Energy Barrier Analysis of High Density Hamr Simulations

E. Roddick, Lei Xu, R. Brockie
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Abstract

Some form of heat assistance is likely to be required to achieve >3Tbpsi recording density and continue the long progression of capacity growth of magnetic recording in hard disk drives. To provide useful component design guidance, micromagnetic simulations of heat assisted magnetic recording (HAMR) must include estimates of the areal density of the recording system. In earlier work prepared for Intermag 2020 we investigated the influence of both near-field transducer and medium design on areal density. Exploring a range of medium and NFT designs we demonstrated that once the thermal gradient of the head & medium system is sufficient, the achievable jitter (and hence linear density) is governed by the magnetic properties of the medium. Including read-back parameters, we outlined requirements for HAMR recording systems capable of achieving > 2 Tbpsi in hard disk drives with product margins [1].
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高密度危害模拟的能量势垒分析
可能需要某种形式的热辅助来实现bbb3tbpsi的记录密度,并继续硬盘驱动器中磁记录容量增长的长期进展。为了提供有用的组件设计指导,热辅助磁记录(HAMR)的微磁模拟必须包括记录系统面密度的估计。在为Intermag 2020准备的早期工作中,我们研究了近场换能器和介质设计对面密度的影响。通过探索一系列介质和NFT设计,我们证明,一旦磁头和介质系统的热梯度足够大,可实现的抖动(因此线性密度)是由介质的磁性控制的。包括回读参数,我们概述了能够在硬盘驱动器中实现> - 2 Tbpsi的HAMR记录系统的要求,产品边际为[1]。
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