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On the Stationary Solution of the Mathematical Model for Grain Boundary Grooving (Functional Equations in Mathematical Models)

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(1)

On

the Stationary

Solution of

the

Mathematical

Model

for

Grain

Boundary Grooving

Akira

Yanagiya

1

and

Yosihito

Ogasawara

2

柳谷 晃 小笠原 義仁

$1$

Advanced Institute for Complex Systems of Waseda University

3-31-1,Kamishakuzii,Nerima-ku,Tokyo,177-0044,Japan. Tel:81-3-5991-4151,Fax:81-3-3928-4110,[email protected]

2

Science

and Engeneering Department of Waseda University

3-4-1,Ookubo,Sinjuku-ku,Tokyo,169-8555, Japan

[email protected]

1. Introduction

In this talk,

we

will present

some

stationarysolution for nonlinear partial

differ-ential equation called Mullins Equation which is occered in the theory ofgrain

boundary grooving.

$u_{t}=-C_{1}^{E}(u)(1+u_{x}^{2})^{1/2}exp(-C_{2}^{E}(u) \frac{u_{xx}}{(1+u_{x}^{2})^{3/2}})+C_{1}^{C}(u)(1+u_{ox}^{2})^{1/2}$

.

(1)

The maintool, which

we

can

use, is the admissibility propertybetween weighted

continuous function spaces for the integral $\mathrm{o}\mathrm{p}\mathrm{e}\mathrm{r}\mathrm{a}\mathrm{t}\mathrm{o}\mathrm{r},\mathrm{a}\mathrm{s}$follows.

$T_{\xi}x(t)=- \int_{t}^{\infty}e^{\zeta_{1}(t-\epsilon)}F(x(s), y(s))ds$,

$T_{\xi}y(t)= \xi e^{\zeta_{2}t}+\int_{0}^{t}e^{\zeta_{2}(t-\epsilon)}F(x(s),y(s))ds$

.

(2)

Prom this admissibility

we can

prove the existence theorem for the special si-multaneous differential equation. This existence theorem

can

be applied for the second order differential equation,

$u’=f(u, u’)= \frac{kT(u)(1+u^{\prime 2})^{3/2}}{v\gamma}ln(\frac{P_{0}(u)}{P_{c}})$

.

(3)

The solution ofthis equation is

one

ofthe stationary solutionfor Mullins Equa

数理解析研究所講究録 1309 巻 2003 年 237-239

(2)

2. Theorems

On the equation (1),

we

are

interested in the stational solution. So

we

shall consider the equation (3) which

we

can

make by putting $u_{t}=0$for the equation

(1). To prove the existence theorem for the stational solution,

we use

the next

two theorems. Theoreml

For the second oreder

differential

equation,

$u’=f(u,u’)$, (4)

suppose that the following hypotheses.

$f(u,p)\in C^{1}(R^{2})$, $x>0$, $\exists\lambda\in R^{1}$ $s.t$

.

$f(\lambda, 0)=0$,

$f_{\mathrm{u}}(\lambda,0)>0$

Then there exits the solution

on

$(0, \infty)$ and it satisfies that

$\exists D>0$ $s.t$

.

$|u(x)-\lambda|\leq Dexp(-rx)$,

where

$0< \tau<|\frac{f_{p}(\lambda,0)-\sqrt{f_{p}(\lambda,0)^{2}+4f_{u}(\lambda,0)}}{2}|$

.

TheOrem2

On the differential equation,

$\omega_{1}’=\zeta_{1}\omega_{1}+F(\omega_{1},\omega_{2})$

,

$\omega_{2}’=\zeta_{2}\omega_{2}+F(\omega_{1},\omega_{2})$

,

$x>0$

,

where,

$f(\eta_{1},\eta_{2})\in C^{1}(R^{2})$, $F(0,0)=0$, $F_{\eta 1}(0,0)=0$

,

$\zeta_{1}>0$

,

$\zeta_{2}<0$,

there exists

some

global nontrivial solution

$\omega(x)=(\omega_{1}(x),\omega 2(x))$, $x>0$,

for every $\tau$,$0<\tau<|\zeta_{2}|$, and the next inequality is satisfied.

$|e^{\tau x}\omega_{1}(x)|+|e^{\tau x}\omega_{2}(x)|<\infty$, $x>0$

.

At first

we

consider TheOrem2. By using the addmissibility of the integral

operator(2),

we can

establish the proof ofTheOrem2. Let consider the integral operator

on

the following function set $\mathrm{B}$

,

$B=\omega(x)=(\omega_{1}(x),\omega_{2}(x))\in C^{0}([0, \infty));||\omega||\leq 2|\xi|$,

$|| \omega||=\sup_{x\geq 0}(e^{\tau ax}\omega_{1}(x)+e^{\tau x}\omega_{2}(x))$

.

(3)

On

this set the integral operator(2) satisfies the contraction princeple. Then

the operator $T_{\xi}$ : B $arrow B$ has the unique fixes point $\omega(x)=(\omega_{1}(x),\omega_{2}(x))$

.

Hence

we

can

prove TheOrem2. Next

we

treat Theoreml, by using theresults of

TheOrem2. Let define thefunction $F(\omega_{1},\omega_{2})$ in TheOrem2 by the next equation,

$F( \eta_{1}, \eta_{2})=f(\frac{\eta_{1}-\eta_{2}}{\zeta_{1}-\zeta_{2}}+\lambda, \frac{\zeta_{1}\eta_{1}-\zeta_{2}\eta_{2}}{\zeta_{1}-\zeta_{2}})-\frac{\eta_{1}-\eta_{2}}{\zeta_{1}-\zeta_{2}}f_{u}(\lambda,0)-\frac{\zeta_{1}\eta_{1}-\zeta_{2}\eta_{2}}{\zeta_{1}-\zeta_{2}}f_{p}(\lambda,0)$,

where

$\zeta_{1}=\frac{f_{p}(\lambda,0)+\sqrt{f_{p}(\lambda,0)^{2}+4f_{u}(\lambda,0)}}{2}>0$,

$\zeta_{2}=\frac{f_{p}(\lambda,0)-\sqrt{f_{p}(\lambda,0)^{2}+4f_{u}(\lambda,0)}}{2}<0$,

where the function $f$

as

in Theoreml. By the result of TheOrem2 there exists

the solution $\omega(x)=(\omega_{1}(x),\omega_{2}(x))$

.

Define

$u(x)= \frac{\omega_{1}(x)-\omega_{2}(x)}{\zeta_{1}-\zeta_{2}}+\lambda$, $x>0$

.

This function $u$ is the solution in Theoreml. At last,

we

can

apply Theoreml

for the equation (3),

we

get the stational solution of (1).

References

$\mathrm{A}.\mathrm{K}\mathrm{i}\mathrm{t}\mathrm{a}\mathrm{d}\mathrm{a},\mathrm{J}.\mathrm{M}\mathrm{a}\mathrm{t}\mathrm{h}.\mathrm{P}\mathrm{h}\mathrm{y}\mathrm{s}.(1986),(1987)$

.

P.Broadbridge,J.Math.Phys.(1989).

参照

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