Figure 3.11 depicts the hysteresis loops obtained from
simulations of a nickel sphere (diameter =200nm,
=0). The
loops in the upper left, upper right and lower left of the figure show
loops yielded with the OOMMF software, whilst the lower right
loop was computed with magpar.
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For each simulation, the applied field direction was varied in and
, respectively the azimuth and polar angle of the applied field.
These are relative to the orientation of the finite difference grid,
aligned with the x-, y- and z-axes.
All the loops show a similar pattern just below saturation, with small openings in the hysteresis where the magnetisation moves from the single domain state into the vortex state.
It is interesting to note that in the loops computed with OOMMF
there is an ``opening'' in the hysteresis loop around =0, the
size of which varies with the direction of the applied field, although
it is never quite eliminated. The results from magpar do not
display this characteristic.
These data show that the inner loop depends on the angles and
. For the spherically symmetric system that we wish to
simulate, how the coordinate system of the simulation software is
aligned relative to the direction of the applied field should be
irrelevant. It is therefore likely that the inner openings in the
hysteresis loops are an artefact of the finite difference simulation
technique as these vary substantially as a function of this direction.
Initially, we assume the applied field is zero and the
magnetisation forms a vortex with the core pointing in the
direction as shown later in figure 3.15, and a very small
field is applied in the opposite direction (i.e.
) such
that the vortex structure of the magnetisation is not significantly
affected. Since the overall magnetic moment of the magnetisation is
finite and points in the direction of the moments in the vortex core,
it is therefore energetically favourable for the system to align the
vortex core with the applied field.
In order for this to happen, the vortex core needs to turn around by
180 degrees (i.e. point in rather than
. If there is
no magnetocrystalline anisotropy in the system, the spherically
symmetric sphere should allow the core to rotate round in either
or
, similar to a typical Stoner-Wohlfarth particle.
The spherical symmetry should not allow the occurrence of the
``inner'' hysteresis loop indicated in figure 3.11; this is
supported by the results presented in the lower right of figure
3.11 computed with the finite element code.
It is plausible therefore to assume that directions along the discretisation axis are either favoured or avoided by the system when a finite difference grid is introduced for symmetric geometries.