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R&D: Experimental Study of Media Heat Sink Thickness Impact on Signal-to-Noise Ratio in HAMR

Thicker HS is trade-off between BGI and thermal gradient; thus, it remains challenging to achieve ultra-high areal density using thermal media design.

Japanese Journal of Applied Physics has published an article written by Somyot Kaitwanidvilai, Nuttapon Chaiduangsri, Department of Electrical Engineering, King Mongkut’s Institute of Technology Ladkrabang, Bangkok, 10520, Thailand, and Damrongsak Tongsomporn, Seagate Technology (Thailand) Ltd., Samutprakarn, 10270 Thailand.

Abstract:Recently, heat-assisted magnetic recording (HAMR) has been demonstrated to extend the areal density growth over the superparamagnetic limited. One key component of this technology is a heat sink layer in HAMR media, which benefits the thermal gradient and transition noise. However, the disadvantage of the heat sink layer (HS) has not been fully explored. In this paper, we investigate the background interference (BGI) impact as a result of the heat sink layer via the spin-stand tester. HAMR heads included a light delivery system that have measured a signal-to-noise ratio and down-track thermal gradient on a variety of HS thickness. Subsequently, we found that a thicker HS is a trade-off between the BGI and thermal gradient. Thus, it remains challenging to achieve an ultra-high areal density using the thermal media design.

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