correlation with \(M_{s}\) [42]. The addition of Fe atoms reduces the (e/a) due to the lower number of electrons in the outer shell of Fe compared to Ni. This correlation was confirmed by EDS microanalysis, which showed that the (e/a) decreased as the Fe content increased (see Table 3). However, other factors such as the Ni/Mn ratio and grain size of the austenitic phase also affect the martensitic transformation and should be taken into account [40, 43]. The thermal hysteresis \(\Delta T\), defined as the difference between the temperatures corresponding to exothermic and endothermic peaks, varies between \(11\, K\) and \(20\; K\), as shown in Table 3. These values are higher than those recently reported for \(Ni_{50-x}Fe_{x}Mn_{40}Sn_{10} (x = 0, 2, 4, 6, 8)\), and \(Ni_{50}Mn_{36-x}Fe_{x}Sn_{14} (x = 0, 2, 3)\) ribbons [29, 31]. The exothermic and endothermic peaks observed in the DSC profiles are utilized to determine the transformation enthalpies \((\Delta H)\), by calculating the area between the peaks and the baseline. \((\Delta H)\) and the entropy changes \((\Delta S)\) associated with the structural transformations are included in Table 3. No trend was observed as a function of the Fe content (or the (e/a) parameter), a similar effect has been reported in Ni-Mn-Sn-Co melt-spun alloys [44]. It is worth noting that while the XRD analysis for the \(x = 0.5\) alloy suggests the coexistence of austenite and martensite phases at room temperature (\(80\%\) austenite and \(20\%\) martensite), the DSC measurements indicate a complete transformation at this temperature. This apparent mismatch could be attributed to several factors. The rapid solidification process during melt spinning can lead to the formation of a metastable state, where the coexistence of phases at room temperature is possible. Additionally, DSC measurements may be more sensitive to the transformation process and could detect the complete transformation even if the XRD results suggest the presence of a mixture of phases. Further investigation using transmission electron microscopy (TEM) could help to clarify this discrepancy and provide a more detailed understanding of the phase distribution in the \(x = 0.5\) alloy.
Magnetic measurements
M(T) at low applied magnetic field (\(H = 50 \, Oe\))
Figure 4 illustrates the temperature-dependent behavior of the ZFC, FC, and FH magnetization M(T) curves for \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5,\, 1,\, 1.5)\) ribbons, measured in the presence of a low magnetic field \((H=50 \, Oe)\). The ZFC data for all samples start at low magnetization value that decreases as the Fe concentration increases. For the \(x=0.5\) sample, upon heating, the ZFC curve rapidly increases up to about \(170 \, K\), after which the magnetization decreases with further heating. Meanwhile, the FH and FC curves decrease with increasing temperature. At approximately \(260 \, K\), the three curves converge, and the magnetization rapidly decreases to zero at around \(300 \, K\).
The Curie temperature of the martensitic phase as determined to be \(T_{C}^{M}=278 \, K\), and no ferromagnetic ordering was observed in the austenitic state of this sample. The structural transformation takes place from a paramagnetic austenitic state to a paramagnetic martensitic state around \(M_{s}=329 \, K\) obtained from calorimetric measurements. For the \(x=1\) sample, M(T) increases very slowly up to about \(210 \, K\), after which the magnetization begins to increase rapidly until the ZFC and FH curves merge at about \(235 \, K\). Upon further increasing the temperature, M(T) first decreases, and an inflection point appears, which corresponds to the Curie temperature \(T_{C}^{M}\) of the magnetic transition of the martensitic phase \(T_{C}^{M}=242 \, K)\). A sharp increase in magnetization accompanied by splitting between the FH and FC curves around \(250 \, K\) up to about \(270 \, K\) is observed, corresponding to the reverse martensitic transformation from a weak-magnetic martensitic state to a ferromagnetic austenitic state. Further increasing the temperature leads to a decrease in magnetization, and the Curie temperature \(T_{C}^{A}\) of the austenitic phase for a ferromagnetic to paramagnetic transition is estimated to be \(T_{C}^{A}=286 \, K\). For the \(x=1.5\) sample, the ZFC, FC, and FH curves start at low magnetization values and increase very slowly upon heating up to the reverse martensitic transformation, which occurs between \(195 \, K\) and \(225 \, K\). The Curie temperature of the austenitic phase for this sample is \(T_{C}^{A}=312 \, K\). The bifurcation between the ZFC and FC curves just below \(T_{C}^{A}\) for this sample could indicate the existence of magnetically inhomogeneous states [5, 8, 45]. The M(T) curves for the \(x=1\) and 1.5 samples in Fig. 5 show the existence of a Hopkinson maximum [46] just below the Curie temperature of the austenitic phase, which can be attributed to a decrease in the magnetic anisotropy due to an increase in the magnetic susceptibility below \(T_{C}^{A}\). This maximum vanishes with higher magnetic fields (see Fig. 5). The Curie points of the martensitic \(T_{C}^{M}\) and austenitic \(T_{C}^{A}\) phases were determined by the minimum of the dM/dT vs. T of FC curves, with \(T_{C}^{A}\) increasing with increasing Fe concentration. The values of the start (\(M_{S}^{M}\), \(A_{S}^{M}\)) and finish (\(M_{F}^{M}\), \(A_{F}^{M}\)) MT temperatures, determined by the two-tangent method, the austenitic Curie temperature \(T_{C}^{A}\), the martensitic Curie temperature \(T_{C}^{M}\), and the magnetization change \(\Delta M\) between the martensitic and austenitic states of the three alloys deduced from M(T) at low applied magnetic field \((50 \, Oe)\) curves are listed in Table 4. The addition of Fe shifts MT to lower temperatures (in good agreement with DSC scans) and \(T_{C}^{A}\) to higher temperatures, as evidenced by the results presented in Table 3. This change leads to an enhancement of the magnetic properties of the austenitic phase, resulting in a large jump in magnetization \(\Delta M\), which ranges from \(3.3 \, emu\,g^{-1}\) for \(x=1\) to \(17 \, emu\,g^{-1}\) for \(x=1.5\), under a low magnetic field of \(50 \, Oe\). This significant increase in \(\Delta M\) may improve the magnetocaloric effect of these alloys, and is consistent with previous studies on Ni-Mn-Sn- based Heusler alloys [16, 22, 47,48,49].
M(T) at high applied magnetic field (\(H = 50 \, k\, Oe\))
Figure 5 represents thermomagnetization curves for \(x=0.5\), 1 and 1.5 compounds at high applied magnetic field \((H=50 \, k \, Oe\)). No splitting between ZFC and FC curves is found, and the Hopkinson maximum vanishes for all samples. However, except \(x=0.5\) (no MT is observed), a considerable drop in the magnetization of MT (\(\Delta M\)) is seen during cooling, which is related to the weak magnetic martensitic phase. Increasing the applied magnetic field shifts MT to lower temperatures and \(T_{C}^{A}\) to higher temperatures (see Table 5). A large value of the magnetization jump \(\Delta M\) is observed (from \(3.3 \, emu\ g^{-1} \) under \(50 \, Oe\) to \(14.6 \, emu\ g^{-1}\) under \(50 \, k\, Oe\) for \(x=1\) and from \(17 \, emu\ g^{-1}\) under \(50 \, Oe\) to \(35 \, emu\ g^{-1}\) under \(50 \,k\, Oe\) for \(x=1.5\)).
Likewise, the magnetization of both austenitic and martensitic phases is strongly related to the applied magnetic field. Figure 6 shows magnetization as a function of the magnetic field at \(300 \, K\) (austenitic phase), \(160 \, K\) (just below MT) and \(200 \, K\) (martensitic phase) for \(x=1.5\). The curve at \(300 \, K\) represents the behavior of the austenite phase, which is ferromagnetic. The magnetization increases with the applied field and shows a tendency toward saturation. The curve at \(160 \, K\) represents the behavior of the martensite phase, which is weakly magnetic, and the magnetization remains low even at high magnetic fields. The curve at \(200 \, K\), just below the martensitic transformation temperature, exhibits a field-induced metamagnetic phase transition. At low fields, the material is in the martensite phase with low magnetization. However, as the field increases, a sudden jump in magnetization occurs at a critical field of approximately \(6 \, kOe\). This jump corresponds to the field-induced transformation from martensite to austenite. When the field is reduced, the transformation reverses, and the magnetization drops back to the low value, exhibiting hysteresis. This metamagnetic behavior can be attributed to the high \(\Delta M\) of this compound, resulting in significant Zeeman energy (\(\mu _{0}\, \Delta M \, H\)) [15]. The Zeeman energy, which depends on the magnetization and the field strength, acts as a driving force for the transformation. The measurements were performed by incrementally increasing and then decreasing the magnetic field to capture the hysteresis effect. The apparent discontinuity observed in the curves is intrinsic to the metamagnetic phase transition and is consistent with the behavior reported in similar materials [4, 15, 50]. This figure clearly demonstrates the characteristic features of the metamagnetic effect: a sharp magnetization jump at a critical field and hysteresis during the field cycling.
Exchange bias effect
Figure 4 clearly showed a bifurcation between the ZFC and FC curves for all samples, which corresponds to a magnetic transition in the ZFC curves around \(250 \, K\) for \(x=0.5\) and 1, and \(300 \, K\) for \(x=1.5\). We refer to this transition temperature as the conventional exchange bias blocking temperature, \(T_{B}\). This bifurcation becomes much more pronounced with decreasing temperature, indicating the coexistence of AFM and FM exchange interaction in the martensitic state [2, 51,52,53]. To further investigate the exchange bias effect, magnetic hysteresis loops were measured after FC (\(H=5\, T\)) at various temperatures for all three alloys (Fig. 7). Figure 7(a-c) shows the loops at \(10 \, K\), \(200 \, K\), \(260\, K\), and \(300\, K\) for \(x = 0.5\), \(x = 1\), and \(x = 1.5\), respectively. These loops reveal a clear shift from the origin, particularly at lower temperatures, indicating the presence of exchange bias. The shift, which is attributed to the exchange coupling between ferromagnetic and antiferromagnetic regions, is most pronounced at \(10 \, K\) and gradually decreases with increasing temperature, consistent with the thermal fluctuations reducing the strength of the exchange coupling. Figure 7(d) compares the hysteresis loops at \(10 \, K\) for all three alloys, highlighting the increasing exchange bias field with increasing Fe content. This observation further supports the coexistence of antiferromagnetic and ferromagnetic coupling in our samples and confirms that Fe doping enhances the exchange bias effect. Figure 8 presents a double-shifted loop at \(10 \, K\) after ZFC of \(x=1.5\) ribbon (no such behavior is observed for \(x=0.5\) and 1 ribbons), this double-shifted loop, usually observed in certain EB materials with AFM and FM layers [54,55,56,57,58,59], is another evidence of the existence of AFM and FM coupling in this sample at low temperatures. A similar behavior was reported in bulk Mn-rich Ni-Mn-Sn Heusler alloys [51]. This explains the lower values of the magnetization observed in the M(T) curves of \(x=1.5\) sample at low temperatures. The ZFC and FC hysteresis loops show a different behavior due to the difference between the magnetic domain structure formed when the system is cooled in the presence of a magnetic field or zero field cooled [51]. Figure 9 shows the variation of the \(H_{EB}\) and \(H_{C}\) as function of temperature from \(10 \, K\) to \(300 \, K\) for \(x=0.5\), 1 and 1.5 ribbons. Here \(H_{EB}\) and \(H_{C}\) are calculated using \(H_{EB}=-(H_{+}+H_{-} )/2\) and \(H_{C}=|(H_{+}-H_{-} )|/2\) (\(H_{+}\) and \(H_{-}\) are the right and left coercive fields, respectively). \(H_{EB}\) is found to decrease with increasing temperature for all samples, due to the reduction of the exchange coupling between the AFM-FM regions by the thermal fluctuation, and it vanishes at temperatures close to \(260\, K\) for \(x=0.5\) and 1, and \(300\, K\) for \(x=1.5\). These temperatures corresponding to the exchange bias blocking temperatures are in good agreement with those extracted from thermomagnetization curves. In contrary with several previous reports where a strong peak is observed in \(H_{C}\) near \(T_{B}\) [51,52,53], in our samples, \(H_{C}\) also shows a monotonic decrease with increasing T. This behavior is consistent with a martensitic phase where nanoscopic FM clusters, near the thermal stability, are embedded in a long-range order AFM matrix [60, 61].
Conclusions
In the present work, we have investigated the effect of Fe doping on the martensitic transformation and the magnetic properties of \(Ni_{50-x}Mn_{37}Sn_{13}Fe_{x} (x= 0.5,\, 1,\, 1.5)\) magnetic shape memory alloys in the form of ribbons, and the main conclusions can be drawn as follows:
-
1.
At room temperature, x=1 and 1.5 ribbons are \(L2_{1}\)-type cubic austenite. However, the \(x= 0.5\) ribbon is a mixture of cubic \(L2_{1}\) and the modulated 10M structure indicating the coexistance of austenite and martensite phases.
-
2.
The addition of Fe shifts the martensitic transformation to lower temperatures and the Curie point of the austenitic phase \(T_{C}^{A}\) to higher temperatures which leads to the enhancement of the magnetism of the austenitic phase.
-
3.
A large value of the magnetization jump, \(\Delta M\), is detected (from \(3.3 \, emu\ g^{-1}\) for \(x=1\) to \(17 \, emu\ g^{-1}\) for \(x=1.5\) under \(50 \, Oe\) applied magnetic field).
-
4.
Exchange-bias effect was found in all ribbons, which confirms the coexistence of antiferromagnetic and ferromagnetic coupling in our samples. The exchange bias effect is found to increase with the increase in Fe content.
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Younsi, W., Louidi, S., Suñol , J.J. et al. Martensitic transformations and magnetic properties of Ni50−xMn37Sn13Fex(x = 0.5, 1, 1.5) melt-spun ribbons. J Therm Anal Calorim (2024). https://doi.org/10.1007/s10973-024-13568-9
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DOI: https://doi.org/10.1007/s10973-024-13568-9