ABSTRACT

Perpendicularmagnetic recording (PMR) in hard disk drives (HDDs)

for computer and consumer electronic applications has been a long-

awaited technology. It was first proposed by S. Iwasaki in 1975

[1] but commercialized in 2005 by Toshiba [2] with 40 GB/1.8-

inch platter (133 Gbits/in2). Implementation of PMR technology has

almost taken three decades due to many challenges and making it

competitive over well-established longitudinal magnetic recording

(LMR) technology. In LMR, a continuous reduction of grain size in

metallic CoCrPt-based alloys is themajor contribution for improving

areal densities. A further increase in the recording density of

≥100 Gbits/in2 needed a grain size smaller than 9 nm and a narrower grain size distribution; this grain size was approaching the

fundamental superparamagnetic limit [3], which leads to thermal

instability in the recording medium. A combination of oriented LMR

media with antiferromagnetically coupled longitudinal magnetic

layers [4] allowed improving thermal stability caused by Mrt (a product of remanent magnetization and thickness) cancellation,

thus partially extending the limit of LMR. A significant increase

of areal density was obtained by introducing PMR technology

with a thicker magnetic recording layer, which provides sufficient

thermal stability and high Mrt as well as high head field strength and gradient. The possibility of PMR to achieve 1 Tbit/in2 was

speculated around 2000 [5, 6]. PMR has made remarkable progress

in the past one decade and the areal density is now approaching

∼920 Gbits/in2. After analyzing different generations of PMR media, significant reduction of magnetic cluster size is highlighted,

while keeping similar structural grain size [7]. Shingled magnetic

recording (SMR) [8] is considered a possible extension of current

PMR technology for areal densities >1 Tbit/in2. SMR media with

track density benefit are developing with similar PMR materials but

advanced head and media design concepts for further improving

areal densities.