Diamond-like carbon for magnetic storage disks
Section snippets
Magnetic storage technology
Magnetic storage is the most economic form of non-volatile storage for many applications [1], [2], [3], [4], [5], [6], [7], [8], [9], [10], [11], [12], [13], [14]. Its great advantage is that the storage density is increasing at a very rapid rate [1], [2], [3], [4], [5] (Fig. 1). Recently, with the introduction of giant magneto-resistive heads, storage densities are increasing at 100% per year. This is much faster than the Moore's law rate for silicon devices (∼50% per year).
Data are stored in
Classification of carbon films
The main properties of the various carbon films are well known, at least for films thicker than 10 nm [20]. Here we present a general classification of carbon films in terms of their bonding and some useful correlations linking mechanical and structural properties of ta-C.
The great versatility of carbon materials arises from the strong dependence of their physical properties on the ratio of sp2 (graphite-like) to sp3 (diamond-like) bonds [20]. There are many forms of sp2 bonded carbons with
Requirements for the carbon overcoat
When first introduced, the role of carbon films was to provide protection against corrosion. Simple a-C was used, deposited by magnetron sputtering. Later, a-C:H was used, produced by the reactive sputtering of graphite in an Ar/hydrogen atmosphere [27], in order to provide also some protection against mechanical wear and damage during head crashes [28], [29], [30], [31]. Many groups have emphasized this role of DLC for mechanical protection. However, hardness is not the critical parameter. For
Optical storage technology
Optical storage is the preferred technology when high-density storage on removable and exchangeable media is required. The advantages are its low cost, media exchangeability (standardization) and robustness. Over the past 20 years, the storage capacity in optical recording has been raised by increasing the numerical aperture of the focussing optics and decreasing the laser wavelength (Fig. 8a.) The new generation of optical storage devices will have approximately a 20-fold higher capacity than
Ultra-thin carbon films characterization
Finding reliable characterization tools for ultra-thin carbon layers down to a few atomic layers thickness is one of the most decisive factors for technology development and production [51], [52], [53], [54], [55], [56], [57], [58], [59], [60], [61], [62], [63], [64], [65]. The carbon performance is judged in terms of its coverage, lubricant compatibility and mechanical hardness. The mechanical hardness is directly related to the fraction of CC sp3 bonds and the carbon film density. The
Evolution of ta-C properties with thickness
Fig. 14, Fig. 20a allow some interesting conclusions on the thickness evolution of ta-C properties. The density, sp3 fraction and Young's modulus all decrease for films below 8-nm thickness [48]. However, there are distinct trends. The XRR density of a 2.2-nm ta-C film, 2.8 g/cm3, corresponds, by using Eq. (1), to ∼60% sp3 content, similar to that found by direct electron energy loss spectroscopy measurements (∼45%) [48]. In contrast, its Young's modulus (∼100 GPa) would correspond to a much
Conclusions
The status of DLC films to be used as overcoat for magnetic and optical storage disks has been reviewed. The main requirements, such as smoothness, density, corrosion protection have been highlighted. In order to achieve ∼1 Tbit/inch2 storage density the challenges is to provide ∼1-nm films with suitable properties and to be able to assess these properties in a lab and then on the production line. The main non-destructive measurement techniques for structural evaluation of the carbon overcoats
Acknowledgements
The author wishes to thank all the people who allowed the work reviewed in this paper to be performed, in particular the research team of the Mainz IBM STD plant. The author thanks J. Robertson, C. Casiraghi, F. Piazza, R. Ohr, M. Von Gradowsky, C. Shug, H. Hilgers, D. Schneider, M.G. Beghi, C.E. Bottani, A. Libassi, B.K. Tanner. The author acknowledges financial support from the Royal Society, from the project ‘Innovative Reaktoren und In-Situ Analytik für Nano-Schutzschichten’ funded by the
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