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Heat-Assisted Magnetic Recording

IEEE Transactions on Magnetics · 2006 · Vol. 42(10) · pp. 2417–2421
R. RottmayerS. BatraDorothea BuechelWilliam A. ChallenerJ. HohlfeldYukiko KubotaLei LiBin LüChristophe MihalceaK. R. MountfieldKalman PelhosChao PengTim RauschMike SeiglerD. WellerXiaoMin Yang

Abstract

Due to the limits of conventional perpendicular magnetic recording, it appears that alternative technologies are needed at areal densities >500 Gb/in <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sup> . Heat-assisted magnetic recording (HAMR) is a promising approach to extend areal densities to 1 Tb/in <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sup> and beyond. All of the unique components necessary for a working HAMR system have been demonstrated. Although HAMR permits writing on high Hc media with lower magnetic fields and can produce higher write gradients than conventional magnetic recording, head/media spacing and the development of high Hc media with small grains remains challenging

Magnetic properties of thin filmsPhase-change materials and chalcogenidesAdhesion, Friction, and Surface InteractionsHeat-assisted magnetic recordingRecording mediaArea densityPhysicsComputer scienceMaterials scienceNuclear magnetic resonanceCondensed matter physicsOpticsAcoustics
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