Lee Kyung-Jin, Deac Alina, Redon Olivier, Nozières Jean-Pierre, Dieny Bernard
SPINTEC - Unité de Recherche Associée CEA/DSM & CNRS/SPM-STIC, CEA Grenoble, 38054 Grenoble, France.
Nat Mater. 2004 Dec;3(12):877-81. doi: 10.1038/nmat1237. Epub 2004 Nov 7.
The possibility of exciting microwave oscillations in a nanomagnet by a spin-polarized current, as predicted by Slonczewski and Berger, has recently been demonstrated. This observation opens important prospects of applications in radiofrequency components. However, some unresolved inconsistencies are found when interpreting the magnetization dynamics within the coherent spin-torque model. In some cases, the telegraph noise caused by spin-currents could not be quantitatively described by that model. This has led to controversy about the need for an effective magnetic temperature model. Here we interpret the experimental results of Kiselev et al. using micromagnetic simulations. We point out the key role played by incoherent spin-wave excitation due to spin-transfer torque. The incoherence is caused by spatial inhomogeneities in local fields generating distributions of local precession frequencies. We observe telegraph noise with gigahertz frequencies at zero temperature. This is a consequence of the chaotic dynamics and is associated with transitions between attraction wells in phase space.
正如斯隆切夫斯基和伯杰所预测的那样,最近已证明自旋极化电流可在纳米磁体中激发微波振荡。这一发现为射频组件的应用开辟了重要前景。然而,在相干自旋扭矩模型中解释磁化动力学时,发现了一些尚未解决的矛盾之处。在某些情况下,该模型无法定量描述由自旋电流引起的电报噪声。这引发了关于有效磁温度模型必要性的争议。在此,我们使用微磁模拟来解释基斯列夫等人的实验结果。我们指出了由自旋转移扭矩引起的非相干自旋波激发所起的关键作用。这种非相干性是由产生局部进动频率分布的局部场中的空间不均匀性引起的。我们在零温度下观察到了千兆赫兹频率的电报噪声。这是混沌动力学的结果,并且与相空间中吸引阱之间的跃迁有关。