Stock
Price Process
and
Statistical
Mechanics
日本大学. 文理学部 黒田 耕嗣 (Koji Kuroda)
Dept. of Math., College ofHunanities and Sciences,
Nihon University
Abstract
Amodel ofan auction for astock market isintroduced to derive adiscrete timestock
price process. Aprobability distribution of trader’s positions configuration is given by
aGibbs distribution in which trading strategies of traders and an effect from market
sentiments are contained. To derive ascaling limit the method of statistical mechanics
is applied to thisprocess , and avolatility function and adrift function
are
described interms ofpolymer weight functions.
Keywords: Auction$\mathrm{m}\mathrm{o}\mathrm{d}\mathrm{e}\mathrm{l},\mathrm{G}\mathrm{i}\mathrm{b}\mathrm{b}\mathrm{s}$ distribution, Stockpriceprocess, Polymer expansion
1Introduction
To describe astock priceprocess manystochasticprocessessuch
as
BlackSholesmodel[l],ICR model [2] and Vasicek model [9] are investigated, particularly in an option price
theory.
In thisarticle
we
introducean
auction model for astock marketcomposedof$\mathrm{N}$ tradersand asingle stock. We derive adiscrete time stochastic process describing astock price
process from this auction model, in which each trader
can
trade unit number of stocks at数理解析研究所講究録 1337 巻 2003 年 191-204
each time $t\in\Lambda_{n}=\{1,2, \cdots, n\}$
.
It is also assumedthat each tradercan
takeone
ofthefollowing three positions, buying position, selling position and neutral position at each
time $t\in\Lambda_{n}=\{1,2, \cdots, n\}$.
Probability distribution for trader’s positions is given by aGibbs measure, in which
tradingstrategies of traders and
an
effect from market sentimentsare
contained. Gibbsmeasures
isintroducedbyDobrushin [4], LanfordandRuelle [8] toinvestigateastatisticalmechanics from mathematicalpoint of view. It is characterized byan interaction energy.
In
our
model this interactionenergy is determined from trading strategies of traders andmarket sentiments.
Applyingamethod ofpolymer expansion developed in atheoryof statis tical
mechan-ics $[3],[6]$
we
derive acontinuous time stock priceprocess,
$S_{t}=S_{0} \exp\{\int_{0}^{t}\sigma(s)dB(s)+\int_{0}^{t}\mu(s)ds\}$by scaling the discretetime process, where $B(t)$ is astandard Brownian motion.
The function $\sigma(s)$ is called avolatility function which describes the strength of the
variation of the stock price, and the function$\mu(s)$ is calledadrift functionwhichdescribes
the trend of the stock price process.
We describe these functions in terms of polymer weight functions defined by the
in-teraction
energies whichdetermined
by trading strategiesand
marketsentiments.
2Model
As stated in the introduction each trader
can
takeone
of the following three positions,buying positiondenoted$\mathrm{b}\mathrm{y}+$, selling positiondenotedby -and neutral position denoted
by 0.
Denote apositions configuration of$\mathrm{N}$ traders at time$t\in\Lambda_{n}$ by
$\omega_{t}=(\omega_{t}(1), \omega_{t}(2),$$\cdots,\omega_{t}(N))$
asequence of positions configuration from time 0to $n-1$ by
$\omega$$=(\omega_{0}, \cdots,\omega_{n-1})$
.
and the totality of$\omega$ by $\Omega_{n}$
.
For any $\omega_{t}$ the number of traders with buying position, selling position, and neutral
position are denoted by$\omega_{t}^{+}$, $\omega_{t}^{-}$ and $\omega_{t}^{0}$ respectively. The number of market participants
is given by $\omega_{t}^{+}+\omega_{t}^{-}$
.
We introduce anotion of modified number of market participantsby
$|\omega_{t}|=\{$
$\omega_{t}^{+}-\omega_{t}^{-}-d_{0}$ if$\omega_{t}$ is active
0otherwise
where $d_{0}$ is apositive constant.
We say$\omega_{t}$(or time $t$) is active if $|\omega_{t}|>0$ and static if $|\omega_{t}|=0$
.
We also put
$<\omega_{1}>=\{$
($v_{t}^{+}-\omega_{t}^{-}-d_{0}$ if$\omega_{t}^{+}-\omega_{t}^{-}>d_{0}$
0if $|\omega_{t}^{+}-\omega_{t}^{-}|\leq d_{0}$
$-(\omega_{t}^{-}\omega_{t}^{+}-d_{0})$ if$\omega_{t}^{-}-\omega_{t}^{+}>d_{0}$
If $<\{v_{t-1}>>0(<0)$, then the number of traders with buying (selling) position is
greater than the number of traders withselling(buying) positionandthestock pricegoes
(down) at time $t$
.
Let $S_{t}$ be astock price at time $t$.
When $\omega$ is givenwe
define thestock priceprocess from $\omega$ by
$\frac{S_{t}}{S_{t-1}}=e^{\alpha<\mathrm{I}v_{t-1}>}$ .
It is easily
seen
that$S_{t}=S_{0} \exp\{\sum_{u=0}^{t-1}<\omega_{u}>\}$.
Gibbs
measure
We introduceaGibbs
measure
as
aprobability distribution of positions configuration$\omega$
.
First
we
definean
interactionenergy
$H(\omega)$ by$H( \omega)=\beta_{1}\sum_{t=0}^{n-1}|\omega_{t}|^{2}+\beta_{2}\sum_{t=0}^{n-1}\Phi(\omega_{t}|\omega_{t-a}, \cdots,\omega_{t-1})$
$- \beta_{3}\sum_{t=0}^{n-1}c(t)f_{1}(|\omega|_{t,a})|\omega_{t}|-\beta_{4}\sum_{t=0}^{n-1}d(t)f_{2}(<\omega>_{t,a})<\omega_{t}>$
where $\beta_{1}$,$\beta_{2}$,$\beta_{3}$, and $\beta_{4}$ are positive numbers which control the strength of interactions
and $c(t)$ and $d(t)$
are
positive functions defined on $\Lambda_{n}$.Nowwe define aGibbs distribution of$\omega$ by
$P_{n}( \omega)=\frac{1}{Z_{n}}\exp\{-H(\omega)\}$,
where $Z_{n}$ is anormalizationconstant called apartition function.
For this Gibbs distribution , the probability $P(\omega)$ is high(low) if the energy $H(\omega)$ is
low(high).
The first term of $H(\omega)$ is aterm controling the number of market participants. The
second term corresponds to trading strategies of$N$ traders and it is assumed that
(A-1) $\Phi(\omega_{t}|\omega_{t-a}, \cdots, \omega_{t-1})=0$ if$\omega_{t}$ is static
(A-2) $\Phi(\overline{\omega}_{t}|\overline{\omega}_{t-a}, \cdots,\overline{\omega}_{t-1})=\Phi(\omega_{t}|\omega_{t-a}, \cdots,\omega_{t-1})$
(A-3) $\Phi(\omega_{t}|\omega_{t-a}, \cdots,\omega_{t-1})>-c|\omega_{t}|$
where $\overline{\omega}_{t}$ is areflectionimage of$\omega_{t}$ defined by $\overline{\omega}_{t}=-\omega_{t}$
.
Traders lookat ahistory $(\omega_{t-a}, \cdots, \omega_{t-1})$ ofpositions configurations and determine
a
present position$\omega_{t}$
.
The third term describes
an
effect on the market from atotal number of marketparticipants from time $t-a$ to $t-1$ and $|\omega|_{t,a}$is given by $|\omega|_{t,a}=|\omega_{t-a}|+\cdots+|\omega_{t-1}|$
.
If$f_{1}(|\omega|_{t,a})>0$, this term worksfor increasing anumber ofmarket participants.
We
assume
that $f_{1}(x)\leq c_{1}x$ $(x>0)$ forsome
$c_{1}>0$.
The firth term describes
an
effecton
the market from achenge of stock price fromtime $t-a$ to $t-1$ and $<\omega>_{t,a}$ is given by $<\omega>_{t,a}=<\omega_{t-a}>+\cdots+<\omega_{t-1}>$. We
assume
that(1) $f_{2}(x)\leq c_{2}|x|$
(2) $f_{2}(0)=0$
(3) $f_{2}(x)+\mathrm{f}2(\mathrm{x})\geq 0$ for all $x\in \mathrm{R}$
(4) $f_{2}(x)+f_{2}(-x)>\epsilon_{1}$ unless $|x-b_{3}|<\delta_{0}$ or $|x+b_{3}|<\delta_{0}$ or $|x|<\delta_{0}$ for some
$\epsilon_{1}>0$,$b_{3}>0$,$\delta_{0}>0$
.
If $f_{2}(<\omega>_{t,a})>0$, this term works for increasing anumber oftraders with buying
positions
3Method
of
cluster expansion
The method of polymer expansion has been developed by mainly Gallavotti[6], and Del
GrOssO[3], for rigorous investigationsof phase transitions in lattice spin systems. (See also
Phister[5] for anice summary of this method.)
In this section
we
summarizeamethod of polymer expansionto stateour
results.For agiven configuration $\omega$
we
denote by $\{t_{1}, \cdots, t_{k}\}$ aset of all active times. Decompose aset
$\alpha(t_{1})\cup\alpha(t_{2})\cup\cdots\cup\alpha(t_{k})$
into aset of connected components $W_{1}$,$\cdots$ ,$W_{m}$, where $\alpha(t_{i})=\{t_{i}-a, \cdots, t_{:}-1\}$
.
Wecallacouple$\xi^{i}$of$W_{\mathrm{i}}=\{t_{f}, \cdots, t_{q}\}$ and the configuration $\{\omega_{t_{f}}, \cdots,\omega_{t_{q}}\}$
on
$W_{\dot{1}}$acluster’and denote it by
$\xi^{\dot{1}}$ $=$ $(\begin{array}{lll}\omega_{f} \cdots \omega_{q}f \cdots q\end{array})$
For any cluster $\xi^{:}$ given in (3.1) put
$p(\xi^{\dot{1}})=\{f, \cdots, q\}$
.
When aconfiguration $\omega\in\Omega_{n}$ is given , afamilyofclusters $\{\xi^{1}, \cdots, \xi^{m}\}$ is determined
uniquely, but this correspondence is not one-t0-0ne.
Todefine probability distributionof$\{\xi^{1}, \cdots,\xi^{m}\}$wefirst introduceaset$A(\xi^{1}, \cdots,\xi^{m})$
by
$A(\xi^{1}, \cdots,\xi^{m})=$
{
$\omega\in\Omega_{n};\{\xi^{1}$,$\cdots$ ,$\xi^{m}\}$ is obtained from $\omega$as
aset of clusters}.
Then aprobability distribution $P(\xi^{1}, \cdots, \xi^{m})$ for aset ofclusters is defined by
$P( \xi^{1}, \cdots , \xi^{m})=\sum_{\omega\in A(\xi^{1},\cdots t^{m})}P(\omega)$.
It follows from the definition of interaction energies that the
occurrence
of clustersbecomes independent and
$P( \xi^{1}, \cdots,\xi^{m})=\prod_{\dot{\iota}=1}^{m}\mathcal{W}(\xi^{i})$
$,\mathrm{w}\mathrm{h}\mathrm{e}\mathrm{r}\mathrm{e}\mathcal{W}(\xi)$ is given by
$\mathcal{W}(\xi)=e^{-|\mathrm{p}(\xi)|\log m\mathrm{o}}\prod_{t\in\hat{p}(\xi)}\exp\{-\beta_{1}|\xi_{t}|^{2}-\beta_{2}\Phi(\xi_{t}|\xi_{t-a}, \cdots, \xi_{t-1})$
$+\beta_{3}c(t)f_{1}(|\xi|_{t,a})|\xi_{t}|+\beta_{4}d(t)f_{2}(<\xi>_{t,a})<\xi_{t}>\}$
Algebraic formalism of cluster expansion
Let $\not\subset$ be aset of all clusters in $\mathrm{Z}$, and 2be aset of mappings given by
$\mathfrak{U}=\{A : C arrow \mathrm{N};|A|<\infty\}$,
where
$|A|= \sum_{\xi\in \mathrm{C}}A(\xi)$
.
Each $A\in \mathfrak{U}$ stands for aconfiguraion of finite number of clusters with multiplicity.
Furthermore,
we
define afunctional space $L$ by$L$ $=$
{
$\varphi:\mathfrak{U}arrow \mathrm{R};\sup_{|A|=n}|\varphi(A)<\infty$for any $n$}.
For any $\varphi_{1}$,$\varphi_{2}\in L$ define aproduct $\varphi_{1}*\varphi_{2}$ by
$\varphi_{1}*\varphi_{2}(A)=\sum_{A_{1}+A_{2}=A}\frac{A!}{A_{1}!}A_{2}!\varphi_{1}(A_{1})\varphi_{2}(A_{2})$
where the
sum runs over
all ordered pairs ($A_{1}$,A2) such that $A_{1}+A_{2}=A$.
It is easily
seen
that$\varphi_{1}*(\varphi_{2}*\varphi_{3})=(\varphi_{1}*\varphi_{2})*\varphi_{3}$
.
This functional space $L$becomes acommutative algebra with aunit element 1given
by
$1(A)=\{$1if
$A=\emptyset$
0otherwise.
Wedefine subspaces
!and
$L_{1}$ given bya
$=\{\varphi\in \mathrm{i}2;\varphi(\emptyset)=0\}$, $L_{1}=\{\varphi\in L; \varphi(\emptyset)=1\}$,and amapping$\mathrm{E}\mathrm{x}\mathrm{p}:h$ $arrow L_{1}$ by
$\mathrm{E}\mathrm{x}\mathrm{p}\varphi(A)=\sum_{k=0}^{\infty}\frac{1}{k!}\varphi*\cdots*\varphi(A)$
.
As
an
inverse mapping of$\mathrm{E}\mathrm{x}\mathrm{p}$ we define amapping$\mathrm{L}\mathrm{o}\mathrm{g}:L_{1}arrow \mathcal{L}_{0}$ by${\rm Log} \varphi(A)=\sum_{k=1}^{\infty}\frac{(-1)^{k+1}}{k!}\varphi_{0}*\cdots\varphi_{0}(A)$
where
$\varphi_{0}=\varphi-1$
.
Then
we
have the followig relation between two mappings${\rm Log}(\mathrm{E}\mathrm{x}\mathrm{p}\varphi)=\varphi$ for any $\varphi\in L_{0}$
$\mathrm{E}\mathrm{x}\mathrm{p}({\rm Log}\varphi)=\varphi$ for any $\varphi\in L_{1}$.
We say $\chi\in L$ is multiplicative if
$\chi(A_{1}+A_{2})=\mathrm{x}(\mathrm{A}\mathrm{i})\cdot\chi(A_{2})\mathrm{f}\mathrm{o}\mathrm{r}$any$A_{1}$,$A_{2}\in \mathfrak{U}$.
The following Lemma is afundamental Lemma for cluster expansion.
Lemma 3.2([3])
If$\chi$ is multiplicative and
$\sum_{A\in \mathfrak{U}}\frac{{\rm Log}\varphi(A)\chi(A)}{A!}<\infty$
then
$\sum_{A\in \mathfrak{U}}\frac{|\varphi(A)\chi(A)|}{A!}<\infty$
and
$\sum_{A\in\alpha}\frac{\varphi(A)\chi(A)}{A!}=\exp\{\sum_{A\in \mathfrak{U}}\frac{{\rm Log}\varphi(A)\chi(A)}{A!}\}$
.
Application of cluster expansion to the probability distribution of clusters
Now
we
applythe method of cluster expansion to the probability distribution$P(\xi_{1}, \cdots,\xi_{m})$ and derive ascaling limit of$W_{t}(\cdot)$
.
First
we
define functionals $\phi_{0}(\xi)$,$\phi_{1}(\xi)$,$\phi_{2}(\xi)$ by$\phi_{0}(\xi)=\exp\{-\beta_{1}|\xi|^{2}-\beta_{2}\Phi(\xi_{t}|\xi_{t-a}, \cdots,\xi_{t-1})-\log m_{0}|p(\xi)|\}$
$\phi_{1}(\xi)=\exp\{\beta_{3}\sum_{t\in \mathrm{p}(\xi)}c(t)f_{1}(|\xi|_{t,a}>)|\xi_{t}|\}$
$\phi_{2}(\xi)=\exp\{\beta_{4}\sum_{t\in p(\xi)}d(t)f_{2}(<\xi>_{t,a})<\xi_{t}>\}$
and
we
define $\phi_{0}(A),\phi_{1}(A)$,$\phi_{2}(A)$,$\alpha(A)$ by$\phi_{0}(A)=\prod_{\xi\in \mathrm{C}}\phi_{0}(\xi)^{A(\xi)}$ $\phi_{1}(A)=\prod_{\xi\in \mathrm{C}}\phi_{1}(\xi)^{A(\xi)}$ $\phi_{2}(A)=\prod_{\xi\in \mathrm{C}}\phi_{1}(\xi)^{A(\xi)}$
$\alpha(A)=\{$1if
$A!=1,p(\xi^{i})\cap p(\xi^{j})=\emptyset$ for all $\xi^{\dot{\iota}}\neq\xi^{j}\in \mathrm{s}\mathrm{u}\mathrm{p}\mathrm{p}A$
0otherwise.
Also we put
$<A>= \sum_{\xi\in C}<\xi>A(\xi)$
$f_{1}(A)= \beta_{3}\sum_{\xi\in C}\sum_{t\in \mathrm{p}(\xi)}c(t)f_{1}(|\xi_{0}|_{t,a})|\xi_{t}|A(\xi)$
$f_{2}(A)= \beta_{4}\sum_{\xi\in C}\sum_{t\in \mathrm{p}(\xi)}d(t)f_{2}(<\xi>_{t,a})<\xi_{t}>A(\xi)$,
and define arefletion image$\overline{A}$ of$A$ by$\overline{A}(\xi)=A(\overline{\xi})$.
The following Lemma is obtained in the similar way developed in $\mathrm{I}$
.
Lemma 3.3
For any $\beta_{2}>0$ and $\beta_{3}>0$ we have
$\sum_{\xi\in \mathrm{C}_{j}O\in p(\xi)}W(\xi)<1$
for sufficiently large $\beta_{1}>0$
.
Put
$\beta_{1}=\inf\{\beta_{1}>0;\sum_{\xi\ni 0}\exp\{-\beta_{1}|\xi|^{2}-c_{3}|\xi|)+\log m_{0}|p(\xi)|\}<1\}<\infty$
.
For any $A\in A$
we
call $A$ apolymer if$\cup\xi Ap(\xi)$
isconnected.
Lemma 3.4
$\alpha^{T}(A)=0$ unless $A$is apolymer.
Lemma 3.5
(1) If$\beta_{1}>\beta_{0}$, then wehave
$\sum_{A\ni 0}\frac{\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)}{A!}|\alpha^{T}(A)|\geq g(\beta_{1})$
where $\alpha^{T}(A)=\log\alpha(A)$ and $g(\beta_{1})arrow 0$
as
$narrow\infty$.(2) For any $0<c<1$
we
have$\sum_{A\ni 0,|A|^{2}\geq k}\frac{\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)}{A!}|\alpha^{T}(A)|\geq g((1-c)\beta_{1})e^{-\mathrm{c}\beta_{1}k}$
if $(1-c)\beta_{1}>h$, where
$|A|^{2}= \sum|\xi|^{2}A(\xi)$
.
$\xi$
As $\phi_{0}(A)$,$\phi_{1}(A)$ and $\phi_{2}(A)$ are multiplicative, by applying the method of cluster
ex-pansion wehave
$Z_{n}= \exp\{\sum_{A\subset\Lambda_{n}}\frac{\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\alpha^{T}(A)}{A!}\}$
.
4Main
Result
We define ascaled
process
$W_{t}^{(n)}(\cdot)$ by$W_{t}^{(n)}( \cdot)=\frac{1}{\sqrt{n}}W_{[nt]}(\cdot)$
.
Decompose $\Lambda_{n}$ into aset of intervals with length $n^{\alpha}$:
$\Lambda_{n}=B_{n}(1)\cup\cdots\cup B_{n}(n^{1-\alpha})$
where $B_{n}(k)=((k-1)n^{\alpha}, kn^{\alpha}]$.
Furthermore
we
assume
that$c(t)=h( \frac{k}{n^{1-\alpha}})$, $d(t)= \frac{1}{\sqrt{n}}g(\frac{k}{n^{1-\alpha}})$ $(t\in B_{n}(k))$
for continuous functions $f(x)$ and $g(x)$,
and put
$h$ $= \inf\{\beta_{1}>h;\sum_{i(A)=0}|A|^{4}e^{-(\beta_{1}|A|^{2}-c_{3}|A|)_{\frac{|\alpha^{T}(A)|}{A!}<\infty}}\}$.
Theorem 4.1 If $\beta_{1}>\beta\alpha$
), then afinite dimensional distribution of $W_{t}^{(n)}(\cdot)$ converges to the
corre-spond finite dimensional distribution of
$\int_{0}^{t}\sigma(s)dB(s)+\int_{0}^{t}\mu(s)ds$
where
$\sigma^{2}(s)=\sum_{:(A)=0}<A>^{2}e^{\beta_{3}h(\epsilon)f_{1}(A)_{\frac{\phi_{0}(A)\alpha^{T}(A)}{A!}}}$
$\mu(s)=\sum_{:(A)=0}g(s)e^{\beta_{3}h(\epsilon)f_{1}(A)}f_{2}(A)<A>\frac{\phi_{0}(A)\alpha^{T}(A)}{A!}$
Outline ofthe proof ofTheorem 4.1
We state
an
outline of the proof ofTheorem 4.1. (See [7] for detail.) The main toolfor the proof is the method of polymer expansion developed in the previous section.
Applying Lemma 3.2 for $\varphi(A)=\exp\{iz\frac{1}{\sqrt{n}}W_{[nt]}(A)\}\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\alpha(A)$ we have
the following description of acharacteristic function $\varphi_{t}^{(n)}(z)$ of
one
dimensionaldistribu-tionof $W_{t}^{(n)}$,
$\varphi_{t}^{(n)}(z)=E[\exp\{iz\frac{1}{\sqrt{n}}\sum_{u\leq[nt]}<\xi_{u}>\}]$
$= \exp\{\sum_{A\subset\Lambda_{n}}(e^{\dot{\iota}z\frac{1}{\mathrm{v}^{\acute{n}}}W_{[nt]}(A)}-1)\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\frac{\alpha^{T}(A)}{A!}\}$
.
Using the Taylor’s expansion
we
have$\sum_{A\subset\Lambda_{n}}(e^{\dot{|}z\frac{1}{\sqrt{n}}W_{[nt]}(A)}-1)\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\frac{\alpha^{T}(A)}{A!}\}$ $=izI_{1}(n)- \frac{1}{2}z^{2}I_{2}(n)-\frac{iz^{3}}{6}I_{3}(n)$, where $I_{1}(n)= \frac{1}{\sqrt{n}}\sum_{A\subset\Lambda_{n}}W_{[nt]}(A)\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\frac{\alpha^{T}(A)}{A!}$ I2(n) $= \frac{1}{n}\sum_{A\subset\Lambda_{n}}W1^{nt}](A)^{2}\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\frac{\alpha^{T}(A)}{A!}$ $I_{3}(n)= \frac{1}{n\sqrt{n}}\sum_{A\subset\Lambda_{\hslash}}W_{[nt]}(A)^{3}e^{z\theta}.\cdot\neq_{n}W_{[nt]}(A)\phi_{0}(A)\phi_{1}(A)\phi_{2}(A)\frac{\alpha^{T}(A)}{A!}$
for
some
$\theta_{1}\in(0,1)$.
Employing the method of poymer expansion developed in the theory of statistical
mechanics we have thefollowing results.
When $\beta_{1}>\mathrm{f}\mathrm{f}\mathrm{i}$ we provethat
$\lim_{narrow\infty}I_{1}(n)=\int_{0}^{t}\mu(s)ds$
$\lim_{narrow\infty}I_{2}(n)=\int_{0}^{t}\sigma^{2}(s)ds$
$\lim_{narrow\infty}I_{3}(n)=0$
It follows from this propositionthat
$\varphi_{t}^{(n)}(z)$ $arrow\exp\{iz\int_{0}^{t}\mu(s)ds-\frac{1}{2}z^{2}\int_{0}^{t}\sigma^{2}(s)ds\}$
Hence the
one
dimensional distribution of $W^{(n)}(t)$ converges to the correspondingdistribution of
$\int_{0}^{t}\mu(s)ds+\int_{0}^{t}\sigma(s)dB(s)$
.
Acharacteristic function of afinite dimensional distribution $\varphi_{t_{1},\cdots,t_{k}}$$(z_{1}, \cdots, z_{k})$ of
$W^{(n)}(t)$ is given by
$\varphi_{t_{1,\prime}t_{k}}\ldots(z_{1}, \cdots, z_{k})=E[\exp\{\frac{1}{\sqrt{n}}\sum_{k=1}^{m}z_{k}W_{[nt_{k}]}\}]$
.
Using the result in
one
dimensionalcase
we have$\varphi_{t_{1,\prime}t_{k}}\ldots(z_{1}, \cdots, z_{k})arrow\exp\{i\sum_{j=1}^{k}z_{j}\int_{0}^{t_{j}}\mu(s)ds-\frac{1}{2}\sum_{p=1}^{k}\sum_{q=1}^{k}z_{\mathrm{p}}z_{q}\int_{0}^{t_{\mathrm{p}}\wedge t_{q}}\sigma^{2}(s)ds\}$
as
$narrow\infty$.
This implies that the finite dimensional distribution of $W^{(n)}(t)$ converges tothe corresponding distribution of
$\int_{0}^{t}\mu(s)ds+\int_{0}^{t}\sigma(s)dB(s)$
.
Remark
on
trading volumeInthis auction model atrading volume$v_{t}$ at time $t$ is given by
$v_{t}={\rm Min}\{\omega_{t}^{+},\omega_{t}^{-}\}$
.
Let
us
remark that trading volume is not alwayszero
when$t$isstatic andaprobabilitydistributionof trading volume$v_{t}$for static$t$is uniformdistribution. So, the expectation
value of$v_{t}$ for static$t$ is given by
$e(v)= \frac{e(v)}{n_{0}}$
$e(v)=. \sum_{\omega_{t}\cdot \mathrm{s}\mathrm{t}\mathrm{a}\mathrm{t}\mathrm{i}\mathrm{c}}v(\omega_{t})$ and $n_{0}=. \sum_{\omega_{\ell}.\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{t}\mathrm{i}\mathrm{c}}1$.
We denote by$V[nt]$ atotal trading volume traded in time interval $[0, [nt]]$ and considera
asymptoticbehavior of$E[V_{[nt]}]$ and $V[V_{[nt]}]$,where $E[V_{[nt]}]$ and $V[V_{[nt]}]$
are an
expectationand avarianceofVjnt], respectively.
Using the method of polymer expansion
we
describe acharacteristicfunction
ofVjnt]andobtain the formulas of$E[V_{[nt]}]$ and $V[V_{[nt]}]$ in terms of polymer weight functions.
Prom these formulas and using the
same
method obtaining the scaling limit of thecharacteristicfunction for afinitedimensional distribution $W[nt]$
we
have$\lim_{narrow\infty}\frac{1}{n}E[V_{[nt]}]=\int_{0}^{t}(\sum_{i(A)=O}v(A)e^{h(x)f_{1}(A)}\frac{\phi_{0}(A)\alpha^{T}(A)}{A!}dx$
$\lim_{narrow\infty}\frac{1}{n}V[V_{[nt]}]=t(\frac{e(v^{2})}{n_{0}}-(\frac{e(v)}{n_{0}})^{2})$
$-( \frac{e(v^{2})}{n_{0}}-(\frac{e(v)}{n_{0}})^{2})\int_{0}^{t}\sum_{i(A)=O}|p(A)|e^{h(x)f1(A)}\frac{\phi_{0}(A)\alpha^{T}(A)}{A!}dx$
$+ \int_{0}^{t}\sum_{:(A)=O}(v(A)-\frac{e(v)}{n_{0}}||p(A)|)^{2}e^{h(x)f_{1}(A)}\frac{\phi_{0}(A)\alpha^{T}(A)}{A!}dx$
where
$v(A)= \sum_{\xi}\sum_{u\in p(\xi)}v(\xi_{u})A(\xi)$
$e(v^{2})=. \sum_{\{v_{t}\cdot \mathrm{s}\mathrm{t}\mathrm{a}\mathrm{t}\mathrm{i}\mathrm{c}}v(\omega_{t})^{2}$
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