Magnetic proper ties of Fe
3C nanogr ains embedded in car bon matr ix Y. H. Lee
a), T. C. Han, and J . C. A. Huang
Physics Department, National Cheng-Kung University, Tainan 70101, Taiwan, Republic of China
ABSTRACT
Magnetron dc co-sputtering of a composite target of graphite disk plus iron rods was used in manufacturing carbon films with Fe 3 C nanograin inclusions. Both temperature and field dependent magnetizations, M(T) and M(H), were measured for samples of various carbon concentrations ( from 37% to 85%). M(T) were measured in both conditions of zero field cooling and a field cooling at H = 100 Oe.
Experimental results of χ (T), obtained from M(T), of zero field cooling, were theoretically fitted by using Wolhfarth’s model of non-interacting particles with log-normal distribution function of particle size. Only the films containing pure Fe 3 C grains are well fitted theoretically. Blocking temperature, grain size, and dispersion of grain size distribution are obtained from fitting results. Saturation magnetization, and coercivity are obtained from the results of M(H) measurements. Films, as deposited, are superparamagnetic and show zero room temperature coercivity. The largest room temperature coercivity of 965 Oe is obtained for the sample of 72 at.% C made at the sputtering pressure of 4 mtorr and annealed at the temperature of 550 o C for 60 min.
High-density magnetic recording medium, on the order of 100 Gb/in 2 , is a target that many investigators are striving for. Although many different materials and techniques 1~7 have been proposed to reach the goal, there are common important features existing among these proposals. They are fine magnetic particles/grains on the order of nanometer and well magnetically insulated in order to have high enough density and signal to noise ratio. Besides, due to ultra-fine magnetic particles, thermal stability is especially important. Thus, high coercivity or high magneto-crystalline anisotropy of a material is concerned. Basing on our long-term research on the topic of diamond-like carbon (DLC) films, we chose making Fe-C composite films for the application of high-density recording media. We have succeeded in making pure Fe 3 C nanograins embedded in amorphous carbon films possessing room temperature coercivity of 965 Oe, which is higher than the reported values among other works on Fe-C composites 8~10 .
Amorphous carbon films containing Fe 3 C nanograins were made by sputtering a two-inch diameter graphite target with several pieces of iron rods, 2 mm diameter and 4 mm long, on top of it. Figure 1 shows carbon concentration of films changing with the sputtering pressure and the number of pieces of iron rods. Dashed line in Fig.1, obtained by referring to the results of TEM studies 11 , is used to identify a region of lower pressures and higher carbon concentrations, in which pure Fe 3 C grains are produced.
Temperature dependent magnetizations, M(T), were measured in a field of H =
100 Oe in both conditions of zero field cooling (ZFC) and a field cooling (FC). The
results of χ (T) = M(T)/H of the samples made at a constant pressure of 8.5 mtorr with
carbon concentrations of 42%, 65%, and 85%, respectively, are selected and displayed
in Fig.2. The films with 42 and 65 at.% C contain both Fe and Fe 3 C grains but the
film with 85 at.% C contains only Fe 3 C grains. In Fig.2, all ZFC curves of susceptibilities, χ (T), show an increasing behavior with temperature until a
Zmaximum is reached at T = T B , temporarily called "blocking temperature", after which decreasing with temperature. The susceptibilities of FC curves, χ (T),
FCincrease with decreasing temperature until reaching a maximum. The maximum is maintained in Fig. 2(a) at low temperatures. However, a low temperature minimum appears, additionally, in both χ (T) of Fig. 2(b) and (c), but it is much weaker in (c).
FCAn additional low temperature minimum in χ (T) is observed only in Fig. 2(b). It is
Zalso found that χ (T) deviates from
FCχ (T) at T = T
Zirr ≠ T B as temperature decreases. Both the difference between χ (T) and
Zχ (T) at T
FCirr ≤ T ≤ T B and the temperature range between T irr and T B are getting smaller from Fig. 2(a) to (c) with carbon concentration getting larger. These characteristic behaviors of χ (T) and
Zχ (T) can be understood in the framework of superparamagnetism
FC12 . On considering a system of single domain magnetic particles, relaxation time τ is important in determining how quickly the remanence M r relaxes to its equilibrium value at temperature T. The relaxation time τ is derived and expressed as 12 :
τ -1 = f o exp(-K a V/k B T) (1)
K a is the magnetic anisotropy constant, V the particle volume, k B the Boltzman constant, T the absolute temperature and f o the frequency factor which has a value of 10 9 ~ 10 11 sec -1 . Obviously, the value of τ depends on both V and T. For a typical time of experiment, τ = 100 sec is a reasonable value to mark the transition to a stable behavior. At temperature T, an upper limit of particle volume V m = 29.9k B T/K a is estimated for being superparamagnetic. Because τ < 100 sec for particles with V
< V m , it shows paramagnetism and gives zero coercivity. For particles of constant size
V, there exists a temperature T B = K a V/29.9k B . When T < T B ( τ > 100 sec), paramagnetism disappears and hysteresis appears. T B is thus called blocking temperature. In Fig.2, all curves of χ (T) increase gradually from low temperature to
Za maximum at T = T B indicating a non-constant size of grains existing in the films. T B
is thus more proper to be called "most probable blocking temperature" and V m , calculated from T B , is "most probable maximum grain volume". For simplicity, we still call T B as "blocking temperature" and V m as "maximum grain volume". By assuming the grain as a spherical ball, the maximum grain diameter, D m , is used, instead.
The curve of χ (T) changes with temperature is governed by the grain size
Zdistribution. By fitting χ (T) theoretically, we can obtain anisotropy constant K
Za
together with T B , V m and grain size distribution function f(x), from which the mean grain volume <V>, and thus the mean grain diameter,<D>, can be calculated. A model of Wohlfarth’s non-interacting magnetic particles is adopted in the process of fitting. According to Wohlfarth 13 , we get
xf(x) = (3K a / ε M s 2
ln(2 π f o τ ) -1 ) dT
d ( χ T) (2)
ε the volume fraction occupied by ferromagnetic particles and is approximated as one, M s the saturation magnetization and is obtained separately from M(H) measurements. In fitting the experimental results of
dT
d ( χ T), f(x) was assumed a
log-normal distribution function as f(x) = (1/ 2 π σ x)exp[-
22
2 ) (ln
σ
x ] (3)
x = V/<V> = T B /<T B > and <T B > is the mean blocking temperature; σ , a fitting
parameter which is related with the dispersion of grain size distribution. Eq. (3) is
then used in calculating χ (T)
Z14 of the films with non-constant grains as
χ (T) =
Z< > ∫
( )0 2
) 3 (
T V
B s
m
dx x T xf
k V ε M
+ ∫
∞) ( 2
) 3
a V T(
s
m