FePt-C granular thin film for heat-assisted magnetic recording (HAMR) media

2014 ◽  
Vol 116 (3) ◽  
pp. 1257-1260 ◽  
Author(s):  
L. Zhang ◽  
S.-X. Xue ◽  
Z.-G. Li ◽  
Y.-P. Liu ◽  
W.-P. Chen
2013 ◽  
Vol 21 (8) ◽  
pp. 9906 ◽  
Author(s):  
Z. H. Cen ◽  
B. X. Xu ◽  
J. F. Hu ◽  
J. M. Li ◽  
K. M. Cher ◽  
...  

2013 ◽  
Vol 19 (9-10) ◽  
pp. 1457-1463 ◽  
Author(s):  
Peng Yu ◽  
Weidong Zhou ◽  
Shengkai Yu ◽  
Kyaw Sett Myo

Author(s):  
Joanna E. Bechtel ◽  
David B. Bogy

The lubricant applied to the disk in a hard drive is a critical component for head-disk interface reliability. In Heat Assisted Magnetic Recording (HAMR), the heat supplied to the disk by the laser will add new thermal considerations to lubricant performance. Investigations into how the lubricant behaves at the small time and length scales seen in HAMR systems need to be conducted numerically. Published works on HAMR lubricant modeling have considered only the van der Waals contribution to disjoining pressure, commonly called the dispersive component, and do not consider the film thickness dependence of viscosity. However, lubricants with reactive end groups such as Fomblin Zdol are widely used, and such simple disjoining pressure and viscosity models do not capture certain lubricant behavior. We have developed a simulation tool that incorporates film thickness dependencies of viscosity and polar and dispersive disjoining pressure into a continuum lubrication model. We investigate the effect of initial thickness on lubricant flow and evaporation under HAMR write conditions considering both components of disjoining pressure and thin-film viscosity. Simulation results indicate the effect of including polar disjoining pressure depends on the initial lubricant thickness. The inclusion of viscosity thickness dependence does not affect simulation results under scanning laser conditions but will be important in reflow simulations.


Author(s):  
K. Ogura ◽  
H. Nishioka ◽  
N. Ikeo ◽  
T. Kanazawa ◽  
J. Teshima

Structural appraisal of thin film magnetic media is very important because their magnetic characters such as magnetic hysteresis and recording behaviors are drastically altered by the grain structure of the film. However, in general, the surface of thin film magnetic media of magnetic recording disk which is process completed is protected by several-nm thick sputtered carbon. Therefore, high-resolution observation of a cross-sectional plane of a disk is strongly required to see the fine structure of the thin film magnetic media. Additionally, observation of the top protection film is also very important in this field.Recently, several different process-completed magnetic disks were examined with a UHR-SEM, the JEOL JSM 890, which consisted of a field emission gun and a high-performance immerse lens. The disks were cut into approximately 10-mm squares, the bottom of these pieces were carved into more than half of the total thickness of the disks, and they were bent. There were many cracks on the bent disks. When these disks were observed with the UHR-SEM, it was very difficult to observe the fine structure of thin film magnetic media which appeared on the cracks, because of a very heavy contamination on the observing area.


2017 ◽  
Vol 78 (2) ◽  
pp. 20301
Author(s):  
Kotchakorn Pituso ◽  
Pirat Khunkitti ◽  
Anan Kruesubthaworn ◽  
Komkrit Chooruang ◽  
Damrongsak Tongsomporn ◽  
...  

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