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Martingale drift of Langevin dynamics and classical canonical spin statistics

Ken Sekimoto

Abstract

The martingale characterizes a kind of fairness or unbiased nature of the stochastic process which is associated with another stochastic process. If $x_t$ evolves according to the Langevin equation whose mean drift is $a_t$ as function of $x_t,$ and that $a_t$ as induced stochastic process is martingale in turn associated with the former process, then we show that the amplitude of $a_t$ is the Langevin function, which is originally the canonical response of a single classical Heisenberg spin under static field. Furthermore, the asymptotic limit of $x_t/t$ obeys the ensemble statistics of such Heisenberg spin.

Martingale drift of Langevin dynamics and classical canonical spin statistics

Abstract

The martingale characterizes a kind of fairness or unbiased nature of the stochastic process which is associated with another stochastic process. If evolves according to the Langevin equation whose mean drift is as function of and that as induced stochastic process is martingale in turn associated with the former process, then we show that the amplitude of is the Langevin function, which is originally the canonical response of a single classical Heisenberg spin under static field. Furthermore, the asymptotic limit of obeys the ensemble statistics of such Heisenberg spin.
Paper Structure (9 sections, 33 equations, 3 figures)

This paper contains 9 sections, 33 equations, 3 figures.

Figures (3)

  • Figure 1: 2D trajectories from ${\vec{x}}_0=(0_+,0_+).$ (Left) Close-up view near the origin. (Right) Whole trajectories up to $t=16.$
  • Figure 2: 2D trajectories from ${\vec{x}}_0=(x_0,0_+)$ with (a) $x_0=0$, (b) $x_0=1$, (c) $x_0=2$ and (d) $x_0=4.$ In all cases the duration is up to $t=40$ and we used the identical set of noise histories for $\vec{\xi}_t$ in (\ref{['eq:eqL']})
  • Figure 3: The 2D orientational distributions of $\lim_{t\to\infty}({{\vec{x}}_t}/{t})={\vec{a} } ^{\,*}_\infty$ for the different starting points, $x_0=0,1,2,$ and $4,$ from top to bottom. We represent the orientation of ${\vec{a} } ^{\,*}_\infty$ using $\cos\theta,$ where $\theta$ is the angle between ${\vec{a} } ^{\,*}_\infty$ and ${\vec{x}}_0=(x_0,0),$ and we show the distributions by the empirical cumulative probability. Numerically the ensemble of ${\vec{a} } ^{\,*}_\infty$ is approximated by 3000 realisations of ${\vec{x}}_t/t|_{t=40}.$ The red dashed curves represent the canonical equilibrium distribution of a single unitary spin under the non-dimensionalized field ${\vec{x}}_0,$ see (\ref{['eq:cancumul']}) in the main text.