Abstract
The non-stationary problem
\begin{equation}
u_{xx}=k^2(x)u_{tt}, \tag{1} \label{1}
\end{equation}
is investigated, where $k(x)=k_0$ for $x<0$ and $k(x)=k_1$ for $x>x_0$, under the initial condition $u_0(x,t) = \mu(t-k_0x)$ for $t<0$, where $\mu(z)=0$ for $z<0$.
It is shown that under the condition $\operatorname{var}\ln k(x)<\pi$, the limit of the solution to equation \eqref{1} as $t\to\infty$ for the case of an incident wave of the form
$$u_0(x,t)=\mu(t-k_0x),\quad\mu(z)=\mu_0,\quad z>z_0$$
is equal to $\lim_{t\to\infty}u(x,t)=\frac{2\mu_0k_0}{k_0+k_1}$. That is, the limit is the same as in the case where $k(x)=k_0$ for $x<0$ and $k(x)=k_1$ for $x>0$.
This result is generalized to the case where $\lim_{x\to-\infty}k(x)=k_0$ and $\lim_{x\to+\infty}k(x)=k_1$. Previously, Atkinson obtained a similar result for the stationary problem $u_{xx}-k^2(x)u=0$ under the condition $\operatorname{var}\ln k(x)\le\pi$.
Full Text
Preamble
In 1967, I. Z. Kayaks [1] investigated the equation $U_{xx} + k^2(x)U = 0$ for $0 < t < a$, as discussed in [2]. Considering the limit as $t \to 0$, where $\mu(z) = 0$ and $n - k_0x$, it was shown that if $\text{var} \ln k(x) < \infty$ as $n \to -\infty$, the solution behaves according to the conditions established in [1]. As $x \to +\infty$, the function $k(x)$ is such that the initial wave $U_0(x, t) = \mu(t - k_0x)$ for $t < 0$, with $\mu(z) = \mu_0 = \text{const}$ for $z > 0$. For the wave equation $U_{xx} = k^2(x)U_{tt}$, we assume $k(x) = k_1$ for $x < 0$. As shown in [FIGURE: 1], we assume $k(x)$ varies such that for $x > x_0$, $k(x) = k_0 = \text{const}$, and the derivative $k'(x)$ is proportional to $1/k_0$. For $t < 0$, the solution is $U(x, t) = \mu(t - k_0x)$, where $\mu(z) = 0$ for $z < 0$.
Following the methodology in [2], the solution to the system (1) can be represented as the sum of two components, $v^(x, t)$ and $W^(x, t)$, which satisfy the following integral relations:
$$\begin{aligned}
v^(x, t) &= v_0(x, t) + \frac{1}{2k(x)^{1/2}} \int k'(s) W^\left[s, \int k(l)dl\right] ds, \
W^(x, t) &= \frac{1}{2k(x)^{1/2}} \int k'(s) k(s) \left[ v^\left(s, \int k(l)dl\right) \right] ds.
\end{aligned}$$
The derivatives are related by $k(x)v^_t(x, t) = -v^_x(x, t) + \frac{1}{2}[W^(x, t) - v^(x, t)]$ and $k(x)W_t(x, t) = W^_x(x, t) + \frac{1}{2}[W^(x, t) - v^(x, t)]$. Defining $v(x, t) = k^{1/2}v^(x, t)$ and $W(x, t) = k^{1/2}(x)W^*(x, t)$, and introducing the variables $\sigma = \int k(l)dl$ and $\sigma_0$, we obtain the system:
$$\begin{aligned}
v(\sigma, t) &= k^{1/2}\mu(t-\sigma) + \frac{1}{2} \int \frac{g'(s)}{g(s)} W(s, \sigma+s) ds, \
W(\sigma, t) &= -\frac{1}{2} \int \frac{g'(s)}{g(s)} v(s, t+\sigma-s) ds,
\end{aligned}$$
where $g(\sigma) = k[x(\sigma)]$. These equations can be solved via successive approximations: $v = v_0 + v_2 + v_4 + \dots$ and $W = W_1 + W_3 + W_5 + \dots$, where the base term is $v_0(\sigma, t) = k^{1/2}\mu(t-\sigma)$.
Under the condition that $|\mu(\sigma)| < M$ and defining $q(\sigma) = \int \frac{|g'(s)|}{g(s)} ds$, we assume $q_0 = q(\sigma_0) < \pi/2$. As demonstrated in [2], if $\text{var} \ln k(x) < \pi$, the terms of the series are bounded by:
$$\begin{aligned}
|v_{2k}(\sigma, t)| &\le M k_0^{1/2} \frac{q^{2k}}{(2k)!}, \
|W_{2k+1}(\sigma, t)| &\le M k_0^{1/2} \frac{q^{2k+1}}{(2k+1)!}.
\end{aligned}$$
Summing these estimates, we find $|U(t, \sigma)| = |v + W| < M k_0^{1/2} \exp(q) (1 + \tan q_0)$. Specifically, the solution satisfies:
$$|v(\sigma, t)| \le M k_0^{1/2} [\cos q + \alpha \sin q] = M k_0^{1/2} \cos(q_0 - q).$$
In the limit as $t \to \infty$, we define the stationary transmission and reflection coefficients. For the case where $\mu(z) = \mu_0$ for $z > z_0$, the asymptotic values $v_{2k}(\sigma)$ and $W_{2k+1}(\sigma)$ are reached for $t > 2k\sigma_0 - \sigma + z_0$.
The final solution for the transmitted wave $U(\sigma)$ and reflected wave $W(\sigma)$ can be expressed as:
$$\begin{aligned}
U(\sigma) &= \mu_0 k_0^{1/2} [\cosh \tau + (\rho - 1) \sinh \tau], \
W(\sigma) &= \mu_0 k_0^{1/2} [\sinh \tau + (\rho - 1) \cosh \tau],
\end{aligned}$$
where $\rho = 1 - \tanh \tau_0$. For a medium where $k(x) = k_0$ for $x < 0$ and $k(x) = k_1$ for $x > x_0$, the reflection coefficient $R$ is given by the standard formula $R = \frac{k_0 - k_1}{k_0 + k_1}$.
In the general case where $\lim_{x \to -\infty} k(x) = k_0$ and $\text{var} \ln k(x) < \pi$ over the interval $(-\infty, +\infty)$, we consider a truncated medium $k_N(x)$ such that $k_N(x) = k(x)$ for $|x| < N$. By taking the limit $N \to \infty$, we ensure the convergence of the approximate solutions $v_N$ and $W_N$ to the exact solutions $v$ and $W$. The error $|v + W - U_N|$ is bounded by $\epsilon$ for sufficiently large $N$, confirming that the integral representation remains valid for infinite domains provided the total variation of the logarithm of the refractive index is bounded.
References
- Atkinson, F. V. Journal of Mathematical Analysis and Applications, 1, No. 3, 4, 255–276, 1960.
- [Author Initials]. Journal of Numerical Physics (N. F.), No. 4, 66–74, 1964.
Submitted May 12, 1966, Moscow State University.