Influence of annealing on martensitic transformation and magnetic entropy change in Ni37.7Co12.7Mn40.8Sn8.8 magnetic shape memory alloy ribbon

https://doi.org/10.1016/j.jmmm.2014.10.077Get rights and content

Highlights

  • Annealing below or above 1173 K had different effects on transformation temperatures of Ni37.7Co12.7Mn40.8Sn8.8 ribbon, which was due to the formation of second phases.

  • A large magnetic entropy change of 15 J/kg K was obtained above 400 K in both the as-spun ribbon and that annealed at 973 K.

  • To achieve a giant high-temperature MCE in Ni37.7Co12.7Mn40.8Sn8.8 ribbon, the annealing temperature should not exceed 973 K.

Abstract

The microstructure, martensitic transformation and magnetic properties of Ni37.7Co12.7Mn40.8Sn8.8 high temperature magnetic shape memory ribbon subjected to different annealing temperature were investigated. Annealing up to 1073 K slightly raised the transformation temperatures and the transformation interval, while annealing at 1173 K considerably decreased the transformation temperature and strongly widened the transformation interval due to the formation of a second phase. The as-spun and annealed ribbon at 973 K exhibited giant magnetic entropy changes of around 15 J/kg K under 15 kOe magnetic field above 400 K. Further increasing annealing temperature caused a decrease of the magnetic entropy change. To achieve a large magnetocaloric effect while keeping an elevated transformation temperature, an appropriate annealing parameter should be carefully considered.

Introduction

Ni–Mn–Sn, including Ni–Co–Mn–Sn, magnetic shape memory alloys (MSMAs) have attracted much attention [1], [2], [3], [4]. Ni–Mn–Sn alloys undergo a first order magneto-structural transition between the paramagnetic/antiferromagnetic martensite phase and the ferromagnetic austenite phase upon heating and cooling [1], [5]. Due to a large magnetization change (ΔM) between the martensite and austenite, the phase transition can be driven by a moderate magnetic field resulting in a large magnetic-field-induced strain (MFIS), giant magnetocaloric effect (MCE) and magneroresistance (MR) [1], [2], [3], [6], [7], [8]. Compared with other Ni–Mn–X (X=In, Ga, Sb) MSMAs, Ni–Mn–Sn has relatively low cost, which makes it more competitive for practical applications. Recently, a giant MCE with an effective magnetic refrigeration capacity of 251 J/kg for 5 T near room temperature was reported in Ni40Co10Mn40Sn10 polycrystalline sample, revealing the promising prospect of Ni–Co–Mn–Sn as a room-temperature magnetic cooling material [9].

The melt spinning technique is an effective method to fabricate homogeneous MSMAs ribbons with a refined and highly textured polycrystalline microstructure [6], [10], [11], [12]. Due to the rapid solidification during processing, some lattice defects and internal stress may be introduced into the ribbons [13]. Thus, an appropriate post-annealing for a short time is of necessity. In addition, the ordering degree and the phase constitution would be changed by the post-annealing [14], which subsequently should have a remarkable effect on the martensitic transformation and magnetic properties. Up to now, some groups had reported the effect of annealing on the transformation temperatures, Curie temperature (Tc) and the MCE in MSMAs ribbons [5], [14], [15], [16], [17]. Whereas, it was evident that such a influence was very complex. For example, the peak magnetic entropy change (ΔSm) of an as-spun Ni44.1Mn44.2Sn11.7 ribbon increased from about 8–32.1 J/kg K by annealing at 1123 K and reduced to 20.1 J/kg K with additional annealing at 1173 K [5]. Liu et al. [14] also reported effects of annealing on Ni45Mn37In13Co5 and Ni46Mn35In14Co5 ribbons. For the former, annealing enhanced ΔM and promoted the magnetic-field-induced transformation (MFIT). In contrast, in the latter ribbon, with increasing the annealing time at 1173 K, the MFIT was smeared and the MCE was weakened due to the formation of second phase particles. Therefore, it is essential to carry out more investigations on the effect of annealing on various Ni–Mn–X ribbons, particularly those tending to precipitate the second phase in some cases.

In this paper, we prepared a Ni–Co–Mn–Sn ribbon with 12.7 at% Co undergoing a martensitic transformation above 373 K, which belonged to a high temperature MSMA. We found the presence of second phases after high temperature annealing, which was seldom reported in Ni–Co–Mn–Sn ribbon. We also discussed the effect of annealing on the microstructure, the martensitic transformation, and the MCE.

Section snippets

Experimental procedures

The as-cast Ni–Co–Mn–Sn alloy was inductively melted in a quartz tube and then ejected onto a rotating copper wheel to produce the ribbons. The surface velocity of the wheel was 10 m/s. Three ribbons were then sealed in vacuum quartz tubes and annealed for 30 min at 973, 1073 and 1173 K, followed by quenching in water. For simplicity, these three samples are denoted as A, B and C ribbons. The microstructure and atomic composition were examined by scanning electron microscopy (SEM) equipped with

Results and discussion

Fig. 1 shows the microstructures of the ribbons annealed at different temperatures. Martensite plates were present in the as-spun (Fig. 1a), A (Fig. 1b) and B (Fig. 1c) ribbons. For the C ribbon (Fig. 1d), a two-phase microstructure was found consisting of the martensite and the particulate-shaped second phase γ. EDS result showed that the detailed composition of γ phase was Ni31.2Co23.4Mn43.7Sn1.7 (at%). In comparison with the matrix (Ni37.6Co10.4Mn40.3Sn9.7), in the γ phase, the Co content

Conclusions

In summary, effects of the annealing temperature on the martensitic transformation and magnetic properties in Ni37.7Co12.7Mn40.8Sn8.8 ribbon were investigated. Annealing at 973 and 1073 K lead to a small rise in the transformation temperatures from 402 to 410 K for As and slightly widened the transformation interval. Annealing at 1173 K reduced the transformation temperatures (As≈317 K) and greatly increased the transformation interval, which could be ascribed to the formation of the Co-rich γ

Acknowledgment

We appreciate technical assistance of Nikole Kucza and Charles Patrick at the VSM, and Brittany Muntifering at the XRD. This work was supported by the National Natural Science Foundation of China (No. 51101040), Harbin Special Fund for Innovation Talents of Science and Technology (2013RFLXJ030), and the State Scholarship Fund of China. PM acknowledges financial support through the National Science Foundation through projects DMR-1207192 and CMMI-1068069, and NSF MRI award 0619795 (XRD).

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