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Temperature distribution effects on the magnetization switching in FePt single domain particles

机译:温度分布对近域粒子磁化切换的影响

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The size of magnetic media to record a single bit have decreased drastically in recently years in order to increase the capacity of storage. However, the continued decrease of grain size brings about a severe superparamagnetic limit. One of the ways to overcome the thermal stability due to superparamagnetism is to adopt higher K{sub}u materials as recording medium. However, because the magnetic field of recording heads is limited to ~15kOe, it is difficult to write the high materials. To overcome this problem the concept of the heat assisted magnetic recording (HAMR) was introduced. The basic idea of the HAMR approach is to write bits of information at an elevated temperature close to the Curie temperature, where the switching field is small, and store the information at room or slightly elevated temperature, where the thermostability ratio is high. To achieve significant areal density advantage, the use of high anisotropy intermetallics such as L1{sub}0 ordered phase FePt has been suggested[1]. When the particles are heated by laser, the temperature in the particles is usually not uniform, and has a certain distribution, for example, a Gaussian distribution. In order to shed light on the effect of the temperature distribution in particles on the magnetization switching, extensive Monte Carlo simulations have been performed. We have considered that a rectangular FePt particle of size with and assumed that the temperature in the particle has a Gaussian distribution in xoy plane, T(x,y)=T{sub}m exp{-[(x-v{sub}1){sup}2/(σ{sub}1){sup}2+(y-v{sub}2){sup}2/(σ{sub}2){sup}2]/2}, where (x, y) is the point coordinate and T{sub}m is the maximum temperature in particle and v,σ are constant, which determine the property of the distribution curve. The temperature dependent parameter saturation magnetization M and anisotropy constant K can evaluated in terms of the single-ion model of FePt. As stated in Ref.2, we have m(T)=M(T)/M(0)=[2tanh(x)+tanh(x/2)]/3=5Tx/6T{sub}c (1) k(T)=K(T)/K(0)=tanh(x)tanh(x/2) (2) where T{sub}c is the Curie temperature of FePt.
机译:磁介质的大小在最近几年中急剧下降,以增加存储容量。然而,晶粒尺寸的持续减少带来了严重的超顺磁极限。克服由于超级分析引起的热稳定性的方法之一是采用更高的k {sub} U材料作为记录介质。然而,因为记录头的磁场限于〜15koe,所以难以写高材料。为了克服这个问题,介绍了热辅助磁记录(HAMR)的概念。 HAMR方法的基本思想是在接近居里温度的高温下写入的信息位,其中开关场很小,并将信息存储在室温或稍高的温度下,其中热能比率高。为了实现显着的面部密度优势,已经提出了使用高各向异性的金属间金属间质如L1 {Sub} 0订购的相位剖面[1]。当通过激光加热颗粒时,颗粒中的温度通常不均匀,并且具有一定的分布,例如高斯分布。为了在磁化切换上的颗粒上的温度分布的影响下,已经进行了广泛的蒙特卡罗模拟。我们已经考虑了矩形的矩形粒子,并假设颗粒中的温度在XOY平面中具有高斯分布,T(x,y)= t {sub} m exp { - [(xv {sub} 1) {sup} 2 /(Σ{sub} 1){sup} 2+(yv {sub} 2){sup} 2 /(σ{sub} 2){sup} 2] / 2},其中(x,y )是点坐标和t {sub} m是粒子和v,σ的最大温度,σ是恒定的,这决定了分布曲线的性质。温度依赖性参数饱和磁化M和各向异性常数k可以根据扫描的单离子模型评估。如在参考文献2所述,我们有m个(T)= M(T)/ M(0)= [2tanh(X)+的tanh(X / 2)] / 3 = 5TX / 6T {子} C(1) K(t)= k(t)/ k(0)= tanh(x)tanh(x / 2)(2)其中t {sub} c是yept的居里温度。

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