Requirements for future high-density recording media are discussed. Simple
formulae are given to estimate the effect of media parameters such as coerc
ivity, magnetization, film thickness as well as grain size on achievable ar
eal density. It is found that reducing the grain size is the most important
single factor for achieving higher storage densities. A reduction of grain
size leads to a strong time dependence of coercivity and will eventually l
ead to superparamagnetic behavior. We present experimental data on the time
dependence of coercivity in the range from 5 ns up to a few 100 mu s. A si
mple formula, which takes the random grain orientation in the media into ac
count, is derived and shown to describe the experimental results more satis
factory than previous theories. Furthermore, we investigate very thin films
and show experimental evidence for transition broadening. A simple theoret
ical estimation shows that, for current media materials, (cubical) grains i
n the range of 10-14 nm are predicted to be thermally stable. (C) 1999 Publ
ished by Elsevier Science B.V. All rights reserved.