Extended Wiener Process in Nonstandard Analysis

Shuya Kanagawa¹, Kiyoyuki Tchizawa²

¹Department of Mathematics, Tokyo City University Setagaya, Tokyo, Japan.
²Institute of Administration Engineering, Ltd., Chiyoda-ku, Tokyo, Japan.

DOI: 10.4236/am.2020.113019                

Abstract

Standing on a different view point from Anderson, we prove that the extended Wiener process defined by Anderson satisfies the definition of the Wiener process in standard analysis, for example the Wiener process at time t obeys the normal distribution N(0,t) by showing the central limit theorem. The essential theory used in the proof is the extended convolution property in nonstandard analysis which is shown by Kanagawa, Nishiyama and Tchizawa (2018). When processing the extension by non-standardization, we have already pointed out that it is needed to proceed the second extension for the convolution, not only to do the first extension for the delta function. In Section 2, we shall introduce again the extended convolution as preliminaries described in our previous paper. In Section 3, we shall provide the extended stochastic process using a hyper number N, and it satisfies the conditions being Wiener process. In Section 4, we shall give a new proof for the non-differentiability in the Wiener process.

Keywords

Wiener Process, Ito’s Process, Stochastic Differential Equation, S-Continuity, Nonstandard Analysis

1. Introduction

Anderson [1] provided stochastic processes in nonstandard analysis to show that for $f\mathrm{<mo>\; :\; </mo>}\Omega \to R$ the following condition (a) is equivalent with (b),

(a) f is Loeb measurable;

(b) there is a measurable function $F\mathrm{<mo>\; :\; </mo>}\Omega \to {}^{\ast }R$ such that

$f\left(\omega \right)\approx F(\omega )$

for almost all $\omega \in \Omega$ (with respect to the Loeb measure ${\mu }_L$ ), where ${}^{\ast }R$ is a lifted space of $R$ constructed from $\omega$ -incomplete ultrafilter.

He proved that the measure on ${}^{\ast }R$ according to the process $W\left(t\right)$ defined by Definition 3.2 satisfies the above condition (b). Therefore, there exists an extended Wiener measure on ${}^{\ast }R$ which is of Loeb measure (Loeb [2], Hurd and Loeb [3]). The existence of the extended Winer measure means that $W\left(t\right)$ is an extended Wiener process in ${}^{\ast }R$ from Kolmogorov’s extension theorem. Benot [4] [5] provided some applications of the extended Wiener measure to the stochastic analysis. Cutland [6] also introduced relevant applications of Loeb measure to the stochastic analysis.

On the other hand, in general, it is not easy to show the existence of the measurable function $F\mathrm{<mo>\; :\; </mo>}\Omega \to {}^{\ast }R$ in (b) for stochastic processes. Therefore, we consider a scheme using extended convolution to show the existence of stochastic processes in ${}^{\ast }R$ without using the above result.

As the main theorem in this paper, we shall provide the extended stochastic process $W\left(t\right)$ described newly in ${}^{\ast }R$. It satisfies the conditions being the Wiener process in nonstandard analysis. It will be proved in Section 3.

The extended Wiener process can be applied to construct some physical models, for example quantum mechanics, using the $\omega$ -incomplete ultrafilter. We consider that our observation is done through the ultrafilter, since the nature is originally described by nonstandard numbers. Because of the above reasons, we need a nonstandard analysis for the convolution by the hyperfunction.

2. Nonstandard Convolution by Hyperfunction

Let $\mathcal{F}$ be the space of all locally integrable functions on $R$. Define the space of all rapidly decreasing $C^{\infty }$ functions $\mathcal{S}$ by

$\underset{x\in R}{sup}\left|x^m{f}^{\left(k\right)}\left(x\right)\right|<\infty$

for any $m\mathrm{,}k\in Z_{+}$. Furthermore define the space of all slowly increasing functions $\mathcal{O}$ by for any $k\in Z_{+}$ there exist some positive constants $C_k$ and $M_k\in Z_{+}$ such that

$\left|f^{\left(k\right)}\left(x\right)\right|<C_k{\left(1+\left|x\right|\right)}^{M_k}.$

$f\in \mathcal{F}$ is Lebesgue integrable on any compact set K such that

$-\infty <{\displaystyle {\int }_K}f\left(x\right)\text{d}x<\infty$

For $f\in C^{\infty }$ there exists continuous k-th derivative $f^{\left(k\right)}\left(x\right)$ for each $k\ge 1$.

For $f\in S\subset C^{\infty }$

$\underset{x\in R}{sup}\left|x^m{f}^{\left(k\right)}\left(x\right)\right|<\infty$

holds for each $k\mathrm{,}m\in Z_{+}$, where $Z_{+}$ means the space of all positive integers.

From the above description, we can easily obtain that

$S\subset \mathcal{O}\subset C^{\infty }\subset F$

For $f\mathrm{,}g\in S$, the convolution of f and g is defined by

$f\ast g\left(x\right)={\displaystyle {\int }_{-\infty }^{\infty }}f\left(s\right)g\left(x-s\right)\text{d}s$

The definition of the convolution can be extended to the k-th convolution by

$f_1\ast f_2\ast \cdots \ast f_k\left(x\right)={\displaystyle {\int }_{-\infty }^{\infty }}\left(f_1\ast \cdots \ast f_{k-1}\right)\left(s\right)f_k\left(x-s\right)\text{d}s$

for each $k\in Z_{+}$.

From the above definitions, we can easily obtain the next result.

Proposition 1.

1) $f\ast g\left(x\right)=g\ast f(x)$

2) $f\ast \left(g+h\right)\left(x\right)=g\ast f\left(x\right)+g\ast h(x)$

3) $\text{supp}\left(f\ast g\right)\subseteq \text{supp}\left(f\right)\cup \text{supp}(g)$

Proposition 2. For $\phi \mathrm{,}\psi \in S$

1) $\phi \psi \in S$

2) $\phi \ast \psi \in S$

3) ${\left(\phi \ast \psi \right)}^{\left(k\right)}\left(x\right)={\phi }^{\left(k\right)}\ast \psi \left(x\right)=\phi \ast {\psi }^{\left(k\right)}(x)$

Let $\tilde{H}$ be the set of rapidly decreasing functions satisfying

1) $f\left(-x\right)=f(x)$

2) ${\displaystyle {\int }_{-\infty }^{\infty }}f\left(x\right)\text{d}x=1$

Define a function $\bar{f}\left(t\right)$ by

$\bar{f}\left(t\right)\left(x\right)=\frac{1}{t}f\left(\frac{x}{t}\right),t\in \left(0,1\right]$

Proposition 3.

1) $f\in \tilde{H}\Rightarrow \bar{f}\left(t\right)\in \tilde{H}$

2) $f\mathrm{,}g\in \tilde{H}\Rightarrow f\ast g\in \tilde{H}$

Example 2.1. Figure 1 gives a typical example of hyperfunction at around the origin.

3. Extended Wiener Process in Nonstandard Analysis

Why does the extended stochastic process in Definition 3.2 satisfy the conditions

Figure 1. $N\left(\mathrm{0,}{\sigma }^2\right)$, $\sigma =6/10$, $\sigma =3/10$, hyperfunction $\sigma =1/N，N\in \text{*NN}$.

being Wiener process? First, let us show the definition of the extended Wiener process according to Anderson [1] [7].

Definition 3.1. For fixed $N\in \text{*NN}$, put $\Delta t=N^{-1}$. The hyperfinite time line $T$ based on $\Delta t$ for the interval $\left[\mathrm{0,}T\right]$ is the set defined by

$T=\left\{\mathrm{0,}\Delta t\mathrm{,2}\Delta t\mathrm{,}\cdots \mathrm{,}T-\Delta t\mathrm{,}T\right\}\mathrm{,}$

for some $T>0$.

Definition 3.2. Assume that a sequence of i.i.d. random variables $\left\{\Delta W_k,k=1,\cdots ,NT\right\}$ has the distribution

$P\left\{\Delta W_k=\sqrt{\Delta t}\right\}=P\left\{\Delta W_k=-\sqrt{\Delta t}\right\}=\frac{1}{2},$

for each $k=\mathrm{1,}\cdots \mathrm{,}NT$. An extended stochastic process $\left\{W\left(t\right)\mathrm{,}t\in T\right\}$ is defined by

$W\left(t\right)={\displaystyle \underset{k=1}{\overset{Nt}{\sum }}}\Delta W_k,t\in T.$ (1)

We shall prove that the extended process $W\left(t\right)$ satisfies the following conditions being Wiener process.

Definition 3.3. If the process $W\left(t\right)$ satisfies the following conditions, then $W\left(t\right)$ is called the Wiener process.

1) $W\left(0\right)=0$. a.s.

2) $W\left(t\right)$ is a continuous function with probability 1.

3) $W\left(t\right)$ has stationary, independent increments.

4) The increment $W\left(t+s\right)-W\left(s\right)$ has the normal distribution $N\left(\mathrm{0,}t\right)$ for any $s\mathrm{,}t\ge 0$.

Theorem 3.4. The extended process $W\left(t\right)$ satisfies the conditions in Definition 3.3.

Proof)

Now, we go back the distribution of $W\left(t\right)$. From the nonstandardization of the convolution in the previous section, we calculate the characteristic function (Fourier transform) of $W\left(t\right)$.

$P\left\{W\left(t\right)\le x\right\}=P\left\{{\displaystyle \underset{k=1}{\overset{Nt}{\sum }}}\Delta W_k\le x\right\}={\displaystyle {\int }_{-\infty }^x}f\ast \cdots \ast f\left(u\right)\text{d}u,$

where $f\left(u\right)$ is the density function of $\Delta W_k$.

$\begin{array}{c}E\left[{\text{e}}^{i\theta W\left(t\right)}\right]=E\left[{\text{e}}^{i\theta {\displaystyle \underset{k=1}{\overset{Nt}{\sum }}\Delta W_k}}\right]={\displaystyle {\int }_{-\infty }^{\infty }}{\text{e}}^{i\theta u}f\ast \cdots \ast f\left(u\right)\text{d}u\\ ={\displaystyle \underset{k=1}{\overset{Nt}{\prod }}{\displaystyle {\int }_{-\infty }^{\infty }}{\text{e}}^{i\theta u}f\left(u\right)\text{d}u}={\displaystyle \underset{k=1}{\overset{Nt}{\prod }}E\left[{\text{e}}^{i\theta \Delta W_k}\right]}\\ ={\displaystyle \underset{k=1}{\overset{Nt}{\prod }}\frac{1}{2}\left\{{\text{e}}^{-i\theta \sqrt{\Delta t}}+{\text{e}}^{i\theta \sqrt{\Delta t}}\right\}}={\displaystyle \underset{k=1}{\overset{Nt}{\prod }}\cos \left(\theta \sqrt{\Delta t}\right)}\\ ={\left(\cos \frac{\theta }{\sqrt{N}}\right)}^{Nt}={\text{e}}^{\frac{t{\theta }^2}{2}}.\end{array}$ (2)

Note that, in standard analysis, the last term in (2) is shown by the following equation,

$\begin{array}{c}{\left(\cos \frac{\theta }{\sqrt{N}}\right)}^{Nt}=\underset{n\to \infty }{lim}{\left(\cos \frac{\theta }{\sqrt{n}}\right)}^{nt}=\underset{n\to \infty }{lim}{\left\{1-\frac{{\theta }^2}{2!n}+\frac{{\theta }^4}{4!n^2}-\cdots \right\}}^{nt}\\ =\underset{n\to \infty }{lim}{\left\{1-\frac{{\theta }^2}{2!n}+\frac{{\theta }^4}{4!n^2}-\cdots \right\}}^{nt}\\ =\underset{n\to \infty }{lim}{\left\{1-\frac{{\theta }^2}{2!n}+\frac{{\theta }^4}{4!n^2}-\cdots \right\}}^{nt}\\ =\underset{n\to \infty }{lim}{\left\{{\left(1-\frac{{\theta }^2}{2n}\right)}^{\frac{2n}{{\theta }^2}}\right\}}^{\frac{t{\theta }^2}{2}}={\text{e}}^{\frac{t{\theta }^2}{2}}.\end{array}$

Therefore, $W\left(t\right)$ obeys the normal distribution $N\left(\mathrm{0,}t\right)$. Furthermore, it is easy to prove that $W\left(t\right)$ has the stationary and independent increments from the Definition 3.2. Then, we can show that $W\left(t\right)$ satisfies all conditions of the Wiener process.

4. Proof of the Non-Differentiability of Wiener Process

In this section, we give the proof that the Wiener process has the property of non-differentiability. It is well known that Wiener process in standard analysis is non-differentiable a.s. though. The proof of the non-differentiability was shown by Dvoretski, Erdös and Kakutani [8]. (See e.g. Theorem 12.25 in Breiman [9].) On the other hand, the law of the iterated logarithm holds for the extended Wiener process as following (3) and (4). As to the law of the iterated logarithm in standard analysis, see e.g. Karatzas and Shreve [10], the Section 2.9. The original proof for i.i.d. random variables is due to Khintchine [11].

Theorem 4.1. Every sample path of Wiener process defined by

$W\left(t\right)={\displaystyle \underset{k=1}{\overset{Nt}{\sum }}}\Delta W_k,t\in {\rm T},$

has the non-differentiability.

Proof)

$\underset{N\in \text{*NN}}{\sup }\frac{W\left(1/\sqrt{N}\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log \left(\sqrt{N}\right)}}=1,a.s.$ (3)

and

$\underset{N\in \text{*NN}}{\inf }\frac{W\left(1/\sqrt{N}\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log \left(\sqrt{N}\right)}}=-1,a.s.$ (4)

Since $W\left(t+s\right)-W\left(t\right)$ is also a Wiener process for some $t\in {\rm T}$ and any $s\in {\rm T}$,

$\underset{N\in \text{*NN}}{\sup }\frac{W\left(t+1/\sqrt{N}\right)-W\left(t\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log \left(\sqrt{N}\right)}}=1,a.s.$ (5)

and

$\underset{N\in \text{*NN}}{\inf }\frac{W\left(t+1/\sqrt{N}\right)-W\left(t\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log \left(\sqrt{N}\right)}}=-1,a.s.$ (6)

for any $t>0$. Therefore

$\underset{N\in \text{*NN}}{\sup }\frac{W\left(t+1/\sqrt{N}\right)-W\left(t\right)}{\sqrt{1/\sqrt{N}}}>\sqrt{2\log \log \left(\sqrt{N}\right)},a.s.$ (7)

and

$\underset{N\in \text{*NN}}{\inf }\frac{W\left(t+1/\sqrt{N}\right)-W\left(t\right)}{\sqrt{1/\sqrt{N}}}<-\sqrt{2\log \log \left(\sqrt{N}\right)},a.s.$ (8)

(7) and (8) imply the non-differentiability of the sample path of Wiener process.

Remark 1. From Definition 3.1 for the extended Wiener process, we have

$\frac{W\left(1/N\right)}{\sqrt{2\left(1/N\right)\log \log \left(N\right)}}=\frac{\Delta W_1}{\sqrt{2\left(1/N\right)\log \log \left(N\right)}}=\{\begin{array}{l}\frac{1}{\sqrt{2\log \log \left(N\right)}}\hfill \\ \frac{-1}{\sqrt{2\log \log \left(N\right)}}.\hfill \end{array}$

Thus the law of the iterated logarithm does not hold for

$\frac{W\left(1/N\right)}{\sqrt{2\left(1/N\right)\log \log \left(N\right)}}.$

Notice that

$\frac{W\left(1/\sqrt{N}\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log (N)}}$

is defined on the hyperfinite line

$\sqrt{T}=\left[0,\Delta t,2\Delta t,3\Delta t,\cdots ,\left(N/\sqrt{N}\right)\Delta t\right].$

Therefore,

$\underset{N\in \text{*NN}}{\sup }\frac{W\left(1/\sqrt{N}\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log (N)}}$

and

$\underset{N\in \text{*NN}}{\inf }\frac{W\left(1/\sqrt{N}\right)}{\sqrt{2\left(1/\sqrt{N}\right)\log \log (N)}}$

exist and the law of the iterated logarithm (3) and (4) hold on the hyperfinite line $\sqrt{T}$.

Remark 2. From Definition 3.2 the Wiener process $W\left(t\right)$ is defined by the sum of i.i.d. random variables $\left\{\Delta W_k,k=1,\cdots ,NT\right\}$. Therefore, we can prove the non-differentiability of Wiener process by the law of the iterated logarithm (3) and (4). Since the above proof in the sense of nonstandard analysis cannot be translated to the proof in standard analysis, another proof using standard one in [8] is needed to show the non-differentiability. This is a typical example of the advantage of the extended Wiener process.

5. Conclusion

Anderson [1] showed that the process $W\left(t\right)$ defined by Definition 3.2 satisfies the conditions (1)-(4) in Definition 3.3 of Wiener process from the equivalence of (a) and (b) due to Loeb [2]. On the other hand, we showed the extended Wiener process for $W\left(t\right)$ satisfies the conditions (1)-(4) directly by the nonstandardization of the convolution. When we extend the time space and obtain extended Wiener process, the nonstandard number N is efficient enough to describe the precise structure. It is also reminded that the N is applied to “extended Wiener measure” described in [12] [13]. The hyperfinite time line $T$ is a key word. Notice that the delta function is described by the normal distribution in this state. Furthermore, we provided a new proof of the non-differentiability on the Wiener process using the extended law of the iterated logarithm for the Wiener process in nonstandard analysis.

Supported

The first author is supported in part by Grant-in-Aid Scientific Research (C), No. 18K03431, Ministry of Education, Science and Culture, Japan.

Symbols

$\Omega$ : probability space

$R$ : real numbers

${}^{\ast }R$ : hyper real numbers

$\mathcal{F}$ : space of all locally integrable functions on $R$

$\mathcal{S}$ : space of all rapidly decreasing functions

$Z_{+}$ : positive natural numbers

$\mathcal{O}$ : space of all slowly increasing functions

$N$ : hyper number

$N^{-1}$ : infinitesimal

$N$ : natural numbers

${}^{\ast }N$ : hyper natural numbers

$T$ : hyperfinite time line

Conflicts of Interest

The authors declare no conflicts of interest regarding the publication of this paper.

References

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