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中国物理学会期刊

Ni50.5Mn24.5G25单晶的预马氏体相变特性

CSTR: 32037.14.aps.54.263

Characteristics of the premartensitic transition in the Ni50.5Mn24.5G25 single crystals

CSTR: 32037.14.aps.54.263
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  • 通过交流磁化率、电阻、有无磁场下的预相变应变、磁致伸缩和磁化强度测量,系统研究了近正配分比Ni505Mn245Ga25单晶的预马氏体相变特性.在自由样品中观察到预马氏体相变应变.在预相变点,沿010方向施加大小约为80kA/m的磁场,在晶体母相的001方向上获得了高达505ppm的磁致伸缩,该值是相同条件下晶体母相磁致伸缩量的5倍多.同时,报道了不同方向磁场对预相变应变干预的结果.利用软模凝结的概念和依据单晶生长的特点,分析了预相变应变产生的机理.而磁场干预预相变应变的机理是磁场增大的磁弹耦合导致的晶格形变与材料内禀形变的竞争.利用磁性测量结果证实和解释了预相变过程中001和010轴方向间进一步增大的各向异性.进而对磁场沿001和010两个晶体学方向所导致的应变特性的差别,包括最大磁致伸缩、饱和预相变应变、饱和场等,进行了分析和讨论.

     

    The characteristics of premartensitic transition on nearly stoichiometric Ni 505Mn245Ga25 single crystals have been investigated systematic ally by various methods, such as the ac magnetic susceptibility, resistance, mag netostriction, premartensitic transition strain and magnetization measurement. T he premartensitic transition strain in free samples was reported, and the enhanc ed premartensitic transition strain with an external magnetic field applied alon g the different directions was investigated. A large magnetostriction up to 505ppm in the 001 direction of the parent phase is obtained in a pulse magnetic field of about 80kA/m applied along the 010 direction at the premartensitic t ransition point, which is over five times larger than that in the parent phase. Based on the soft mode condensation and characteristic of the crystal growth, th e mechanism of the premartensitic transition strain was analyzed. The effect of magnetic field intervened premartensitic transition strain is attributed to the competition between the crystal lattice deformation induced by the enhancing mag netoelastic coupling and the intrinsic deformation originated from the soft-mode condensation. We found that the premartensitic transition further generated the anisotropy between two crystallographic directions of 001 and 010, which is proved by the magnetization measurement. Furthermore, the resulting strain prop erties, such as the largest magnetostriction, the saturated premartensitic trans ition strain and saturated field, have been discussed in detail.

     

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