Effect of Sb-doping on martensitic transformation and magnetocaloric effect in Mn-rich Mn 50 Ni 40 Sn 10 x Sb x ( x = 1 , 2 , 3 , and  4 ) alloys
Shah Ishfaq Ahmad, Hassan Najam ul, Liu Jun, Gong Yuanyuan, Xu Guizhou, Xu Feng
Jiangsu Key Laboratory of Advanced Micro & Nano Materials and Technology, School of Materials Science and Engineering, Nanjing University of Science and Technology, Nanjing 210094, China

 

† Corresponding author. E-mail: xufeng@njust.edu.cn

Abstract

We investigate the influence of Sb-doping on the martensitic transformation and magnetocaloric effect in Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys. All the prepared samples exhibit a B2-type structure with the space group at room temperature. The substitution of Sb increases the valence electron concentration and decreases the unit cell volume. As a result, the magnetostructural transformation shifts rapidly towards higher temperatures as x increases. The changes in magnetic entropy under different magnetic field variations are explored around this transformation. The isothermal magnetization curves exhibit typical metamagnetic behavior, indicating that the magnetostructural transformation can be induced by a magnetic field. The tunable martensitic transformation and magnetic entropy changes suggest that Mn50Ni40Sn Sb x alloys are attractive candidates for applications in solid-state refrigeration.

PACS: 75.30.Sg
1. Introduction

In recent decades, magnetic cooling refrigerators based on the magnetocaloric effect (MCE) have received considerable attention. Compared with the traditional gas compression for refrigeration, magnetic cooling offers advantages in terms of low cost, safety, size, low mechanical vibration, high cooling efficiency, and environmental friendliness.[14] The application of magnetic refrigeration is strongly dependent on the MCE of materials. The large MCE observed in coupled materials has led to the widespread investigation of compounds that exhibit a magnetic first-order transition, e.g., LaFe Si x ,[5] MnFeP As ,[6] Gd5Si Ge x ,[7] and especially Ni-Mn-based ferromagnetic shape memory alloys.[8,9]

Recent experimental and theoretical work demonstrates that the MCE in Ni-Mn-based magnetic shape memory alloys is related to the thermal and magnetic-field-induced magnetostructural transformation (MT), which can be tuned by changing the valence electron concentration ( . The MT and coupled MCE have been widely investigated in Ni-rich Ni-Mn-based Heusler alloys, such as Ni50Mn37Sn13,[10] Ni43Co7Mn39Sn11,[11] Ni50Mn Sb B x ,[12] Ni44Co Mn In ,[13] Ni Cu x Mn31Ga19,[14] and Ni Co x Mn Al .[15] The MT and MCE are also observed in high-Mn-content Mn2NiX ( , Sn, and Ga) inverse Heusler alloys.[1618] It is known that Mn50Ni40In10 alloy undergoes an MT from ferromagnetic austenite to weak magnetic martensite during cooling, and Co-doping leads to an increase in the magnetization difference ( between the two phases.[17,18]

A similar transition is observed in Mn50Ni40Sn10 alloy. The MT in Mn50Ni40Sn10 alloy is very sensitive to the p-d hybridization, which can be influenced by atomic substitution, resulting in a tunable MCE.[19,20] Attempts have been made to tune the MT through the partial substitution of Ni by Cu or Co in Mn50Ni40Sn10 alloys.[21,22] However, the influence of sp-elements like antimony (Sb) on the MT and magnetic properties of Mn-rich Mn2NiSn inverse Heusler alloys has not yet been reported. In the current work, Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys are prepared by arc-melting. The effects of Sb-substitution on the structure, magnetic phase transition, and MCE around the MT are investigated and discussed in detail. Our results reveal that the MCE and transition temperature of Mn50Ni40Sn Sb x alloys are strongly dependent on the Sb concentration, and demonstrates that Sb-doped Mn2NiSn alloys are competent candidates for refrigeration applications.

2. Experimental details

A series of polycrystalline Mn-rich Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys were prepared by arc-melting the appropriate amounts of high-purity Mn, Ni, Sn, and Sb (99.95 wt.% purity) in an argon atmosphere. The samples were re-melted three times to enhance their homogeneity. The resultant samples were then sealed in vacuum quartz tubes and annealed at 1073 K for three days before being quenched in cold water. The martensitic transformations in the Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys were identified by differential scanning calorimetry (DSC) in the temperature range 150–350 K with a cooling and heating rate of 10 K/min. The crystal structure was investigated by x-ray powder diffraction (XRD) using Cu- radiation at room temperature (RT). The target compositions were confirmed through x-ray energy dispersive spectrometry (EDS), and the results are presented in Table 1. The magnetic measurements were carried out on a physical property measurement system (PPMS).

Table 1.

The measured compositions and structural parameters of Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys.

.
3. Results and discussion

The RT XRD patterns of the Mn-rich Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys are shown in Fig. 1. The presence of (220), (400), and (422) peaks indicates that the Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys exhibit a Heusler-type B2 structure with the space group at RT. Using the XRD data, the lattice parameter a and unit cell volume were calculated (listed in Table 1). Because the atomic size of Sb ( Å) is smaller than that of Sn ( Å), both a and unit cell volume decrease with increasing Sb content.

Fig. 1. (color online) XRD patterns of Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys at room temperature.

The thermal-induced structural transformations in the Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys were investigated by DSC in heating and cooling cycles. As shown in Fig. 2, large endothermic and exothermic peaks are observed, corresponding to the occurrence of the first-order structural transformation between martensite and austenite. As x increases from 1 to 4, the endothermic and exothermic peaks in the heating and cooling processes increase by 37 K and 38 K, respectively. It has been reported that the structural transformation temperature in Ni–Mn-based magnetic shape memory alloys is strongly related to e/a. The calculated e/a for the Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys are given in Table 2. Here, the 3d and 4s electrons are considered as valence electrons in transition metals, and the 5s and 5p electrons are considered to be valence electrons in main-group elements. Because Sn has fewer 5p electrons than Sb, e/a increases with the Sb content. With the increase in e/a, the structural transformation shifts to higher temperatures. A similar relation between the structural transformation temperature and e/a has been observed in other Ni–Mn-based magnetic shape memory alloys.[2225] Additionally, previous reports on Ge-doped NiMnSn and Ga-doped NiMnIn alloys indicate that the structural transformation temperature increases as the unit cell volume decreases.[26,27] In the present study, the Sb substitution causes the lattice to shrink, which may enhance the hybridization between Ni and Mn/Sn, leading to an increase in the structural transformation temperature.[28]

Fig. 2. (color online) DSC curves of Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys.
Table 2.

The martensitic start temperature ( , martensitic finish temperature ( , austenitic start temperature ( , austenitic finish temperature ( , and valence electron concentration ( for Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys.

.

Figure 3 shows the temperature dependence of magnetization ( for the samples under an applied magnetic field of 0.01 T in the heating and cooling processes. In the heating process, the Mn50Ni40Sn9Sb1 alloy experiences the magnetic order–disorder transition of martensite at approximately 170 K, followed by a sharp MT to ferromagnetic austenite at around 198 K. With further heating to 313 K, the magnetization in this sample gradually decreases to zero, corresponding to the Curie temperature of austenite. An obvious irreversibility between the heating and cooling curves is observed during the MT, indicating the first-order nature of this transition. The characteristic temperatures of the MT, austenitic start temperature , austenitic finish temperature , martensitic start temperature , and martensitic finish temperature , are listed in Table 2. As compared in Table 2 and Fig. 3, the MT shifts to higher temperatures asxincreases, which agrees with the DSC measurements. As the transformation temperature is tuned to be close to the Curie temperature of austenite, the magnetization of austenite decreases remarkably with Sb substitution, leading to low values of .

Fig. 3. (color online) MTcurves for Mn50Ni40Sn Sb x alloys: (a) x = 1, (b) x = 2, (c) x = 3, and (d) x = 4, under an applied magnetic field of 0.01 T during the heating and cooling processes.

To study the magnetic properties around MT in more detail, the isothermal magnetization (MB) was measured by the so-called loop method.[29] Before applying the magnetic field, the samples were cooled to full martensitic state, then slowly heated to the measurement temperature with a ramp rate of 3 K/min. As shown in Fig. 4, the metamagnetic behavior can be observed when the temperature is close to , which corresponds to the magnetic field-induced MT from martensite to austenite. The existence of magnetic hysteresis indicates the first-order nature of the transition. The observed magnetic field-induced MT is related to between martensite and austenite.[30] For x = 1, 2, 3, and 4, the values of under 5 T are 42 A·m2/kg, 40 A·m2/kg, 26 A·m2/kg, and 28 A·m2/kg, respectively. The decrease of leads to the reduced magnetic field driving capacity in Mn50Ni40Sn6Sb4 alloy.

Fig. 4. (color online) MB curves for Mn50Ni40Sn Sb x alloys: (a) x = 1, (b) x = 2, (c) x = 3, and (d) x = 4.

According to the MB curves, the isothermal magnetic entropy change ( as a function of temperature was estimated under different magnetic field variations for Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys using Maxwell's equation:[31]

(1)
As shown in Fig. 5, the maximum values of under a magnetic field variation of 0–5 T are 19.16 J·kg K , 17.29 J·kg K , 12.63 J·kg K , and 8.65 J·kg K for x = 1, 2, 3, and 4, respectively. As the magnetic field variation decreases to 0–2 T, the corresponding values reduce to 9.17 J·kg K , 6.67 J·kg K , 4.63 J·kg K , and 2.88 J·kg K , respectively. The values of decrease with the increase in Sb content. The maximum values of in Fig. 5 are comparable to those in Mn50Ni Co x Sn10 and Ni Co x Mn32Al18 ferromagnetic shape memory alloys.[32,33] As well as , the effective refrigeration capacity (RC ) is an important parameter for evaluating the magnetic cooling capacity of MCE materials. The RC of Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys was determined by subtracting the average hysteresis loss (HL) from the refrigeration capacity (RC). Here, the values of RC were obtained by integrating the area under the curves as a function of temperature within the full width at half maximum, and the average HL was calculated from the area surrounded by the MB curves in Fig. 4. For Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys, the RC values are found to be 131.9 J·kg , 123.9 J·kg , 72.1 J·kg , and 71.9 J·kg and the average HL values are 88.2 J·kg , 84.8 J·kg , 35.3 J·kg , and 17.5 J·kg , respectively. Therefore, the corresponding RC is 43.8, 39.1 J·kg , 36.8 J·kg , and 54.5 J·kg under a magnetic field variation of 0–5 T. Furthermore, as the MT of Mn-rich Mn50Ni40Sn Sb x alloys is highly dependent on the Sb content, the MCE can be tuned over a wide temperature range, which is a valuable property for magnetic refrigerants.

Fig. 5. (color online) Temperature dependent for Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys.
4. Conclusion

In summary, we investigated the effect of Sb substitution on the martensitic transformation and magnetocaloric properties of Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys. The Mn-rich Mn50Ni40Sn Sb x (x = 1, 2, 3, and 4) alloys have a B2-type structure at RT. As the Sb content increases, the MT shifts to higher temperatures. The magnetization difference between martensite and austenite means that the MT can be induced by an applied magnetic field. Obvious metamagnetic behavior can be observed in the MB curves. The coupled maximum values with a magnetic field variation of 0–5 T are 19.16 J·kg K , 17.29 J·kg K , 12.63 J·kg K , and 8.65 J·kg K for x = 1, 2, 3, and 4, respectively. The tunable MCE indicates the potential for promising applications as a magnetic cooling refrigerant.

Reference
1 Jaronie M J Martin L Aleksandar S Mark A G 2014 Mater. Design 56 1078
2 Guillou F Porcari G Yibole H Van Dijk N Bruck E 2014 Adv. Mater. 26 2671
3 Gutfleisch O Willard M A Bruck E Chen C H Sankar S G Liu J P 2011 Adv. Mater. 23 821
4 Zhang H Shen B G 2015 Chin. Phys. B 24 127504
5 Hu F X Shen B G Sun J R Wang G J Cheng Z H 2002 Appl. Phys. Lett. 80 826
6 Tegus O Bruck E Buschow K Boer F D 2002 Nature 415 150
7 Liu J Gottschall T Skokov K P Moore J D Gutfleisch O 2012 Nat. Mater. 11 620
8 Hu F X Shen B G Sun J R 2013 Chin. Phys. B 22 037505
9 Wang D H Han Z D Xuan H C Ma S C Chen S Y Zhang C L Du Y W 2013 Chin. Phys. B 22 077506
10 Umetsu R Y Sheikh A Ito W Ouladdiaf B Ziebeck K R A Kanomata T Kainuma R 2011 Appl. Phys. Lett. 98 042507
11 Ma S C Shih C W Liu J Yuan J H Lee S Y Lee Y I Chang H W Chang W C 2015 Acta Mater. 90 292
12 Luo H Meng F Jiang Q Liu H Liu E Wu G Wang Y 2010 Scripta Mater. 63 569
13 Gong Y Y Wang D H Cao Q Q Liu E K Liu J Du Y W 2015 Adv. Mater. 27 801
14 Li P P Wang J M Jiang C B 2011 Chin. Phys. B 20 028104
15 Kainuma R Ito W Umetsu R Y Oikawa K Ishida K 2008 Appl. Phys. Lett. 93 091906
16 Tian L G Hong L Z Yan M F Qiao M X Heng W G 2013 Chin. Phys. B 22 126201
17 Llamazares J L S Sanchez T Santos J D Perez M J Sanchez M L Hernando B Escoda L Sunol J J Varga R 2008 Appl. Phys. Lett. 92 012513
18 Wu Z Liu Z Yang H Liu Y Wu G 2011 Appl. Phys. Lett. 98 061904
19 Xuan H C Zheng Y X Ma S C Cao Q Q Wang D H Du Y W 2010 J. Appl. Phys. 108 103920
20 Liu Z H Aksoy S Acet M 2009 J. Appl. Phys. 105 033913
21 Xuan H C Han P D Wang D H Du Y W 2014 Intermetallics 54 120
22 Hernando B Llamazares J L S Santos J D Escoda L Sunol J J Varga R Baldomir D Serantes D 2008 Appl. Phys. Lett. 92 042504
23 Santos J D Sanchez T Alvarez P Sanchez M L Llamazares J L S Hernando B Escoda L Suñol J J Varga R 2008 J. Appl. Phys. 103 07B326
24 Han Z D Wang D H Zhang C L Xuan H C Gu B X Du Y W 2007 Appl. Phys. Lett. 90 042507
25 Ito W Xu X Umetsu R Y Kanomata T Ishida K Kainuma R 2010 Appl. Phys. Lett. 97 242512
26 Han Z D Wang D H Zhang C L Xuan H C Zhang J R Gu B X Du Y W 2009 Mater. Sci. Eng. B 157 40
27 Aksoy S Krenke T Acet M Wassermann E F Moya X Manosa L Planes A 2007 Appl. Phys. Lett. 91 241916
28 Priolkar K R Lobo D N Bhobe P A Emura S Nigam A K 2011 Europhys. Lett. 94 38006
29 Caron L Ou Z Q Nguyen T T Thanh D T C Tegus O Bruck E 2009 J. Magn. Magn. Mater. 321 3559
30 Xuan H C Han P D Wang D H Du Y W 2014 J. Alloy. Compd. 582 369
31 Han Z Chen X Zhang Y Chen J Qian B Jiang X F Wang D H Du Y W 2012 J. Alloys. Compd. 515 114
32 Sharma J Suresh K G 2015 J. Alloys. Compd. 620 329
33 Xuan H C Chen F H Han P D Wang D H Du Y W 2014 Intermetallics 47 31