Due to the limits of conventional perpendicular magnetic recording, it appears that alternative technologies are needed at areal densities >500 Gb/in 2 . Heat-assisted magnetic recording (HAMR) is a promising approach to extend areal densities to 1 Tb/in 2 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
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Rottmayer et al. (2006) studied this question.
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