Galvanomagnetic properties of Ag/M (M  Fe,Ni, Co) layered metallic films

Magnetoresistance and the Hall Effect have been measured at 4.2, 78, and 300 K for a series of layered metallic films produced by sputtering. The sample periodicity Λ lay between 11 Å and 400 Å. The field and temperature dependencies of the magnetization were measured on a SQUID magnetometer. From the anomalous Hall Effect and magnetization measurements, surface anisotropy parameters are calculated. The magnetoresistance as a function of field direction is sharply peaked when the field is perpendicular to the sample. The associated anisotropy is Λ dependent.     

Magnetic properties of the intermetallic compounds Y15Fe77−xTxB8 (T = Mn,Co, Ni,x = 7, 17)

Magnetic properties of the compounds Y₁₅Fe_77−xT_xB₈, where T stands for Mn, Co or Ni and x equals 7 or 17 were investigated within the temperature range 80 to 650 K. X-ray diffraction yielded a tetragonal structure of Nd₂Fe₁₄B type for all samples. The compounds appeared ferromagnetic: substitution of Mn or Ni for Fe leads to decrease of the Curie temperature and magnetization, while an increase of both quantities was observed for T = Co.     

First-principles study of structural,electronic, and magnetic properties of Mn4XGe3 （X = Fe,Co,Ni）

In order to search for promising candidates for spintronic applications, this paper systematically studies three ternary compounds based on Mn5Ce3 by using a full-potential linearized augmented plane wave method within the density functional theory. Through structure optimization and electronic structure calculations, it finds that Mn4FeCe3 and MnaCoCe3 have much higher spin-polarization than original intermetallic compound Mn5Ce3, although the spin polarization of MnaNiCe3 is lower than that of Mn5Ce3. The calculated result is in agreement with experiment in the case of Mn4FeCe3. Both of them can be taken as promising candidates for spintronics applications because of their high spin-polarization and compatibility with semiconductors.     

Magnetic properties of nanoparticles of Prussian blue-based molecular magnets M 3[Cr(CN)6]2⋅zH2O (M=Fe, Co, and Ni)

The nanoparticles of Prussian blue-based molecular magnets, M ₃[Cr(CN)₆]₂?zH₂O (where M=Fe, Co, and Ni), prepared by a slow addition (drop by drop) of chemicals using the co-precipitation method, are investigated by means of X-ray diffraction, infra red spectroscopy and dc magnetization measurement techniques. The formation of nanoparticles has been confirmed by scanning electron microscopy, whereas the characteristic peak, observed in the range of 1900–2300 cm^?1 in the infrared spectra, corresponds to the CN stretching frequency of $\mbox{Cr}^{\mathrm{+III}}$ –CN– $M^{\mathrm{+II}}$ , and confirms the formation of Prussian blue compounds. The results, derived from the Rietveld refinement of X-ray diffraction patterns, reveal that all samples are nanocrystalline in nature with a face-centered cubic crystal structure of space group Fm3m. The particle size and the lattice constants decrease with an increasing atomic number of the transition metals (M=Fe, Co and Ni). The magnetization data show a magnetically ordered state of all nanoparticle samples with a low coercivity (except for the Fe₃[Cr(CN)₆]₂?zH₂O) as well as the remanent magnetization. In addition, by varying M with Fe, Co and Ni, the magnetic ordering temperature increases from ～12 to ～28 K, whereas the maximum magnetization and the coercive field decrease from ～14 to ～4.5 μ_B/f.u. and ～554 to ～22 Oe, respectively. The observed magnetization behavior has been discussed in terms of the structural changes due to the decreasing particle size as well as the varying nature of the metal ions.     

Structural and Thermodynamic Properties of M3W3N （M=Fe,Co, Ni）

Ternary transition metal nitrides, Fe3 W3N, Coa W3N, and Nia WaN~ are studied by the use of interatomic potentials acquired from lattice inversion. The study indicates that Fe3 WaN would be more stable than the other compounds in the family of intermetallic tungsten nitrides. The investigation of phonon density of states indi- cates that the lower frequency modes are mostly excited by the metal atoms, and the higher frequency modes are mostly excited by the nitrogen atoms. A qualitative analysis is carried out with the relevant potentials for the phase stability and vibrational modes.     

Superconducting and electronic properties of the metallic glass system La75Si25−x M x (M=Cr,Mn, Fe,Co, Ni,Cu, B,Al, Ga,In)

A new ternary metallic glass system, La₇₅Si_25–x M _x (where M is a 3d or a IIIA element) has been prepared by melt spinning. The superconducting transition temperature,T _c , is depressed by the magnetic 3d elements. For low Fe concentrations (less than 5 at.%) the depression is about 0.3 K/at.%. Part of the depression may be explained by a decreased density of states atE _F as determined by UPS measurements. The strongest depression is associated with the magnetic pair breaking due to spin scattering. In the IIIA additions we correlateT _c with the atomic radius of the additive.     

Mn(SiO2)3(M=Fe,Co,Ni;n=1-3)团簇的几何结构、光电性质及磁性

基于密度泛函理论中的广义梯度近似系统研究M_n(SiO₂)₃(M=Fe,Co,Ni;n=1-3)团簇的几何结构、光电性质和磁学性质.结果表明:Fe,Co原子相对于Ni原子更易于在(SiO₂)₃团簇上聚集;通过分析团簇的分裂途径及其产物,发现稳定性较好的氧化硅是一种很好的用于负载过渡金属"岛膜"的载体材料;M_n(SiO₂)₃团簇的能隙恰好位于近红外光谱范围内.通过磁性分析发现,该复合团簇的磁矩主要局域在过渡金属原子周围,而且,Fe₂(SiO₂)₃和Co₃(SiO₂)₃具有相对较大的磁矩,这主要源于过渡金属原子的d轨道间相互耦合.能隙和磁性两方面性质进一步肯定了二氧化硅磁性复合材料在医学界被用作光动力靶向治疗的可观前景.     

Mössbauer study of hydrided amorhous Fe−M−Zr (M=Co,Cr) alloys

Mössbauer spectra of hydrided amorphous Fe₉₀?_xCo_xZr₁₀ (A_x) and Fe₉₀?_yCr_yZr₁₀ (B_y) (x=4, 10, 20; y=0, 4, 7, 13, 16, 20) are studied. For low hydriding time values (t), the average hyperfine field \(\left( {\bar B_{hf} } \right)\) and isomer shift δ_is show a drastic increase which can mainly be associated with the volume effect. For higher (t) values, an electron transfer effect can be responsible for the hyperfine parameter variation. The influence of hydrogenation on magnetic anisotropy is also discussed.     

M@C_(20)H_(20)(M=Sc,V,Cr,Mn,Fe,Co,Ni)几何结构和电子性质的理论研究

采用密度泛函理论(DFT)中的广义梯度近似(GGA)方法对M@C_(20)H_(20)(M=Sc,V,Cr,Mn,Fe,Co,Ni)几何结构和电子性质进行了计算研究.几何结构优化发现,过渡金属原子M内掺到C_(20)H_(20)笼时,都稳定于碳笼中心.能隙和内掺能计算发现,M@C_(20)H_(20)的热力学稳定性随着M原子序数的增大而逐渐减弱,内掺M原子使得其动力学稳定性大幅度下降,但是其中Ni@C_(20)H_(20)结构仍然具有良好的热力学和动力学稳定性,其有望在实验中被成功合成出来.电子性质研究发现,随着M原子序数的逐渐增大,M原子对M@C_(20)H_(20)前线轨道的贡献也越来越大,M@C_(20)H_(20)(M=Sc,V,Cr,Mn,Fe,Co)都具有一定的磁矩,而Ni@C_(20)H_(20)为闭壳层结构,磁矩为零.     

Er3(Fe,Co,M)29化合物(M=Cr,V,Ti,Mn,Ga,Nb)的结构与磁性

合成了Er3Fe29-x-yCoxMy化合物(M=Cr,V,Ti,Mn,Ga,Nb)并用x射线衍射和磁测量等手段研究了它们的结构和磁性.发现Fe基Er3(Fe,M)29化合物结晶成哑铃对Fe-Fe无序替代的Th2Ni17型结构(P63/mmc空间群)而不能形成Nd3(Fe,Ti)29型结构,因此其化学式也可以用Er2-n(Fe,M)17+2n(n=0.2)表示.当Er3Fe29化合物中部分Fe原子被M原子所取代时,其居里温度均有一定程度的提高.所有Er3(Fe,M)29化合物在室温均为易面型各向异性.当Er3(Fe,M)29(M=Cr,V)中的部分Fe原子被Co原子取代且Co原子数与Fe原子数达到一定比值时,得到一个单斜结构的新相.磁测量表明Er3Fei95Co6V3.5在室温可能为单轴各向异性,在162K出现自旋重取向,其各向异性由易轴型变为易面型.在5K下于难磁化方向磁化时观察到一个一级磁化过程(FOMP).     

Mössbauer spectroscopy of single-crystal LiNbO3:Fe(III)

Mössbauer spectra of LiNbO₃: Fe(III)-monocrystals in external magnetic fields of 0.3–7T with various configurations of the -direction, c-axis of the crystal, and the magnetic field direction are interpreted by means of a spin Hamiltonian. A consistent set of hyperfine and crystal-field parameters could be least squares fitted for all spectra. Arguments that Fe(III) substitutes Nb(V) are given.Work partly performed in ICEx/UFMG, Depto. de Fisica, Belo Horizonte, Brasil     

Structure,magnetic properties and magnetocaloric effects of Fe50Mn15−x Co x Ni35 alloys

Fe50Mn15-xCoxNi35(x=0,1,3,5,7)alloys were prepared by arc melting under purified argon atmosphere.The ingots were homogenized at 930°C for 90h followed by water quenching.The crystal structure,magnetic properties and magnetocaloric effects of the alloys were studied by X-ray diffraction(XRD)and MPMS-7-type SQUID.The results show that all samples still maintained a single-(Fe,Ni)-type phase structure.With the increase of the content of Co,the Curie temperatures of these alloys increased and exhibited a second-order magnetic transition from ferromagnetic(FM)to paramagnetic(PM)state near Curie temperature.The maximum magnetic entropy change and the relative cooling power of Fe50Mn10Co5Ni35alloy was 2.55 J/kg·K and 181 J/kg,respectively,for an external field change of 5T.Compared with rare earth metal Gd,Fe50Mn15-xCoxNi35 series of alloys have obvious advantage in resource price;their Curie temperatures can be tuned to near room temperature,maintain a relatively large magnetic entropy change at the same time and they are a type of potential magnetic refrigeration materials near room temperature.     

Fabrication of Fe:CdSe solar rechargeable (semiconductor–septum) storage cells

The Fe:CdSe thin films have been electrodeposited potentiostatically onto the stainless steel substrates, from non-aqueous bath containing (CH₃COO)₂ · Cd · 2H₂O, SeO₂ and FeCl₃. The solar rechargeable (semiconductor–septum) storage cell is fabricated with the configuration C|1 M polysulphide|n-Fe:CdSe|stainless steel||1 M FeCl₃ or 1 M K₄Fe(CN)₆|C. The charging and discharging modes are studied and discussed. The comparison of FeCl₃ and K₄Fe(CN)₆ based solar rechargeable storage cells, showed that FeCl₃ based storage cell is superior than that of K₄Fe(CN)₆ based electrolyte because relatively charging time is minimum and discharging time is maximum. Thus it is concluded that the storage cell works not only as a generator but also as the storage of electricity.     

Magnetic and mechanical properties of Ni–Mn–Ga/Fe–Ga ferromagnetic shape memory composite

A ferromagnetic shape memory composite of Ni–Mn–Ga and Fe–Ga was fabricated by using spark plasma sintering method. The magnetic and mechanical properties of the composite were investigated. Compared to the Ni–Mn–Ga alloy,the threshold field for magnetic-field-induced strain in the composite is clearly reduced owing to the assistance of internal stress generated from Fe–Ga. Meanwhile, the ductility has been significantly improved in the composite. A fracture strain of 26% and a compressive strength of 1600 MPa were achieved.     

Quantum-chemical modeling of the electronic structure and magnetic properties of Sn1 − x − y M x Sb y O2, M = Cr, Mn, Co, or Ni (x = 0.25; y = 0, 0.25)

The electronic and magnetic structures of the Sn_0.75 M _0.25O₂ and Sn_0.5 M _0.25Sb_0.25O₂ (M = Cr, Mn, Co, Ni) compounds with a structure that is derivative of the rutile structure are modeled using the ab initio spin-polarized tight-binding linear muffin-tin orbital (TB-LMTO) method. The magnetic moments of the transition metal atoms are calculated. The data obtained are used to analyze the influence of the composition of Sn_{1 ? x ? y} M _x Sb _y O₂ phases on their electronic spectra and the magnetic and transport characteristics.     

Synthesis and Reactivity of Mg(II)–Fe(II)–Fe(III) Hydroxycarbonates

Green rust-like compounds (GRs) were discovered as natural minerals in various hydromorphic soils, where anoxic conditions allow their stability. They may control some redox processes in aquifers and participate to the transformation of various pollutants. Since Mg(II) cations are present in the fields where GRs were discovered, a partial substitution of Mg(II) to Fe(II) leading to intermediate compounds between GRs and usual Mg(II)–Fe(III) hydroxysalts is suspected. Mg(II)–Fe(II)–Fe(II) hydroxycarbonates can be obtained as intermediate oxidation products of (Mg, Fe)(OH)₂ in carbonate-containing aqueous media obeying to [Fe^II _4(1–x)Mg^II _4x Fe^III ₂(OH)₁₂]²⁺ [CO₃ ^2– nH₂O]^–2. TMS spectra at 12 K are similar to those of GRs, i.e., two quadrupole doublets, one due to Fe(II) with a large isomer shift =1.29 mms^–1 (with respect to -iron at room temperature) and quadrupole splitting E _Q=2.76 mms^–1, the other one due to Fe(III) with smaller hyperfine parameters =0.49 mms^–1 and E _Q=0.44 mms^–1. Fe(II) ions oxidise rapidly into Fe(III) with dissolved O₂. The reactivity is similar to that of Fe(II)–Fe(III) hydroxysalts GR, and thus the potential of Mg(II)–Fe(II)–Fe(III) compounds for reducing pollutants.     

Ionic and electronic transport in perovskite-type La(Ga,M)O3−δ (M=Mg, Cr, Fe, Co, Ni, Nb)

Oxygen ion conduction in La_0.9Sr_0.1Ga_1−xM_xO_3−δ (M=Cr, Fe; x=0 – 0.20), LaGa_1−xM_xO_3−δ (M=Co, Ni; x=0.20 – 0.60), LaGa_1−x−yCo_xMg_yO_3−δ (x=0.35 – 0.60; y=0.10 – 0.25) and LaGa_0.85−xMg_0.15(Nb_0.33Mg_0.66)_xO_3−δ (x=0 – 0.20) is reported. At temperatures below 1200 K the ionic conductivity of La(Ga,M)O_3−δ (M=Co, Ni) increases with increasing oxygen nonstoichiometry, but is lower than for La(Ga,Mg)O_3−δ and (La,Sr)GaO_3−δ. Co-doping with Nb and Mg was found to result in decreasing ionic transport in La(Ga,Nb,Mg)O_3−δ due to blocking of oxygen sites by Nb⁵⁺. Small additions of Fe to the B-site of La_0.9Sr_0.1GaO_3−δ increase the ionic conductivity, whereas substitution of Cr for Ga has the opposite effect. Incorporation of transition metal cations into the Ga site leads to a higher p-type electronic conductivity in all studied perovskites. Paper presented at the 6th Euroconference on Solid Sate Ionics, Cetraro, Calabria, Italy, Sept. 12–19, 1999.