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9.3 Time step dependence

The time step dependence of the numerical integration schemes has been investigated by simulating a single rigid magnetic moment. The material parameters were chosen as $M_\mathrm{s}=1281197~\frac{\mathrm{A}}{\mathrm{m}}$, $K_1=6.9\times 10^{6}~\frac{\mathrm{J}}{\mathrm{m^3}}$, $\alpha=0.1$, and $V=1~\mathrm{nm}^3$. The effective field, which is just the anisotropy field, is then given by

\begin{displaymath}
H_\mathrm{ani} = \frac{2 K_1}{\mu_0 M_\mathrm{s}} =
8571~\frac{\mathrm{kA}}{\mathrm{m}} \quad.
\end{displaymath}

For the time for one full precession of the magnetization vector we obtain

\begin{displaymath}
T=\frac{1}{f}=
\frac{2 \pi}{\omega}=
\frac{2 \pi}{\gamma H_\mathrm{ani}}=
3.32~\mathrm{ps}
\quad,
\end{displaymath}

where $\omega=\gamma H$ is the Larmor frequency For the average magnetization in thermal equilibrium we find with ([*])


Temperature $\langle {M_z} \rangle / M_\mathrm{s}$
10 K $0.98979$
50 K $0.94268$
200 K $0.71976$

Figure: Time step dependence of numerical integration schemes
[Average magnetization at 10 K] \includegraphics[scale=0.7]{fig/sim051401.eps}
[ $\langle {M_z^2} \rangle $ at 10 K] \includegraphics[scale=0.7]{fig/sim051401_02.eps}

Figure: Time step dependence at higher temperatures
[Average magnetization at 50 K] \includegraphics[scale=0.7]{fig/sim082105.eps}
[Average magnetization at 200 K] \includegraphics[scale=0.7]{fig/sim082107.eps}

With the Milshtein scheme we find the correct values for time steps smaller than $0.01$ ps, which is about $1/300$ of the precession time. The Heun scheme is also suitable for time steps, which are ten times larger, because it has a higher order of convergence. As a rule, the discretization time step should be at most $1/30$th of the precession time of the magnetization vector in the effective field. This behaviour is verified at higher temperatures of 50 and 200 K. The results shown in figure [*] confirm, that the same rules apply for higher temperatures and therefore larger thermal fluctuations.


next up previous contents
Next: 10. Simulation of fine Up: 9. Rigid magnetic moment Previous: 9.2 Stochastic perturbation   Contents
Werner Scholz 2000-05-16