R3（Fe,Mo）29（R=Sm,Y）化合物及其氮化物的磁性

合成了Ｒ３（Ｆｅ,Ｍｏ）２９（Ｒ＝Ｓｍ,Ｙ）化合物并在０．１ＭＰａ氮气条件下通过气相氮化法制备出其氮化物。Ｒ３（Ｆｅ,Ｍｏ）２９金属间化合物氮化后仍保持母相结构,但是晶胞体积发生膨胀,氮化处理同时导致化合物居里温度Ｔｃ和饱和磁化强度σｓ升高同时Ｓｍ３（Ｆｅ,Ｍｏ）２９化合物由平面各向异性变为单轴各向异性,但Ｙ３（Ｆｅ,Ｍｏ）２９Ｎｘ化合物的各向异性仍与母相相同,为面各向异性。     

用Ga取代部分Fe对R3（Fe,Mo）29结构及磁性的影响

详细研究了Ｇａ取代Ｒ３（Ｆｅ,Ｍｏ）２９（Ｒ＝Ｓｍ,Ｙ）（Ｇａ＜０．１５）中的部分Ｆｅ对其结构和内禀磁性的影响,包括不同的Ｇａ取代对Ｒ３（Ｆｅ,Ｍｏ）２９化合物的晶胞常数、居里温度、饱和磁化强度、磁晶各向异性的影响。结果表明：在Ｒ３（Ｆｅ,Ｍｏ,Ｇａ）２９化合物中,随着Ｇａ含量的增加,晶胞体积膨胀,居里温度升高,饱和磁化强度下降,Ｆｅ原子的平均磁矩降低,Ｓｍ３（Ｆｅ０．９６６－ｘＭｏ０．０３４Ｇａｘ）２９化合物的各向异性由平面向锥面结构转变,继续增加Ｇａ含量,有可能出现单轴各向异性。     

代位合金元素原子在Fe3Al金属间化合物亚点阵占位的中子衍射研究

用中子衍射分析法研究了Ｃｒ，Ｍｏ，Ｔｉ，Ｎｉ，Ｍｎ，Ｓｉ等代位合金元素当量成分，ＤＯ３结构Ｆｅ３Ａｌ金属间化合物亚点阵中的原子占位及其对单胞中Ｆｅ原子磁矩，ＤＯ３－Ｂ２转变行为的影响。     

18Ni马氏体时效钢时效机理的研究

采用小角Ｘ射线散射、Ｍｏｓｓｂａｕｅｒ谱、透射电镜等方法研究了１８Ｎｉ马氏体时效钢的时效过程。结果表明，１８Ｎｉ合金在固溶处理后５００℃等温时效过程中，首先发生调幅分解，然后在调幅组织的Ｎｉ－Ｍｏ－Ｔｉ富集区以原位形核方式析出含Ｆｅ的Ｎｉ３（Ｍｏ、Ｔｉ）型金属间化合物，随时效时间延长，Ｎｉ３Ｍｏ和Ｎｉ３Ｔｉ粒子聚集长大并部分溶解，同时析出球形Ｆｅ２Ｍｏ金属间化合物，并形成逆转变奥氏体。     

R3（Fe,M）29化合物中的Fe—Fe及R—Fe之间的交换作用

根据Ｒ３（Ｆｅ，Ｍ）２９（Ｒ＝稀土，Ｍ＝Ｖ、Ｔｉ、Ｍｏ）化合物的居里温度的实验值，使用平均场近似的方法计算Ｒ３（Ｆｅ，Ｍ）２９化合物中的Ｒ－Ｆｅ，Ｆｅ－Ｆｅ之间的交换耦合参数ＪＲＦｅ和ＪＦｅＦｅ。结果表明：对于Ｒ相同而Ｍ不同时，当Ｍ＝Ｖ时ＪＦｅＦｅ最大，而Ｍ＝Ｍｏ时ＪＦｅＦｅ最小；但是，当Ｍ＝Ｔｉ时ＪＲＦｅ最大，当Ｍ＝Ｍｏ时ＪＲＦｅ最小。     

Y2Fe17—xMnx的结构和磁性

Ｘ射线衍射证实了Ｙ２Ｆｅ１７－ｘＭｎｘ的结构与Ｙ２Ｆｅ１７相同Ｙ２Ｆｅ１７－ｘＭｎｘ化合物晶格常数，居里温度，饱和磁化强度和研究结果表明：晶格常数并非随Ｍｎ含量的增加而连续增大，而是在ｘ＝２．０处出现一最小值。     

W, Co, Ni对时效合金强度和韧性的影响

研究了Ｗ,Ｃｏ,Ｎｉ对时效合金强度和韧性的影响。结果表明：高Ｃｏ的ＦｅＷＣｏ合金有强的时效硬化能力,但其韧性较低。以Ｎｉ取代部分Ｃｏ之后,合金的韧性得到大的提高。ＦｅＷＣｏ合金的Ｃｏ量约２３％,Ｗ,Ｍｏ总量超过１８％时,硬度增加甚少,韧性损害较大,而ＦｅＷＣｏＮｉ的Ｃｏ当量达２３％,Ｗ,Ｍｏ总量达２４％时获得最佳的强度和韧性的配合。萃取化合物的Ｘ射线衍射（ＸＲＤ）分析表明,时效合金的主要金属间化合物是Ｆｅ３Ｗ２型,还有Ｆｅ７Ｗ６和Ｆｅ２Ｗ型化合物。淬火态、退火态萃取物的化学分析表明,时效合金中,Ｗ,Ｍｏ主要存在于化合物中,而Ｃｏ,Ｎｉ主要存在于固溶体中。时效硬化主要通过Ｗ,Ｍｏ金属间化合物的析出引起。而Ｃｏ,Ｎｉ主要通过影响析出相的数量、析出物形态及分布状态来影响时效硬化。     

化学镀Fe—Mo—W—B非晶态合金的晶化

利用化学镀获得非晶态Ｆｅ－Ｍｏ－Ｗ－Ｂ四元合金镀层。用Ｘ射线衍射方法研究了镀层的结构和晶化过程。结果表明;Ｂ含量在９．８ａｔ％－２７．３ａｔ％范围内镀层为非晶态结构,该区域大于Ｆｅ－Ｂ二元合金镀层,但不如Ｆｅ－Ｍｏ－Ｂ三元合金镀层。观察到两步晶化过程：首先析出的晶化相为α－Ｆｅ,Ｆｅ３Ｂ和（Ｍｏ,Ｗ）２Ｂ;然后在较高温度出现Ｆｅ２Ｂ,（Ｍｏ,Ｗ）Ｂ和Ｆｅ（Ｍｏ,Ｗ）的衍射峰。     

中铬强韧抗磨铸铁的研究

改变了中铬铸铁的结晶过程，改善和细化了显微组织。其基体为马氏体，主要碳化物为（ＣｒＦｅ）７Ｃ３和Ｃｒ７Ｃ３，还有Ｆｅ７Ｃ３、Ｃｒ２３Ｃ６、ＭｏＣ等碳化物和ＦｅＭｏＭｎ、Ｆｅ３ＭＯ２等合金化合物，消除了渗碳体（ＦｅＣｒ）３Ｃ。其硬度ＨＲＣ≥５６，与高铬铸铁相当，得到了耐磨性和韧性较高的中铬铸铁、因而中铬铸铁磨球的破碎率低，球磨机的生产率较高。所以复合变质处理并热处理后的中铬强韧铸铁是一种低成本的优质的抗磨铸铁。     

Ga替代对Gd2（Fe,Co）17化合物磁性的影响

通过Ｘ射线衍射和磁性测量手段研究了Ｇｄ２（Ｆｅ０．８Ｃｏ０．２）１７－ｘＧａｘ（０≤Ｘ≤８）化合物的结构和磁性。实验结果表明Ｇｄ２（Ｆｅ０．８Ｃｏ０．２）１７－ＸＣａＸ化合物均为菱方的Ｔｈ２Ｚｎ１７型结构,单胞体积Ｖ随Ｃａ含量的增加单调上升,居里温度Ｔｃ和饱和磁化强度Ｍｓ随Ｇａ含量的增加而单调下降。粉末取向样品的Ｘ射线衍射结果表明,随Ｇａ含量的增加,化合物的室温易磁化方向由易面转变为易轴,Ｇｄ２（Ｆｅ．８Ｃｏ０．２）１７－ＸＣａＸ化合物的３ｄ亚晶格出现室温单轴各向异性可能与Ｃａ原子的择优占位有关。     

Y_3(Fe,M0)_(29)金属间化合物的结构特性

使用Rietveld方法对Y3（Fe,Mo）29金属间化合物的X射线衍射谱和中子衍射谱进行分析,得出了Y3（Fe,Mo）29金属间化合物属A2／m空间群的结论.坐标变换结果表明Y3（Fe,Mo）29金属间化合物的空间结构是1∶12和2∶17的混合结构     

Peculiarities of the R3(Fe,Si)29 phase formation in the Sm---Fe---Si system

The phase content of the Sm(Fe_1−xSi_x)_y alloys (0.05≤x≤0.15; 8.5≤y≤12) has been studied by X-ray diffraction using micromonocrystals. The compounds Sm₂(Fe,Si)₁₇, Sm(Fe,Si)₁₂ and a novel Sm₃(Fe,Si)₂₉ compound with a monoclinic unit cell are found. The lattice parameters of Sm₃(Fe,Si)₂₉ are: a=1.056 nm, b=0.850 nm, c=0.966 nm, β=96.8°. This compound forms as a result of a solid state transformation from the high-temperature Sm₂(Fe,Si)₁₇ phase. Diffuse effects observed in rocking photographs suggest transition structures arising from this transformation. The Curie temperatures of Sm₃(Fe,Si)₂₉ vary in the interval 496–521 K.     

用CBED测定PrCo_(12)B_6化合物的空间群

用会聚束电子衍射(CBED)方法测定了PrCo_(12)B_6化合物的空间群为R3m.     

DETERMINATION OF SPACE GROUP OF PrCo_(12)B_6 COMPOUND BY CONVERGENT BEAM ELECTRON DIFFRACTION

The space group of PrCo_(12)B_6,compound has been determined using the convergent beam elec-tron diffraction method.The space group is found to be R3m.     

Spontaneous volume magnetostriction of Dy2AlFe12Mn4 compound

The structure and magnetic properties of Dy2AlFe12Mn4 compound have been investigated by means of X-ray diffraction and magnetization measurements. The Dy2AlFe12Mn4 compound has a hexagonal Th2Ni17-type structure. Negative thermal expansion was found in Dy2AlFe12Mn4 compound from 229 to 280 K by X-ray dilatometry. The coefficient of the average thermal expansion is α= -3.8×10-5 K-1. The magnetostrictive deformations from 105 to 270 K have been calculated by means of the differences between the experimental values of the lattice parameters and the corresponding values extrapolated from the paramagnetic range. The result shows that the spontaneous volume magnetostrictive deformation ωs; decreases from 6.2×10-3 to near zero with the temperature increasing from 105 to 270 K, the spontaneous linear magnetostrictive deformation λc. along the c axis is much larger than the spontaneous linear magnetostrictive deformation λa in basal-plane at the same temperature except close to 249 K.     

Ce(Au,Sb)2 with UHg2 structure type, a new member of the AlB2 family

A new ternary compound Ce(Au,Sb)₂, with a homogeneity range has been observed from X-ray powder diffraction of as cast alloys, a = 4.743–4.712 Å, c = 3.567–3.768 Å. Its crystal structure was investigated by X-ray diffraction from Ce(Au_1−xSb_x)₂ (x = 0.266) single crystal: CAD-4 automatic diffractometer, Mo K radiation, a = 4.7256(6) Å, c = 3.6711(6) Å, P6/mmm space group, V = 70.997(17) Å³, Z = 1, ρ = 10.732 Mg/m³, μ = 76.369 mm⁻¹, R₁ = 0.0415, wR₂ = 0.0793 for 99 reflections with I > 2σ(I₀). The coordination polyhedron of X (X = 0.734Au + 0.266Sb) atom is a full-capped trigonal prism [XCe₆X₃X₂]. Ce atom is coordinated by 14 atoms: [CeX₁₂Ce₂]. The compound is isotypic with UHg₂ structure, a deformation derivative of AlB₂ structure type. It forms isostructural compounds with La and Pr.     

Nd3（Fe,Mo）29化合物及其氮化物的磁结构和内禀磁性

制备了具有Nd3（Fe,Ti）29型单斜结构的单相铁基金属间化合物Nd3（Fe,Mo）29及其氮化物,详细研究了：其在4．2K～300K之间的磁结构;磁晶各向异性;居里温度Tc,饱和磁化强度σs等内禀磁性。研究结果表明：Nd3（Fe,Mo）29金属间化合物氮化后仍保持母相结构,氮化后的晶胞体积,居里温度Tc和饱和磁化强度σs分别比氮化前提高了5．9％,70．9％,6．6％;N3d（Fe,Mo）29金属间化合物在230K左右存在自族重取向,温度低于230K时,其磁晶各向异性为锥面,温度高于230K时,其磁晶各向异性为易面;氮化后自族重取向消失。     

Phase diagram of the CsBr-CaBr2 system

The phase diagram of the CsBr-CaBr2 system was re-determined by using differential thermal analysis and high ternperature and room ternperature X-ray diffraction analysis. It is concluded that there are three intermediate compounds in this system： a.congruently melting compound, CsCaBr3, with a melting point of 823℃ and two incongruently melting compounds, Cs2CaBr4 and Cs3Ca2Br7, whose peritectic points being 597℃ and 635℃, respectively. X-ray diffraction analysis indicated that compound CsCaBr3 is of slightly distorted perovskite structure.     

Crystal structure of La5Ti4GaO17

The crystal structure of La₅Ti₄GaO₁₇ compound synthesized by heat-treatment of the co-precipitated hydroxy-oxalates has been determined by the X-ray powder diffraction. It was found that crystal structure of La₅Ti₄GaO₁₇ belongs to the CaLa₄Ti₅O₁₇-type structure (space group Pmnn, a = 0.3912(1) nm, b = 3.128(1) nm, c = 0.5523(1) nm, Z = 2). The final R_W value is equal to 0.081 for 169 independent reflections.     

The 473 K isothermal section of the Cu–Ti–Sn ternary system

The phase relationships of the Cu–Ti–Sn ternary system at 473 K have been investigated mainly by means of X-ray powder diffraction (XRD), scanning electron microscopy (SEM), optical microscopy (OM) and differential thermal analysis (DTA). The isothermal section consists of 17 single-phase regions, 33 two-phase regions and 17 three-phase regions. The existence of 12 binary compounds and 2 ternary compounds, namely Cu₄Ti, Cu₃Ti₂, Cu₄Ti₃, CuTi, CuTi₂, Cu₃Sn, Cu₆Sn₅, Ti₃Sn, Ti₂Sn, Ti₅Sn₃, Ti₆Sn₅, Ti₂Sn₃, CuTi₅Sn₃ and CuTiSn, are confirmed in the Cu–Ti–Sn ternary system at 473 K. No new ternary compound is found. The maximum solid solubility of Cu in Ti₆Sn₅ was approximately 10 at.% Cu.