<th id="5nh9l"></th><strike id="5nh9l"></strike><th id="5nh9l"><noframes id="5nh9l"><th id="5nh9l"></th><strike id="5nh9l"></strike>
<progress id="5nh9l"><noframes id="5nh9l"><th id="5nh9l"><noframes id="5nh9l">
<th id="5nh9l"></th> <strike id="5nh9l"><noframes id="5nh9l"><span id="5nh9l"></span>
<progress id="5nh9l"><noframes id="5nh9l"><span id="5nh9l"><noframes id="5nh9l"><span id="5nh9l"></span><strike id="5nh9l"><noframes id="5nh9l"><strike id="5nh9l"></strike>
<span id="5nh9l"><noframes id="5nh9l">
<span id="5nh9l"><noframes id="5nh9l">
<span id="5nh9l"></span><span id="5nh9l"><video id="5nh9l"></video></span>
<th id="5nh9l"><noframes id="5nh9l"><th id="5nh9l"></th>
<progress id="5nh9l"><noframes id="5nh9l">

射頻濺射Fe1-xNix/Cu超晶格的結構與磁性

Structure and Magnetic Properties of RF Sputtered Fe1-xNix/Cu Superlattices

  • 摘要: 應用射頻濺射技術制備了面心立方結構的Fe1-xNix/Cu(x=0.26~0.54)金屬超晶格.Mgo單晶襯底的采用以及在面心立方結構的Cu上實施外延等措施保證了在Ni質量分數低至0.26時Fe-Ni合金層仍保持了良好的面心立方的晶體結構,而且直到液氦溫區這種面心立方結構仍是穩定的.磁性測量表明,當Fe-Ni合金層的Ni質量分數低至接近因瓦合金成分(x=0.35)時,其飽含磁矩呈下降趨勢,即表現出偏離Slater-Pauling規律的傾向.同時,面心立方結構的Fe-Ni合金層的飽合磁矩有很強的溫度依賴性,表明面心立方結構的Fe-Ni合金中飽含磁矩對Slater-Pauling規律的偏離與所謂的馬氏體預相變無關,而與合金中Fe-Fe原子對的反鐵磁性耦合有關.

     

    Abstract: Applying ny sputtering techniques, a series of fcc (Fe1-xNix/Cu)10 superlattices are prepared with Ni concentrations x ranging from 0.26 to 0.54. The use of MgO single crystal substrates and Cu sublayers in the superlattice growth ensure well defined fcc crystal structures in the Fe-Ni sublayers with a Ni concentration as low as 26% and down to liquid helium temperatures.The magnetization of the Fe-Ni sublayers in the super-lattices is reduced when the composition of the Fe-Ni layers approaches the Invar composition, i.e., it shows a deviation from the well-known Slater-Pauling curve. Strong dependence of magnetization on temperature is also observed for the Fe-Ni sublayers with Invar compositions, consistent with the behavior of the bulk Fe-Ni Invar alloys. It is concluded that the deviation of magnetic moment of FeNi alloys near the Invar composition may not be attributed to the so-called premartensitic transformation, but to the Fe-Fe antiferromagnetic interactions in the alloys.

     

/

返回文章
返回
<th id="5nh9l"></th><strike id="5nh9l"></strike><th id="5nh9l"><noframes id="5nh9l"><th id="5nh9l"></th><strike id="5nh9l"></strike>
<progress id="5nh9l"><noframes id="5nh9l"><th id="5nh9l"><noframes id="5nh9l">
<th id="5nh9l"></th> <strike id="5nh9l"><noframes id="5nh9l"><span id="5nh9l"></span>
<progress id="5nh9l"><noframes id="5nh9l"><span id="5nh9l"><noframes id="5nh9l"><span id="5nh9l"></span><strike id="5nh9l"><noframes id="5nh9l"><strike id="5nh9l"></strike>
<span id="5nh9l"><noframes id="5nh9l">
<span id="5nh9l"><noframes id="5nh9l">
<span id="5nh9l"></span><span id="5nh9l"><video id="5nh9l"></video></span>
<th id="5nh9l"><noframes id="5nh9l"><th id="5nh9l"></th>
<progress id="5nh9l"><noframes id="5nh9l">
259luxu-164