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数学物理学报, 2024, 44(2): 326-353

带有非局部 Laplace 算子的饱和 Schrödinger-Klein-Gordon 方程的概自守动力学

张天伟,, 李永昆,*

云南大学数学与统计学院 昆明 650500

Almost Automorphic Dynamics of Nonlocal Laplacian Saturating Schrödinger-Klein-Gordon Equations

Zhang Tianwei,, Li Yongkun,*

School of Mathematics and Statistics, Yunnan University, Kunming 650500

通讯作者: * 李永昆,Email: yklie@ynu.edu.cn

收稿日期: 2022-06-8   修回日期: 2023-10-7  

基金资助: 国家自然科学基金(12261098)
国家自然科学基金(11861072)

Received: 2022-06-8   Revised: 2023-10-7  

Fund supported: NSFC(12261098)
NSFC(11861072)

作者简介 About authors

张天伟,Email:yntwzhang@outlook.com

摘要

迄今为止, 几乎没有学者研究 Schrödinger 或 Klein-Gordon 方程的概自守动力学. 该文结合 Galerkin 方法、 Laplace 变换、Fourier 级数和 Picard 迭代研究了带有非局部 Laplace 算子饱和 Schrödinger-Klein-Gordon 方程的概自守弱解的一些结果. 此外, 还考虑了该方程的全局指数收敛性.

关键词: Schrödinger; Klein-Gordon; Galerkin 方法; Fourier 级数; Picard 迭代

Abstract

To the best of the authors' knowledge, almost no literature focuses on the almost automorphic dynamics to Schrödinger or Klein-Gordon equations. This paper gives some results on almost automorphic weak solutions to a nonlocal Laplacian saturating Schrödinger-Klein-Gordon equations by employing a mix of Galerkin method, Laplace transform, Fourier series and Picard iteration. Beyond that, global exponential convergence of the equations is investigated.

Keywords: Schrödinger; Klein-Gordon; Galerkin method; Fourier series; Picard iteration

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本文引用格式

张天伟, 李永昆. 带有非局部 Laplace 算子的饱和 Schrödinger-Klein-Gordon 方程的概自守动力学[J]. 数学物理学报, 2024, 44(2): 326-353

Zhang Tianwei, Li Yongkun. Almost Automorphic Dynamics of Nonlocal Laplacian Saturating Schrödinger-Klein-Gordon Equations[J]. Acta Mathematica Scientia, 2024, 44(2): 326-353

1 引言

本文用 Rd 表示 d 维欧式空间, R0=[0,+), R+=(0,+); Z+={1,2,}; 用 C 表示复数集. 设 ΩRd 中一个具有光滑边界 Ω 的有界开域, ˉΩ:=ΩΩ. 本文致力于研究如下带有非局部 Laplace 算子的饱和 Schrödinger-Klein-Gordon 方程

{itz2(Δ)αz+iaz+μzw1+ρ|z|+ϱ|w|=f(x,t),inΩ×R+,2t2w+(Δ)βw+btw+cw=ν|z|21+ε|z|+g(x,t),inΩ×R+,z=w=0,inΩ×R0,
(1.1)

其中 z=z(x,t), w=w(x,t) 分别表示复标量核子场和实介子场; i=1 是虚数单位; α,β(0,1) 满足 2max; \hbar>0 为普朗克常数; a>0 为系统的耗散机制; b>0 是阻尼系数; c>0 为介子的质量; \mu, \nu>0 是耦合常数; f\in\mathbf{C}, g\in\mathbf{R} 表示外力; 饱和函数 \mathbf{Sat} _1 \mathbf{Sat} _2 定义为

\mathbf{Sat} _1(\mathbf{z} \mathbf{w} )=\frac{\mathbf{z} \mathbf{w} }{1+\rho|\mathbf{z}|+\varrho| \mathbf{w} |},\quad \mathbf{Sat} _2(|\mathbf{z}|^2)=\frac{|\mathbf{z}|^{2}}{1+\varepsilon|\mathbf{z}|},

其中 \mathbf{z}=\hat{\mathbf{z}}+\mathrm{i}\breve{\mathbf{z}}\in\mathbf{C}, |\mathbf{z}|=\sqrt{\hat{\mathbf{z}}^2+\check{\mathbf{z}}^2}, \rho, \varrho\varepsilon 为正饱和系数. 令 \rho, \varrho, \varepsilon\rightarrow0, 则方程 (1.1) 转化为非饱和方程, 这类方程在过去的几十年中被广泛研究, 参见文献 [1],[2],[3],[4],[5].

方程 (1.1) 的初值条件为

\mathbf{z}(x,0)=\varphi(x)=\hat{\varphi}(x)+\mathrm{i}\breve{\varphi}(x),\quad \mathbf{w} (x,0)=\phi(x),\quad \lim\limits_{t\rightarrow0}\frac{\partial}{\partial t} \mathbf{w} (x,t)=\psi(x),\quad \mbox{在 $\Omega$ 中}.

著名的 Schrödinger-Klein-Gordon 方程是量子场论中描述守恒的复中子场与实介子场相互作用的经典模型. 耦合的 Schrödinger-Klein-Gordon 方程, 因其相当精确地描述了物理系统关于时间的量子态, 而且这种耦合方程的发展为科学和工程领域开辟了新的前景, 因此这类方程吸引了许多学者的关注. 近年来 Schrödinger-Klein-Gordon 系统成为描述量子力学的重要工具, 被众多学者所研究, 参见文献 [3],[4],[5],[6],[7]. 另一方面, 问题 (1.1) 中的非线性项 \mathbf{Sat} _1 \mathbf{Sat} _2 可以看作一种特殊的"饱和非 Kerr 律", 出现在许多应用中. 饱和定律精确地描述了经过激光束的气体蒸气介电常数的变化, 这种现象也发生在光纤的孤子传播中. 在半导体掺杂光纤中, 孤子输运模型采用饱和非线性而不是通常的 Kerr 非线性. 这么做的主要动机是在半导体掺杂玻璃和其他复合材料可以观察到较弱的非线性. 饱和函数已经被广泛研究, 参见文献 [8],[9],[10],[11],[12].

Bochner 在其微分几何著作[13]中首次提出了概自守的概念, 它是概周期的推广. 概自守的概念在研究一类常微分方程、抛物方程和广义微分方程的概自守动力学中是必不可少的, 这一事实进一步说明了概自守在动力学定性研究中的重要性. 首先, 就从系数空间到解空间的升力性质而言, 动力学在概周期的范畴内通常不是封闭的, 但是在概自守的范畴内是封闭的. 其次, 概自守动力学的出现说明了周期系统与概周期系统的主要区别. 例如, 在单调动力系统中, 周期系数的"升力"永远不可能是概自守的. 研究概自守动力学的另一个重要意义是它与 Levitan N-概周期性的关系. 因为概自守函数在本质上是 N-概周期的, 所以目前对概自守动力学的研究与 N-概周期的情况密切相关, 参见文献 [14],[15],[16],[17],[18],[19],[20].

纵观历史, 几乎全部现有的文章都集中在 Schrödinger 或 Klein-Gordon 方程的概周期动力学的研究上, 参见文献 [21],[22],[23],[24],[25],[26]. 例如, 利用 KAM 定理, 作者在文献 [21],[22],[23],[24] 中研究了一类特殊的 Schrödinger 方程的概周期解. Signing[25] 考虑了具有概周期集的 Klein-Gordon 型方程的均匀化问题. Abdallah 等[26]研究了具有非线性概周期项的 Klein-Gordon-Schrödinger 无限维格系统的一致全局吸引子的存在性. 然而, 据我们所知, 目前几乎没有文献涉及到 Schrödinger 或 Klein-Gordon 方程的概自守动力学研究. 受此启发, 本文将结合 Galerkin 方法、Fourier 级数、Laplace 变换和 Picard 迭代, 研究带有非局部 Laplace 算子的饱和 Schrödinger-Klein-Gordon 方程 (1.1) 在合适的函数空间中概自守弱解的存在性和唯一性.

1.1 非局部 Laplace 算子

s\in(0,1), \mathscr{S} 是速降函数组成的 Schwartz 空间, 分数阶 Laplace 算子[27] (-\Delta)^{s}:\mathscr{S}\rightarrow \mathrm{L}^2(\mathbf{R}^d) 表示为

\label{dy1} (-\Delta)^{s}{ \mathbf{u} }(x)=C(d,s)\lim\limits_{\epsilon\rightarrow 0^+}\int_{\mathbf{R}^d\setminus \mathbf{B}(x,\epsilon)} \frac{{ \mathbf{u} }(x)-{ \mathbf{u} }(y)}{|x-y|^{d+2s}} \mathrm{d}y,\quad\forall { \mathbf{u} }\in\mathscr{S}, x\in\mathbf{R}^d,

其中 \mathbf{B}(x,\epsilon) 表示球心为 x\in\mathbf{R}^d, 半径为 \epsilon 的球, C(d,s) 是标准化常数, 其表达式为

\frac{1}{C(d,s)}=\int_{\mathbf{R}^d}\frac{1-\cos\zeta_1}{|\zeta|^{d+2s}} \mathrm{d}\zeta, \quad \zeta=(\zeta_1,\zeta'), \zeta'\in\mathbf{R}^{d-1}.

s\in(0,1), (-\Delta)^{s} 的一个等价形式为

\label{dy2} (-\Delta)^{s} \mathbf{u} (x)=-\frac{1}{2}C(d,s)\int_{\mathbf{R}^d} \frac{ \mathbf{u} (x+y)+ \mathbf{u} (x-y)-2 \mathbf{u} (x)}{|y|^{d+2s}} \mathrm{d}y,\quad \forall \mathbf{u} \in\mathscr{S}, x\in\mathbf{R}^d.

\mathrm{X}^s(\Omega) 表示所有 Lebesgue 可测函数 { \mathbf{u} }:\mathbf{R}^d\rightarrow\mathbf{R} 组成的线性空间, 使得在 \mathrm{X}^s(\Omega) 中任意函数 { \mathbf{u} }\Omega 的限制属于 \mathrm{L}^2(\Omega), 定义 \mathrm{X}^s(\Omega) 的范数为

| \mathbf{u} |_{\mathrm{X}^s}=| \mathbf{u} |_{2} +\bigg(\int_{Q\times Q}\frac{| \mathbf{u} (x)- \mathbf{u} (y)|^2}{|x-y|^{d+2s}} \mathrm{d}x\mathrm{d}y\bigg)^{\frac{1}{2}}, \quad\forall \mathbf{u} \in\mathrm{X}^s(\Omega),

其中 |\cdot|_2 表示 \mathrm{L}^2(\Omega) 的范数, Q:=(\mathbf{R}^d\times \mathbf{R}^d)\backslash(\eth\Omega\times\eth\Omega), \eth\Omega:=\mathbf{R}^d\backslash\Omega. 定义

\mathrm{X}_0^s(\Omega):=\{u\in\mathrm{X}^s(\Omega): \mathbf{u} =0\ \text{在}\ \mathbf{R}^d\backslash\Omega\ \text{中几乎处处成立}\},

其范数为

| \mathbf{u} |_{\mathrm{X}_0^s}=\bigg(\int_{\mathbf{R}^d\times\mathbf{R}^d}\frac{| \mathbf{u} (x)- \mathbf{u} (y)|^2}{|x-y|^{d+2s}} \mathrm{d}x\mathrm{d}y\bigg)^{\frac{1}{2}},\quad \forall \mathbf{u} \in\mathrm{X}_0^s(\Omega), x\in\mathbf{R}^d.

\left(\mathrm{X}_0^s(\Omega), |\cdot|_{\mathrm{X}_0^s}\right) 是 Hilbert 空间, 其内积为

\big\langle \mathbf{u}, \mathbf{v} \big\rangle_{\mathrm{X}_0^s}= \int_{\mathbf{R}^d\times\mathbf{R}^d}\frac{[ \mathbf{u} (x)- \mathbf{u} (y)][ \mathbf{v} (x)- \mathbf{v} (y)]}{|x-y|^{d+2s}} \mathrm{d}x\mathrm{d}y, \quad \forall \mathbf{u}, \mathbf{v} \in\mathrm{X}_0^s(\Omega).

定义空间 \mathrm{L}_{s}^2(\Omega)=\{ \mathbf{u} :(-\Delta)^s \mathbf{u} \in\mathrm{L}^2(\Omega)\}, | \mathbf{u} |_{s,2}:=|(-\Delta)^s \mathbf{u} |_2, \forall{ \mathbf{u} }\in\mathrm{L}_{s}^2(\Omega).

考虑如下特征值问题

\begin{cases} (-\Delta)^s{ \mathbf{u} }=\lambda { \mathbf{u} }, &\quad \mbox{在}\ \Omega\ \mbox{中}, \\[0.25cm]{ \mathbf{u} }=0,&\quad \mbox{在}\ \mathbf{R}^d\backslash\Omega\ \mbox{中},\end{cases}
(1.2)

其中 s\in(0,1), d>2s. 问题 (1.2) 的弱解表示为

\label{45.10} \int_{\mathbf{R}^d\times\mathbf{R}^d}\frac{[{ \mathbf{u} }(x)-{ \mathbf{u} }(y)][ \mathbf{v} (x)- \mathbf{v} (y)]}{|x-y|^{d+2s}} \mathrm{d}x\mathrm{d}y=\lambda\int_{\Omega}{ \mathbf{u} }(x) \mathbf{v} (x) \mathrm{d}x, \quad \forall \mathbf{v} \in \mathrm{X}_0^s(\Omega),

其中 { \mathbf{u} }\in \mathrm{X}_0^s(\Omega). 根据文献 [28] 可知, 在 \mathrm{L}^2(\Omega,\mathbf{R}) 中存在对应于非局部 Laplace 算子 (-\Delta)^{s} 的一个完备的规范正交基 \{e_k\}_{k=1}^{\infty}\subseteq\mathrm{X}_0^s(\Omega). 同时, 它也是 \mathrm{X}_0^s(\Omega) 的正交基. 设 \{\lambda_k\}_{k=1}^{\infty}\{e_k\}_{k=1}^{\infty} 对应的特征值序列, 则 0<\lambda_1\leq \lambda_2\leq \cdots\leq \lambda_k\leq \cdots, \lim\limits_{k\rightarrow\infty}\lambda_k=\infty.

1.2 主要结果

\mathbb{E}_{\mathbf{z}}=\left\{ \mathbf{z}: \mathbf{z}\in\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{X}_0^\alpha(\Omega)), \dot{\mathbf{z}}_t\in \mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega)) \right\},
\mathbb{E}_{ \mathbf{w} }=\left\{ \mathbf{w} : \mathbf{w} \in\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{X}_0^\beta(\Omega)), \dot{ \mathbf{w} }_t\in\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{X}_0^\beta(\Omega)), \ddot{ \mathbf{w} }_t\in \mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega)) \right\},

其中 \dot{\mathbf{z}}_t:=\frac{\partial\mathbf{z}}{\partial t}, \dot{ \mathbf{w} }_t:=\frac{\partial \mathbf{w} }{\partial t}, \ddot{ \mathbf{w} }_t:=\frac{\partial^2 \mathbf{w} }{\partial t^2}, \forall t\in\mathbf{R}_0.

定义1.1(\mathbf{z}, \mathbf{w} )\in \mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} } 满足

\begin{eqnarray*} \left\{ \begin{array}{lll} \Big\langle\mathrm{i}\hbar\dot{\mathbf{z}}_t+ \mathrm{i}a\mathbf{z} + \mu \mathbf{Sat} _1(\mathbf{z} \mathbf{w} ),\xi\Big\rangle_{\mathrm{L}^2} -\frac{1}{2}c_{\alpha}\hbar^2\langle\mathbf{z},\xi\rangle_{\mathrm{X}_0^\alpha}=\langle f,\xi\rangle_{\mathrm{L}^2},\\ \Big\langle\ddot{ \mathbf{w} }_t+b\dot{ \mathbf{w} }_t+c \mathbf{w},\zeta\Big\rangle_{\mathrm{L}^2} +\frac{c_{\beta}}{2}\langle \mathbf{w},\zeta\rangle_{\mathrm{X}_0^\beta} =\big\langle \nu \mathbf{Sat} _2(|\mathbf{z}|^2)+g,\zeta\big\rangle_{\mathrm{L}^2},\\ \mathbf{z}(0)=\varphi,\quad \mathbf{w} (0)=\phi,\quad \dot{ \mathbf{w} }_t\big|_{t=0}=\psi, \end{array} \right. \end{eqnarray*}

其中 t\in\mathbf{R}_+, c_\alpha:=C(d,\alpha), c_\beta:=C(d,\beta), \xi, \zeta\in \mathrm{L}^2(\Omega). 则 (\mathbf{z}, \mathbf{w} )\in \mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} } 是方程 (1.1) 的一个全局弱解.

利用 Galerkin 方法, 本章的第一个主要结果如下所示

定理1.1 假设如下条件成立.

(\mathcal{K}_1) (\varphi,\phi,\psi)=(\hat{\varphi},\breve{\varphi},\phi,\psi) \in \{\mathrm{C}^2(\Omega)\cap\mathrm{X}_0^\alpha(\Omega)\cap\mathrm{L}_\alpha^2(\Omega)\}^2\times \{\mathrm{C}^2(\Omega)\cap\mathrm{X}_0^\beta(\Omega)\cap\mathrm{L}_{\beta}^2(\Omega)\}\times\mathrm{L}^2(\Omega).

(\mathcal{K}_2) f, g\in \mathrm{L}^\infty(\mathbf{R}_0,\mathrm{L}^{2}(\Omega))\cap C^1(\mathbf{R}_0,\mathrm{L}^{2}(\Omega)), \dot{f}_t:=\frac{\partial f}{\partial t}, \dot{g}_t:=\frac{\partial g}{\partial t} \in \mathrm{L}_{\mathrm{loc}}^\infty(\mathbf{R}_0,\mathrm{L}^{2}(\Omega)).

则方程 (1.1) 在 \mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} } 中至少存在一个全局弱解 (\mathbf{z}_0, \mathbf{w} _0).

\{e_k^\alpha\}_{k=1}^{\infty}\subseteq\mathrm{X}_0^\alpha(\Omega)\{e_k^\beta\}_{k=1}^{\infty}\subseteq\mathrm{X}_0^\beta(\Omega)\mathrm{L}^2(\Omega,\mathbf{R}) 中分别对应于非局部 Laplace 算子 (-\Delta)^{\alpha}(-\Delta)^{\beta} 的两个完备的规范正交基. 同时, 它们也分别是 \mathrm{X}_0^\alpha(\Omega)\mathrm{X}_0^\beta(\Omega) 的正交基. 设\{\lambda_k^\alpha\}_{k=1}^{\infty}\{\lambda_k^\beta\}_{k=1}^{\infty} 分别为 \{e_k^\alpha\}_{k=1}^{\infty}\{e_k^\beta\}_{k=1}^{\infty} 对应的特征值序列. 则 \lambda_k^\alpha\lambda_k^\beta 具有有限的多重性且满足

0<\lambda_1^\alpha\leq \lambda_2^\alpha\leq \cdots\leq \lambda_k^\alpha\leq \cdots,\quad \lim\limits_{k\rightarrow\infty}\lambda_k^\alpha=\infty,
0<\lambda_1^\beta\leq \lambda_2^\beta\leq \cdots\leq \lambda_k^\beta\leq \cdots,\quad \lim\limits_{k\rightarrow\infty}\lambda_k^\beta=\infty.

定义 (\cdot)_k:=\langle \cdot,e_k\rangle_{\mathrm{L}^2}, k\in\mathbf{Z}_+, \langle\cdot,\cdot\rangle_{\mathrm{L}^2} 表示 \mathrm{L}^2(\Omega) 的内积. 根据状态估计、矩阵理论和 Laplace 变换, 可知 (\mathbf{z}_0, \mathbf{w} _0)=(\hat{\mathbf{z}}_0,\breve{\mathbf{z}}_0, \mathbf{w} _0) 可以表示为如下形式的 Fourier 级数

\begin{array}{l} {\left[\begin{array}{c} \hat{\mathbf{z}}_{0} \\ \breve{\mathbf{z}}_{0} \end{array}\right](t)=\sum_{k=1}^{\infty}\left\{e^{-\frac{a}{\hbar} t}\left[\begin{array}{cc} \cos \left(\dot{\lambda}_{k}^{\alpha} t\right) & \sin \left(\dot{\lambda}_{k}^{\alpha} t\right) \\ -\sin \left(\dot{\lambda}_{k}^{\alpha} t\right) & \cos \left(\dot{\lambda}_{k}^{\alpha} t\right) \end{array}\right]\left[\begin{array}{c} \hat{\varphi}_{k} \\ \breve{\varphi}_{k} \end{array}\right]\right.} \\ +\frac{1}{\hbar} \int_{0}^{t} e^{-\frac{a}{\hbar}(t-s)}\left[\begin{array}{cc} \cos \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) & \sin \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) \\ \sin \left(\dot{\lambda}_{k}^{\alpha}(s-t)\right) & \cos \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) \end{array}\right] \\ \left.\times\left[\begin{array}{c} -\mu \widehat{\mathbf{S a t}}_{1, k}\left(\mathbf{z}_{0} \mathbf{w}_{0}\right)+\operatorname{Im} f_{k} \\ \mu \widetilde{\mathbf{S a t}}_{1, k}\left(\mathbf{z}_{0} \mathbf{w}_{0}\right)-\operatorname{Re} f_{k} \end{array}\right](s) \mathrm{d} s\right\} e_{k}^{\alpha}, \\ \end{array}
(1.3)
\mathbf{w} _{0}(t)=\sum\limits_{k=1}^\infty\Bigg\{e^{-\frac{b}{2}t}\left[ \cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t) \right]\phi_k + \frac{1}{\grave{\lambda}_k^\beta}e^{-\frac{b}{2}t}\sin(\grave{\lambda}_k^\beta t)\psi_k \\ +\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \left[\nu \mathbf{Sat} _{2,k}(|\mathbf{z}_0(t)|^2)+g_k(s)\right]\mathrm{d}s\Bigg\}e_k^\beta,
(1.4)

其中 \mathbf{z}_0=\hat{\mathbf{z}}_0+\mathrm{i}\breve{\mathbf{z}}_0, t\in \mathbf{R}_+,

\widehat{ \mathbf{Sat} }_1(\mathbf{z}_0 \mathbf{w} _0)=\frac{\hat{\mathbf{z}}_0 \mathbf{w} _0}{1+\rho|\mathbf{z}_0|+\varrho| \mathbf{w} _0|},\quad \widetilde{ \mathbf{Sat} }_1(\mathbf{z}_0 \mathbf{w} _0)=\frac{\breve{\mathbf{z}}_0 \mathbf{w} _0}{1+\rho|\mathbf{z}_0|+\varrho| \mathbf{w} _0|},
\acute{\lambda}_k^\alpha=\frac{1}{2}c_{\alpha}\hbar\lambda_k^\alpha,\quad \grave{\lambda}_k^\beta=\sqrt{\frac{1}{2}c_{\beta}\lambda_k^\beta+c-\frac{b^2}{4}}, \quad k=1,2,\cdots.

基于式 (1.3)-(1.4), 可知方程 (1.1) 的全局弱解 ({z}_0,{w}_0) 具有如下的唯一性、能量估计和全局指数收敛性.

定理1.2(\mathcal{K}_1)-(\mathcal{K}_2) 及以下条件成立, 则 (\mathbf{z}_0, \mathbf{w} _0)=(\hat{\mathbf{z}}_0,\breve{\mathbf{z}}_0, \mathbf{w} _0) 是方程 (1.1) 在 \mathrm{C}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) \cap\{\mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} }\} 中的唯一全局弱解.

\left(\mathcal{K}_{3}\right) b^{2}<2 c_{\beta} \lambda_{1}^{\beta}+4 c.

而且, 若 a\varrho>2\mu, 那么我们有以下的能量估计

\max\limits_{t\in\mathbf{R}_0}|\mathbf{z}_0(t)|_2\leq \frac{2\varrho(a|\varphi|_{2}+f_{\infty})}{a\varrho-2\mu}:=\mathbf{z}_{\infty},
\max\limits_{t\in\mathbf{R}_0}| \mathbf{w} _0(t)|_{2} \leq\frac{2\grave{\lambda}_1^\beta+b}{2\grave{\lambda}_1^\beta}|\phi|_{2} +\frac{1}{\grave{\lambda}_1^\beta}|\psi|_{2} +\frac{2}{\grave{\lambda}_1^\beta b}\Big[\frac{\nu}{\varepsilon}\mathbf{z}_\infty+g_{\infty}\Big]:= \mathbf{w} _{\infty},

其中 f_\infty:=\sup\limits_{t\in\mathbf{R}_0}|f(\cdot,t)|_{2}, g_\infty:=\sup\limits_{t\in\mathbf{R}_0}|g(\cdot,t)|_{2}.

定理1.3(\mathcal{K}_1)-(\mathcal{K}_3) 以及如下假设成立.

(\mathcal{K}_4) \min\left\{\frac{a}{\hbar},\frac{b}{2}\right\}>\max\left\{ \frac{64\mu^2}{a \hbar\rho_0^2},\frac{9\nu^2}{2b(\grave{\lambda}_1^\beta)^2\varepsilon^2}\right\}, 其中 \rho_0:=\min\{\rho,\varrho\}.

则方程 (1.1) 在弱解意义下是全局指数收敛的.

最后, 为了研究方程 (1.1) 的渐近概自守弱解, 我们利用 (1.3)-(1.4) 构造了一个 Picard 迭代序列并有如下结论

定理1.4(\mathcal{K}_1)-(\mathcal{K}_4) 及如下假设成立.

(\mathcal{K}_5) (f,g)=(\mathrm{Re}f,\mathrm{Im}f,g)\in\mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3).

(\mathcal{K}_6) \gamma:=\max\bigg\{\frac{8\sqrt{2}\mu}{a\rho_0}, \frac{3\nu}{b\grave{\lambda}_1^\beta\varepsilon}\bigg\}<1.

则方程 (1.1) 存在唯一的全局指数稳定的渐近概自守弱解, 其中 \mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) 表示从 \mathbf{R}_0 映到 \{\mathrm{L}^2(\Omega)\}^3 的所有渐近概自守函数组成的空间, 其定义将在第 5 节中给出.

本文的结构安排如下. 在第 3 节中, 引入了一些基本函数空间, 并用 Galerkin 方法证明了方程 (1.1) 全局弱解的存在性. 第 4 节利用矩阵理论和 Laplace 变换构造了全局弱解的 Fourier 级数, 并证明了该解的唯一性和收敛性. 并且, 给出了定理 1.2 和 1.3 的证明. 在第 5 节中, 利用 Picard 迭代方法研究了方程 (1.1) 的唯一全局渐近概自守弱解的存在性.

2 能量估计和全局弱解

I_T=(0,T), \bar{I}_T=[T], \forall T>0, \mathbb{K} 是某个有限维度量空间的子集, \mathbb{H} 表示距离为 \|\cdot\|_{\mathbb{H}} 的某个度量空间.

\bullet \mathrm{C}^m(\mathbb{K}):=\mathrm{C}^m(\mathbb{K},\mathbb{H}) 表示从 \mathbb{K} 映到 \mathbb{H} 的所有 m 阶连续可微函数组成的空间, 其范数为 \|\cdot\|_{\mathrm{C}^m}, \forall m\in\mathbf{Z}_+m=\infty. \mathrm{C}_0^m(\mathbb{K}):=\{\eta\in\mathrm{C}^m(\mathbb{K}): \mathrm{supp}\eta\subset\subset\Omega\}.

\bullet \mathrm{L}^p(\Omega):=\mathrm{L}^p(\Omega,\mathbf{C}) 表示所有可测复值映射 \eta:\Omega\rightarrow \mathbf{C} 组成的集合, 其范数为

|\eta|_{p}=\left[\int_{\Omega}|\eta(x)|^p \mathrm{d}x\right]^{\frac{1}{p}}.

特别地, \mathrm{L}^2(\Omega) 是 Hilbert 空间, 其内积为

\langle\eta,\eta\rangle_{\mathrm{L}^2}=\int_{\Omega}\eta(x)\bar{\eta}(x) \mathrm{d}x,

相应的范数为 |\eta|_2=\sqrt{\langle\eta,\eta\rangle_{\mathrm{L}^2}}. 此外, \mathrm{L}^\infty(\Omega) 表示 \Omega 上所有本性有界映射组成的集合, 其范数为 |\cdot|_{\infty}.

\bullet \mathrm{L}^p(I_T):=\mathrm{L}^p(I_T,\mathbb{H}) 表示所有的可测向量值映射 \eta:I_T\rightarrow \mathbb{H} 组成的集合, 其范数为 \|\cdot\|_{\mathrm{L}^p}, 其中

\| \eta\|_{\mathrm{L}^p}=\left\{ \begin{array}{ll} \displaystyle\bigg[\int_{0}^T\| \eta(t)\|_{\mathbb{H}}^p \mathrm{d}t\bigg]^{\frac{1}{p}}, \quad& \hbox{if $p\in[1,\infty)$;} \\ \mathrm{ess}\sup\limits_{t\in I_T}\| \eta(t)\|_{\mathbb{H}}, & \hbox{if $p=\infty$.} \end{array} \right.

此外, \mathrm{L}_{\mathrm{loc}}^p(I_T,\mathbb{H}) 为由 \mathrm{L}_{\mathrm{loc}}^p(I_T,\mathbb{H})=\big\{ \eta\in \mathrm{L}^p(I_T): \forall T>0\big\} 定义的局部 Lebesgue 空间.

定义 \mathbb{K}_n^\alpha=\mathrm{span}\{e_1^\alpha,\cdots,e_n^\alpha\}, \mathbb{K}_n^\beta=\mathrm{span}\{e_1^\beta,\cdots,e_n^\beta\}, n\in\mathbf{Z}_+,

\hat{\mathbf{z}}_n(t)=\sum\limits_{k=1}^n\hat{\mathbf{z}}_{k,n}(t)e_k^\alpha,\quad \breve{\mathbf{z}}_n(t)=\sum\limits_{k=1}^n\breve{\mathbf{z}}_{k,n}(t)e_k^\alpha,
\mathbf{z}_n(t)=\hat{\mathbf{z}}_n(t)+\mathrm{i}\breve{\mathbf{z}}_n(t)=\sum\limits_{k=1}^n\Big[\hat{\mathbf{z}}_{k,n}(t) +\mathrm{i}\breve{\mathbf{z}}_{k,n}(t)\Big]e_k^\alpha,\quad \mathbf{w} _n(t)=\sum\limits_{k=1}^n \mathbf{w} _{k,n}(t)e_k^\beta,

其中 (\mathbf{z}_n, \mathbf{w} _n) 是如下方程的解

\begin{cases} \Big\langle\mathrm{i}\hbar\frac{\partial\mathbf{z}_n}{\partial t}+ \mathrm{i}a\mathbf{z}_n+ \mu \mathbf{Sat} _1(\mathbf{z}_n \mathbf{w} _n),\xi\Big\rangle_{\mathrm{L}^2}-\frac{1}{2}c_{\alpha}\hbar^2\langle\mathbf{z}_n,\xi\rangle_{\mathrm{X}_0^\alpha}=\langle f,\xi\rangle_{\mathrm{L}^2},\\ \Big\langle\frac{\partial^2 \mathbf{w} _n}{\partial t^2}+b\frac{\partial \mathbf{w} _n}{\partial t}+c \mathbf{w} _n,\zeta\Big\rangle_{\mathrm{L}^2}+\frac{1}{2}c_{\beta}\langle \mathbf{w} _n,\zeta\rangle_{\mathrm{X}_0^\beta}=\big\langle \nu \mathbf{Sat} _2(|\mathbf{z}_n|^2)+g,\zeta\big\rangle_{\mathrm{L}^2},\\ \mathbf{z}_n(0)=\varphi+\frac{\varphi}{n},\quad \mathbf{w} _n(0)=\phi+\frac{\phi}{n},\quad \frac{\partial \mathbf{w} _n(t)}{\partial t}\bigg|_{t=0}=\psi+\frac{\psi}{n},\end{cases}
(2.1)

\forall\xi\in \mathbb{K}_n^\alpha, \zeta\in \mathbb{K}_n^\beta, t\in\bar{I}_T, n\in\mathbf{Z}_+. 根据常微分方程基本理论, 可知若 (f,g)\in\mathrm{C}^1\times\mathrm{C}^1, 则方程 (2.1) 存在唯一的解 (\mathbf{z}_n, \mathbf{w} _n)\in \mathrm{C}^2\times\mathrm{C}^3, \forall t\in\bar{I}_T, n\in\mathbf{Z}_+.

2.1 状态估计

定义 f_{T_\infty}:=\sup\limits_{t\in\bar{I}_T}\{|f(\cdot,t)|_{2},|\dot{f}_t(\cdot,t)|_{2}\}, g_{T_\infty}:=\sup\limits_{t\in\bar{I}_T}\{|g(\cdot,t)|_{2},|\dot{g}_t(\cdot,t)|_{2}\}. 接着, 我们将给出方程 (2.1) 的一些状态估计.

引理2.1(\mathcal{K}_1)-(\mathcal{K}_2) 成立. 则存在某些正常数 M_{\mathbf{z}}^T, M_{ \mathbf{w} }^T, M_{\mathbf{z}_\alpha}^T, M_{ \mathbf{w} _\beta}^T, M_{\dot{\mathbf{z}}}^T, M_{\dot{ \mathbf{w} }}^T, M_{\dot{ \mathbf{w} }_\beta}^T, M_{\ddot{ \mathbf{w} }}^T 使得

\begin{cases} \left|\mathbf{z}_n(t)\right|_2^2\leq M_{\mathbf{z}}^T,\quad\left| \mathbf{w} _n(t)\right|_2^2\leq M_{ \mathbf{w} }^T,\quad \left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2^2\leq M_{\dot{\mathbf{z}}}^T,\quad \left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_2^2\leq M_{\dot{ \mathbf{w} }}^T,\\ \left|\mathbf{z}_n(t)\right|_{\mathrm{X}_0^\alpha}^2\leq M_{\mathbf{z}_{\alpha}}^T,\quad\left| \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2\leq M_{ \mathbf{w} _{\beta}}^T,\quad \left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2\leq M_{\dot{ \mathbf{w} }_{\beta}}^T,\quad \left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|_2^2\leq M_{\ddot{ \mathbf{w} }}^T,\end{cases}

\forall t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+.

1) \{\mathbf{z}_n\}, \{ \mathbf{w} _n\}, \left\{\frac{\partial}{\partial t} \mathbf{w} _n\right\}\mathrm{L}^2-估计和 \{ \mathbf{w} _n\}\mathrm{X}_0^\beta-估计.

在 (2.1) 式的第一个方程中令 \xi={z}_n, 取对应的虚部, 由插值不等式, 可得

\frac{\hbar}{2} \frac{\mathrm{d}}{\mathrm{d} t}\left|\mathbf{z}_{n}(t)\right|_{2}^{2}+a\left|\mathbf{z}_{n}(t)\right|_{2}^{2} \leq|f|_{2}\left|\mathbf{z}_{n}(t)\right|_{2} \leq \frac{1}{2}\left|\mathbf{z}_{n}(t)\right|_{2}^{2}+\frac{1}{2}|f|_{2}^{2},
(2.2)

\frac{\mathrm{d}}{\mathrm{d} t}\left|\mathbf{z}_{n}(t)\right|_{2}^{2} \leq \frac{1}{\hbar}\left|\mathbf{z}_{n}(t)\right|_{2}^{2}+\frac{1}{\hbar}|f|_{2}^{2} \Rightarrow\left|\mathbf{z}_{n}(t)\right|_{2}^{2} \leq 4|\varphi|_{2}^{2}+\frac{t}{\hbar} f_{T_{\infty}}^{2}+\frac{1}{\hbar} \int_{0}^{t}\left|\mathbf{z}_{n}(s)\right|_{2}^{2} \mathrm{~d} s,

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+. 利用 Gronwall 不等式, 可得

\left|\mathbf{z}_{n}(t)\right|_{2}^{2} \leq\left[4|\varphi|_{2}^{2}+\frac{T}{\hbar} f_{T_{\infty}}^{2}\right] e^{\frac{T}{\hbar}}:=M_{\mathbf{z}}^{T}, \quad \forall t \in \bar{I}_{T}, n \in \mathbf{Z}_{+}

同理, 在 (2.1) 式的第二方程中取 \zeta=\frac{\partial}{\partial t}{w}_n, 有

\begin{aligned} & \frac{1}{2} \frac{\mathrm{d}}{\mathrm{d} t}\left|\frac{\partial}{\partial t} \mathbf{w}_{n}(t)\right|_{2}^{2}+b\left|\frac{\partial}{\partial t} \mathbf{w}_{n}(t)\right|_{2}^{2}+\frac{c_{\beta}}{4} \frac{\mathrm{d}}{\mathrm{d} t}\left|\mathbf{w}_{n}(t)\right|_{\mathrm{X}_{0}^{\beta}}^{2}+\frac{c}{2} \frac{\mathrm{d}}{\mathrm{d} t}\left|\mathbf{w}_{n}(t)\right|_{2}^{2} \\ \leq & {\left[\frac{\nu}{\varepsilon}\left|\mathbf{z}_{n}(t)\right|_{2}+g_{T_{\infty}}\right]\left|\frac{\partial}{\partial t} \mathbf{w}_{n}(t)\right|_{2} } \end{aligned}

进而

\frac{\mathrm{d}}{\mathrm{d}t}\left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_2^2 +\frac{c_{\beta}}{2}\frac{\mathrm{d}}{\mathrm{d}t}\left| \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2 +c\frac{\mathrm{d}}{\mathrm{d}t}\left| \mathbf{w} _n(t)\right|_2^2 \leq\frac{2}{b}\Big[\frac{\nu}{\varepsilon}|\mathbf{z}_n(t)|_{2}+g_{T_\infty}\Big]^2,
(2.3)

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+. 因此,

\begin{aligned} & \left|\frac{\partial}{\partial t} \mathbf{w}_{n}(t)\right|_{2}^{2}+\frac{c_{\beta}}{2}\left|\mathbf{w}_{n}(t)\right|_{\mathbf{X}_{0}^{\beta}}^{2}+c\left|\mathbf{w}_{n}(t)\right|_{2}^{2} \\ \leq & \frac{2 T}{b}\left[\frac{\nu}{\varepsilon} \sqrt{M_{\mathbf{z}}^{T}}+g_{T_{\infty}}\right]^{2}+4|\psi|_{2}^{2}+2 c_{\beta}|\phi|_{\mathbf{X}_{0}^{\beta}}^{2}+4 c|\phi|_{2}^{2}:=a_{1}, \end{aligned}
(2.4)

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+.

由不等式 (2.4), 可知

\left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_2^2\leq a_1:=M_{\dot{ \mathbf{w} }}^T,\quad\left| \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2\leq \frac{2a_1}{c_{\beta}}:=M_{ \mathbf{w} _{\beta}}^T,\quad \left| \mathbf{w} _n(t)\right|_2^2\leq \frac{a_1}{c}:=M_{ \mathbf{w} }^T,

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+.

2) \left\{\frac{\partial}{\partial t}\mathbf{z}_n\right\}\mathrm{L}^2-估计和 \{\mathbf{z}_n\}\mathrm{X}_0^\alpha-估计.

对 (2.1) 式的第一个方程两边同时取微分, 令 \xi=\frac{\partial}{\partial t}{z}_n, 取其虚部, 可得

\frac{1}{2}\frac{\mathrm{d}}{\mathrm{d}t}\left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2^2 +a\left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2^2 =\mathrm{Im}\left\langle-\mu\frac{\partial}{\partial t} \mathbf{Sat} _1(\mathbf{z}_n(t) \mathbf{w} _n(t))+\dot{f}_t, \frac{\partial\mathbf{z}_n(t)}{\partial t}\right\rangle_{\mathrm{L}^2}\qquad\quad
(2.5)

t\in \bar{I}_T\backslash\{0\} 几乎处处成立, 其中 n\in\mathbf{Z}_+. 通过直接计算可得

\begin{aligned} & \left|\operatorname{Im}\left\langle\mu \frac{\partial}{\partial t} \mathbf{S a t}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right), \frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}}\right| \\ \leq & \left|\mu \operatorname{Im}\left\langle\frac{\mathbf{z}_{n}(t) \frac{\partial \mathbf{w}_{n}(t)}{\partial t}}{1+\rho\left|\mathbf{z}_{n}(t)\right|+\varrho\left|\mathbf{w}_{n}(t)\right|}, \frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}}\right| \\ & +\left|\mu \operatorname{Im}\left\langle\frac{\rho \mathbf{z}_{n}^{2}(t) \mathbf{w}_{n}(t) \frac{\partial \overline{\mathbf{z}}_{n}(t)}{\partial t}}{2\left|\mathbf{z}_{n}(t)\right|\left(1+\rho\left|\mathbf{z}_{n}(t)\right|+\varrho\left|\mathbf{w}_{n}(t)\right|\right)^{2}}, \frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}}\right| \\ & +\left|\mu \operatorname{Im}\left\langle\frac{\varrho \mathbf{z}_{n}(t) \mathbf{w}_{n}^{2}(t) \frac{\partial \mathbf{w}_{n}(t)}{\partial t}}{\left|\mathbf{w}_{n}(t)\right|\left(1+\rho\left|\mathbf{z}_{n}(t)\right|+\varrho\left|\mathbf{w}_{n}(t)\right|\right)^{2}}, \frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}}\right| \\ \leq & \frac{2 \mu}{\rho}\left|\frac{\partial}{\partial t} \mathbf{w}_{n}(t)\right|_{2}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2}+\frac{\mu}{2 \varrho}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2}^{2} \\ \leq & \frac{(\rho+2 \varrho) \mu}{2 \rho \varrho}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2}^{2}+\frac{\mu}{\rho} M_{\dot{\mathbf{w}}}^{T}, \quad \forall t \in \bar{I}_{T} \backslash\{0\} \text { a.e., } \end{aligned}

t\in \bar{I}_T\backslash\{0\} 几乎处处成立, 其中 n\in\mathbf{Z}_+. 结合 (2.5) 式可知

\frac{1}{2} \frac{\mathrm{d}}{\mathrm{d} t}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2}^{2} \leq\left[\frac{(\rho+2 \varrho) \mu}{2 \rho \varrho}+\frac{1}{2}\right]\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2}^{2}+\frac{\mu}{\rho} M_{\dot{\mathbf{w}}}^{T}+\frac{1}{2} f_{T_{\infty}}^{2}

t\in \bar{I}_T\backslash\{0\} 几乎处处成立, 其中 n\in\mathbf{Z}_+. 由 Gronwall 不等式可得

\left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2^2 \leq \left[\left|\dot{\mathbf{z}}_n(0)\right|_2^2 + \frac{2\mu}{\rho}M_{\dot{ \mathbf{w} }}^T+f_{T_\infty}^2\right] \exp\left\{\left[ \frac{(\rho+2\varrho)\mu}{\rho\varrho}+1\right]T\right\},

t\in \bar{I}_T\backslash\{0\} 几乎处处成立, 其中 n\in\mathbf{Z}_+. 其中 \dot{\mathbf{z}}_n(0):=\frac{\partial}{\partial t}\mathbf{z}_n(t)\Big|_{t=0}, n\in\mathbf{Z}_+.

在 (2.1) 式的第一个方程中, 依次取 t\rightarrow0, \xi=\dot{{z}}_n(0), 由分部积分公式可得

\Big\langle\mathrm{i}\hbar\dot{\mathbf{z}}_n(0)+ \mathrm{i}a\varphi_n + \mu \mathbf{Sat} _1(\varphi_n\phi_n),\dot{\mathbf{z}}_n(0)\Big\rangle_{\mathrm{L}^2} -\hbar^2\langle(-\Delta)^\alpha\varphi_n,\dot{\mathbf{z}}_n(0)\rangle_{\mathrm{L}^2}=\langle f(\cdot,0),\dot{\mathbf{z}}_n(0)\rangle_{\mathrm{L}^2},

其中 \varphi_n=\varphi+\frac{\varphi}{n}, \phi_n=\phi+\frac{\phi}{n}, n\in\mathbf{Z}_+. 取相应的虚部可得

\left|\dot{\mathbf{z}}_n(0)\right|_2 \leq \frac{1}{\hbar}\left[2 a|\varphi|_2+\frac{2 \mu}{\varrho}|\varphi|_2+2 \hbar^2|\varphi|_{\alpha, 2}+f_{T_{\infty}}\right]:=a_2, \quad \forall n \in \mathbf{Z}_{+}

|\dot{\mathbf{z}}_n(0)|_2\leq \frac{1}{\hbar}\left[ 2a|\varphi|_2 +\frac{2\mu}{\varrho}|\varphi|_2 +2\hbar^2|\varphi|_{\alpha,2}+f_{T_\infty}\right]:=a_2,\quad \forall n\in\mathbf{Z}_+.

利用不等式 (2.6) 可知

\left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2^2 \leq \left[a_2^2 + \frac{2\mu}{\rho}M_{\dot{ \mathbf{w} }}^T+f_{T_\infty}^2\right] \exp\left\{\left[ \frac{(\rho+2\varrho)\mu}{\rho\varrho}+1\right]T\right\}:=M_{\dot{\mathbf{z}}}^T,

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+.

在 (2.1) 式的第一个方程中, 令 \xi=\hbar\frac{\partial}{\partial t}{z}_n+a{z}_n, 并取其实部可得

\begin{aligned} \frac{1}{2} c_{\alpha} \hbar^{2} \operatorname{Re}\left\langle\mathbf{z}_{n}(t), \hbar \frac{\partial}{\partial t} \mathbf{z}_{n}(t)+a \mathbf{z}_{n}(t)\right\rangle_{\mathbf{X}_{0}^{\alpha}}= & \operatorname{Re}\left\langle\mu \operatorname{Sat}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right), \hbar \frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}} \\ & +\operatorname{Re}\left\langle\mu \mathbf{S a t}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right), a \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}} \\ & -\operatorname{Re}\left\langle f, \hbar \frac{\partial}{\partial t} \mathbf{z}_{n}(t)+a \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}}, \end{aligned}
(2.7)

其中

\begin{aligned} \operatorname{Re}\left\langle\mu \operatorname{Sat}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right), \hbar \frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}} & \leq \mu \hbar\left|\mathbf{S a t}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right)\right|_{2}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2} \\ & \leq \frac{\mu \hbar}{\varrho}\left|\mathbf{z}_{n}(t)\right|_{2}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2} \leq \frac{\mu \hbar}{\varrho} \sqrt{M_{\mathbf{z}}^{T}} \sqrt{M_{\dot{\mathbf{z}}}^{T}}, \\ \operatorname{Re}\left\langle\mu \mathbf{S a t}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right), a \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}} & \leq a \mu\left|\mathbf{S a t}_{1}\left(\mathbf{z}_{n}(t) \mathbf{w}_{n}(t)\right)\right|_{2}\left|\mathbf{z}_{n}(t)\right|_{2} \\ & \leq \frac{a \mu}{\varrho}\left|\mathbf{z}_{n}(t)\right|_{2}^{2} \leq \frac{a \mu}{\varrho} M_{\mathbf{z}}^{T}, \\ -\operatorname{Re}\left\langle f, \hbar \frac{\partial}{\partial t} \mathbf{z}_{n}(t)+a \mathbf{z}_{n}(t)\right\rangle_{\mathrm{L}^{2}} & \leq \hbar|f|_{2}\left|\frac{\partial}{\partial t} \mathbf{z}_{n}(t)\right|_{2}+a|f|_{2}\left|\mathbf{z}_{n}(t)\right|_{2} \\ & \leq \hbar f_{T_{\infty}} \sqrt{M_{\dot{\mathbf{z}}}^{T}}+a f_{T_{\infty}} \sqrt{M_{\mathbf{z}}^{T}}, \end{aligned}

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+.

将上述结果代入式 (2.7) 可得

\frac{c_{\alpha}\hbar^3}{4}\frac{\mathrm{d}}{\mathrm{d}t}|\mathbf{z}_n(t)|_{\mathrm{X}_0^\alpha}^2 +\frac{ac_{\alpha}\hbar^2}{2}|\mathbf{z}_n(t)|_{\mathrm{X}_0^\alpha}^2\leq a_3,\quad \forall t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+,
(2.8)

其中

a_3:=\frac{\mu\hbar}{\varrho}\sqrt{M_{\mathbf{z}}^T}\sqrt{M_{\dot{\mathbf{z}}}^T}+ \frac{a\mu}{\varrho}M_{\mathbf{z}}^T+ \hbar f_{T_\infty}\sqrt{M_{\dot{\mathbf{z}}}^T}+af_{T_\infty}\sqrt{M_{\mathbf{z}}^T}.

利用不等式 (2.8) 可得

|\mathbf{z}_n(t)|_{\mathrm{X}_0^\alpha}^2\leq 4|\varphi|_{\mathrm{X}_0^\alpha}^2+ \frac{4a_3T}{c_{\alpha}\hbar^3}:=M_{\mathbf{z}_\alpha}^T,\quad \forall t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+.

3) \left\{\frac{\partial^2}{\partial t^2} \mathbf{w} _n\right\}\mathrm{L}^2-估计和 \left\{\frac{\partial}{\partial t} \mathbf{w} _n\right\}\mathrm{X}_0^\beta-估计.

对 (2.1) 式的第二个方程两边同时微分, 取 \zeta=\frac{\partial^2}{\partial t^2}{w}_n, 有

\frac{1}{2}\frac{\mathrm{d}}{\mathrm{d}t}\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|_2^2 +b\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|_2^2 +\frac{c}{2}\frac{\mathrm{d}}{\mathrm{d}t}\left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_2^2 +\frac{c_{\beta}}{4}\frac{\mathrm{d}}{\mathrm{d}t} \left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2 \\ =\left\langle\nu\frac{\partial}{\partial t} \mathbf{Sat} _2(|\mathbf{z}_n(t)|^2) +\dot{g}_t,\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right\rangle_{\mathrm{L}^2} \\ \leq \nu\left|\left\langle\frac{(2+\varepsilon|\mathbf{z}_n(t)|)\mathbf{z}_n(t)}{2(1+\varepsilon|\mathbf{z}_n(t)|)^2} \frac{\partial}{\partial t}\bar{\mathbf{z}}_n(t),\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right\rangle_{\mathrm{L}^2} \right| \\ +\nu\left|\left\langle\frac{(2+\varepsilon|\mathbf{z}_n(t)|)\bar{\mathbf{z}}_n(t)}{2(1+\varepsilon|\mathbf{z}_n(t)|)^2} \frac{\partial}{\partial t}\mathbf{z}_n(t),\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right\rangle_{\mathrm{L}^2} \right|+g_{T_\infty}\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|_2 \\ \leq \frac{2\nu}{\varepsilon}\left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2 \left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right| +g_{T_\infty}\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right| \\ \leq \frac{8\nu^2}{b\varepsilon^2}\left|\frac{\partial}{\partial t}\mathbf{z}_n(t)\right|_2^2 +b\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|^2+\frac{2g_{T_\infty}^2}{b} \\ \leq \frac{8\nu^2}{b\varepsilon^2}M_{\dot{\mathbf{z}}}^T +\frac{2g_{T_\infty}^2}{b}+b\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|^2 \\ :=a_4+b\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|^2,
(2.9)

t\in \bar{I}_T\backslash\{0\} 几乎处处成立, 其中 n\in\mathbf{Z}_+.

定义 \ddot{ \mathbf{w} }_n(0):=\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\Big|_{t=0}, \forall n\in\mathbf{Z}_+. 在 (2.1) 式的第二个方程中依次令 t\rightarrow0, \zeta=\ddot{{w}}_n(0) 可得

\begin{aligned} \left|\ddot{\mathbf{w}}_{n}(0)\right|_{2}^{2} & \leq\left[b\left|\psi_{n}\right|_{2}+c\left|\phi_{n}\right|_{2}+\left|(-\Delta)^{\beta} \phi_{n}\right|_{2}+\nu\left|\mathbf{S a t}_{2}\left(\left|\varphi_{n}\right|^{2}\right)\right|_{2}+g_{T_{\infty}}\right]\left|\ddot{\mathbf{w}}_{n}(0)\right|_{2} \\ & \leq\left[2 b|\psi|_{2}+2 c|\phi|_{2}+2|\phi|_{\beta, 2}+\frac{2 \nu}{\varepsilon}|\varphi|_{2}+g_{T_{\infty}}\right]\left|\ddot{\mathbf{w}}_{n}(0)\right|_{2}, \end{aligned}

其中

\varphi_n=\varphi+\frac{\varphi}{n},\quad \phi_n=\phi+\frac{\phi}{n},\quad \psi_n=\psi+\frac{\psi}{n}, n\in\mathbf{Z}_+.

因此,

|\ddot{ \mathbf{w} }_n(0)|_2\leq 2b|\psi|_2+2c|\phi|_2 +2|\phi|_{\beta,2} +\frac{2\nu}{\varepsilon}|\varphi|_2 +g_{T_\infty}:=a_5,\quad \forall n\in\mathbf{Z}_+.

由 (2.9) 式可知

\left|\frac{\partial^2}{\partial t^2} \mathbf{w} _n(t)\right|_2^2\leq 2a_4T+a_5^2+4c\psi^2+2c_\beta|\psi|_{\mathrm{X}_0^{\beta}}^2:=M_{\ddot{ \mathbf{w} }}^T,\quad \left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2\leq \frac{2M_{\ddot{ \mathbf{w} }}^T}{c_\beta}:=M_{\dot{ \mathbf{w} }_{\beta}}^T,

其中 t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+. 证毕.

2.2 全局弱解

定理1.1 的证明 由引理 2.1 可得

\begin{cases} \{{\mathbf{z}}_n\} \text{ 在 }\mathrm{L}^\infty(I_T,\mathrm{L}^2(\Omega)\cap\mathrm{X}_0^\alpha(\Omega))\text{ 中有界};\\[2mm] \left\{\frac{\partial}{\partial t}{\mathbf{z}}_n\right\} \text{ 在 }\mathrm{L}^\infty(I_T,\mathrm{L}^2(\Omega))\text{ 中有界};\\[2mm] \{{ \mathbf{w} }_n\} \text{ 在 }\mathrm{L}^\infty(I_T,\mathrm{L}^2(\Omega)\cap\mathrm{X}_0^\beta(\Omega))\text{ 中有界};\\[2mm] \left\{\frac{\partial}{\partial t}{ \mathbf{w} }_n\right\} \text{ 在 }\mathrm{L}^\infty(I_T,\mathrm{L}^2(\Omega)\cap\mathrm{X}_0^\beta(\Omega))\text{ 中有界};\\ \left\{\frac{\partial^2}{\partial t^2}{ \mathbf{w} }_n\right\} \text{ 在 }\mathrm{L}^\infty(I_T,\mathrm{L}^2(\Omega))\text{ 中有界}.\end{cases}

因此, 存在 \{({\mathbf{z}}_n,{ \mathbf{w} }_n)\}_{n\in\mathbf{Z}_+} 的一个子列 (仍记为 \{({\mathbf{z}}_n,{ \mathbf{w} }_n)\}_{n\in\mathbf{Z}_+}) 使得当 n\rightarrow\infty 时, 有

\begin{cases} \text{在$\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega)\cap\mathrm{X}_0^\alpha(\Omega))$ 中 }{\mathbf{z}}_n\stackrel{}{\rightharpoonup}{\mathbf{z}}_0;\\[2mm] \text{在 $\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega))$ 中 }\frac{\partial}{\partial t}{\mathbf{z}}_n\stackrel{}{\rightharpoonup}\frac{\partial}{\partial t}{\mathbf{z}}_0;\\[2mm] \text{在$\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega)\cap\mathrm{X}_0^\beta(\Omega))$ 中 }{ \mathbf{w} }_n\stackrel{}{\rightharpoonup}{ \mathbf{w} }_0;\\[2mm] \text{在 $\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega)\cap\mathrm{X}_0^\beta(\Omega))$ 中 }\frac{\partial}{\partial t}{ \mathbf{w} }_n\stackrel{}{\rightharpoonup}\frac{\partial}{\partial t}{ \mathbf{w} }_0;\\ \text{在$\mathrm{L}_{\mathrm{loc}}^2(\mathbf{R}_+,\mathrm{L}^2(\Omega))$ 中 }\frac{\partial^2}{\partial t^2}{ \mathbf{w} }_n \stackrel{}{\rightharpoonup}\frac{\partial^2}{\partial t^2}{ \mathbf{w} }_0.\end{cases}

因为 \mathrm{X}_0^\alpha(\Omega)\hookrightarrow\mathrm{L}^2(\Omega)\mathrm{X}_0^\beta(\Omega)\hookrightarrow\mathrm{L}^2(\Omega) 是紧的, 所以可以选取 \{({\mathbf{z}}_n,{ \mathbf{w} }_n)\}_{n\in\mathbf{Z}_+} 的一个子列 (仍记为 \{({\mathbf{z}}_n,{ \mathbf{w} }_n)\}_{n\in\mathbf{Z}_+}) 使得当 n\rightarrow\infty 时, 在 \mathrm{L}^2(\Omega) 中对每个 t\in\mathbf{R}_+

{\mathbf{z}}_n\rightarrow{\mathbf{z}}_0,\quad { \mathbf{w} }_n\rightarrow{ \mathbf{w} }_0.

由于在 \mathrm{L}^2(\Omega) 中, 当 n\rightarrow\infty 时, 有{z}_n\rightarrow{z}_0. 因此当 n\rightarrow\infty 时, 有

\|{\mathbf{z}}_0(t)\|_{2}\leq\|{\mathbf{z}}_n(t)\|_{2}+\|{\mathbf{z}}_n(t)-{\mathbf{z}}_0(t)\|_{2} \leq \sqrt{M_{{\mathbf{z}}}^T}+\|{\mathbf{z}}_n(t)-{\mathbf{z}}_0(t)\|_{2}\rightarrow \sqrt{M_{{\mathbf{z}}}^T},

\|{\mathbf{z}}_0(t)\|_{2}^2\leq M_{{\mathbf{z}}}^T, \forall t\in\bar{I}_T.

注意到

|\langle {\mathbf{z}}_n(t),{\mathbf{z}}_0(t)\rangle_{\mathrm{X}_0^\alpha}| \leq \|{\mathbf{z}}_n(t)\|_{\mathrm{X}_0^\alpha}\|{\mathbf{z}}_0(t)\|_{\mathrm{X}_0^\alpha}\leq \sqrt{M_{{\mathbf{z}}_\alpha}^T}\|{\mathbf{z}}_0(t)\|_{\mathrm{X}_0^\alpha},\quad n\in\mathbf{Z}_+, t\in\bar{I}_T\backslash\{0\}.

在上述不等式中令 n\rightarrow\infty 可得

\|{\mathbf{z}}_0(t)\|_{\mathrm{X}_0^\alpha}^2\leq M_{{\mathbf{z}}_\alpha}^T,\quad \forall t\in\bar{I}_T.

同理, 有

\|{ \mathbf{w} }_0(t)\|_{2}^2\leq M_{{ \mathbf{w} }}^T,\quad \|{ \mathbf{w} }_0(t)\|_{\mathrm{X}_0^\beta}^2\leq M_{{ \mathbf{w} }_\beta}^T,\quad \forall t\in\bar{I}_T.

由于

\left| \mathbf{Sat} _1(\mathbf{z}_n \mathbf{w} _n)- \mathbf{Sat} _1(\mathbf{z}_0 \mathbf{w} _0)\right| =\bigg|\frac{(\mathbf{z}_n-\mathbf{z}_0) \mathbf{w} _n}{1+\rho|\mathbf{z}_n|+\varrho| \mathbf{w} _n|}+\frac{\mathbf{z}_0( \mathbf{w} _n- \mathbf{w} _0)}{1+\rho|\mathbf{z}_0|+\varrho| \mathbf{w} _0|} \\ +\frac{\mathbf{z}_0 \mathbf{w} _n}{1+\rho|\mathbf{z}_n|+\varrho| \mathbf{w} _n|}-\frac{\mathbf{z}_0 \mathbf{w} _n}{1+\rho|\mathbf{z}_0|+\varrho| \mathbf{w} _0|}\bigg| \\ \leq \frac{2}{\varrho}|\mathbf{z}_n-\mathbf{z}_0|+\frac{2}{\rho}| \mathbf{w} _n- \mathbf{w} _0|,

从而,

\begin{aligned} \Big|\left\langle \mathbf{Sat} _1(\mathbf{z}_n \mathbf{w} _n)- \mathbf{Sat} _1(\mathbf{z}_0 \mathbf{w} _0),\xi\right\rangle_{\mathrm{L}^2}\Big| &\leq&\left|\frac{2}{\varrho} \left\langle|\mathbf{z}_n-\mathbf{z}_0|,|\xi|\right\rangle_{\mathrm{L}^2} \right| +\left|\frac{2}{\rho} \left\langle| \mathbf{w} _n- \mathbf{w} _0|,|\xi|\right\rangle_{\mathrm{L}^2} \right| \\ &\leq&\frac{2}{\varrho} |\mathbf{z}_n-\mathbf{z}_0|_2|\xi|_2 +\frac{2}{\rho} | \mathbf{w} _n- \mathbf{w} _0|_2|\xi|_2, \end{aligned}

\lim\limits_{n\rightarrow\infty}\left\langle \mathbf{Sat} _1(\mathbf{z}_n \mathbf{w} _n)- \mathbf{Sat} _1(\mathbf{z}_0 \mathbf{w} _0),\xi\right\rangle_{\mathrm{L}^2}=0,\quad \forall\xi \in \mathbb{K}_m^\alpha, m\in\mathbf{Z}_+.

注意到 \bigcup\limits_{m=1}^{\infty}\mathbb{K}_m^\alpha \mathrm{L}^2(\Omega) 中稠密, 所以, 当 n\rightarrow\infty 时, 在 \mathrm{L}^2(\Omega) 中有

\mathbf{Sat} _1(\mathbf{z}_n \mathbf{w} _n)\rightharpoonup \mathbf{Sat} _1(\mathbf{z}_0 \mathbf{w} _0).

同理, 当 n\rightarrow\infty 时, 在 \mathrm{L}^2(\Omega) 中有 \mathbf{Sat} _2(|\mathbf{z}_n|^2)\rightharpoonup \mathbf{Sat} _2(|\mathbf{z}_0|^2).

对 (2.1) 式的两边同时取极限, 利用 Lebesgue 控制收敛定理以及 \bigcup\limits_{n=1}^{\infty}\mathbb{K}_n^{\alpha} \bigcup\limits_{n=1}^{\infty}\mathbb{K}_n^{\beta}\mathrm{L}^2(\Omega) 中稠密, 可得

\begin{matrix} \left\{ \begin{array}{lll} \left\langle\mathrm{i}\hbar\frac{\partial}{\partial t}\mathbf{z}_0+ \mathrm{i}a\mathbf{z}_0 + \mu \mathbf{Sat} _1(\mathbf{z}_0 \mathbf{w} _0)-f,\xi\right\rangle_{\mathrm{L}^2} =\frac{1}{2}c_{\alpha}\hbar^2\langle\mathbf{z}_0,\xi\rangle_{\mathrm{X}_0^\alpha},\\ \left\langle\left(\frac{\partial^2}{\partial t^2}+b\frac{\partial}{\partial t}+c\right) \mathbf{w} _0 - \nu \mathbf{Sat} _2(|\mathbf{z}_0|^2)-g,\zeta\right\rangle_{\mathrm{L}^2} +\frac{1}{2}c_{\beta}\langle \mathbf{w} _0,\zeta\rangle_{\mathrm{X}_0^\beta} =0,\\ \mathbf{z}_0(0)=\varphi,\quad \mathbf{w} _0(0)=\phi,\quad \frac{\partial \mathbf{w} _0(t)}{\partial t}\bigg|_{t=0}=\psi, \end{array} \right. \end{matrix}

其中 \xi, \zeta\in\mathrm{L}^2(\Omega), t\in \mathbf{R}_+. 显然, (\mathbf{z}_0, \mathbf{w} _0)\in \mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} } 是方程 (2.1) 的一个全局弱解 (见定义 1.1). 证毕.

3 Fourier 级数, 唯一性和收敛性

3.1 (\mathbf{z}_0, \mathbf{w} _0) 的 Fourier 级数

定义 \mathbf{z}_0(t)=\hat{\mathbf{z}}_0(t)+\mathrm{i}\breve{\mathbf{z}}_0(t), \mathbf{w} _0(t)=\sum\limits_{k=1}^\infty \mathbf{w} _{k,0}(t)e_k^\beta, 其中

\hat{\mathbf{z}}_0(t)=\sum\limits_{k=1}^\infty\hat{\mathbf{z}}_{k,0}(t)e_k^\alpha,\quad \breve{\mathbf{z}}_0(t)=\sum\limits_{k=1}^n\breve{\mathbf{z}}_{k,0}(t)e_k^\alpha,\quad\forall t\in \mathbf{R}_+.

因为在 \mathrm{X}_0^\alpha(\Omega) 中, 当 n\rightarrow\infty 时有 {z}_n\stackrel{}{\rightharpoonup}{z}_0, 所以

\langle \mathbf{z}_0, e_k^\alpha\rangle_{\mathrm{X}_0^\alpha} =\lim\limits_{n\rightarrow\infty}\langle \mathbf{z}_n, e_k^\alpha\rangle_{\mathrm{X}_0^\alpha} =\lambda_k^\alpha\lim\limits_{n\rightarrow\infty}\langle\mathbf{z}_n, e_k^\alpha\rangle_{\mathrm{L}^2} =\lambda_k^\alpha\langle\mathbf{z}_0, e_k^\alpha\rangle_{\mathrm{L}^2},\quad k=1,2,\cdots.

同理, \langle \mathbf{w} _0, e_k^\beta\rangle_{\mathrm{X}_0^\beta} =\lambda_k^\beta\langle \mathbf{w} _0, e_k^\beta\rangle_{\mathrm{L}^2}, \forall k=1,2,\cdots . 因此, 模型 (2.10) 的第一个方程可转化为

\begin{eqnarray*} \left\{ \begin{array}{lll} \left\langle\hbar\frac{\partial}{\partial t}\hat{\mathbf{z}}_0(t),e_k^\alpha\right\rangle_{\mathrm{L}^2}&=& \frac{1}{2}c_{\alpha}\hbar^2\lambda_k^\alpha\langle\breve{\mathbf{z}}_0(t),e_k^\alpha\rangle_{\mathrm{L}^2} -a\langle\hat{\mathbf{z}}_0(t),e_k^\alpha\rangle_{\mathrm{L}^2}\\ && -\mu\langle \widehat{ \mathbf{Sat} }_1(\mathbf{z}_0(t) \mathbf{w} _0(t)),e_k^\alpha\rangle_{\mathrm{L}^2}+\langle\mathrm{Im} f(x,t),e_k^\alpha\rangle_{\mathrm{L}^2},\\ \left\langle\hbar\frac{\partial}{\partial t}\breve{\mathbf{z}}_0(t),e_k^\alpha\right\rangle_{\mathrm{L}^2}&=& -\frac{1}{2}c_{\alpha}\hbar^2\lambda_k^\alpha\langle\hat{\mathbf{z}}_0(t),e_k^\alpha\rangle_{\mathrm{L}^2} -a\langle\breve{\mathbf{z}}_0(t),e_k^\alpha\rangle_{\mathrm{L}^2}\\ && +\mu\langle\widetilde{ \mathbf{Sat} }_1(\mathbf{z}_0(t) \mathbf{w} _0(t)),e_k^\alpha\rangle_{\mathrm{L}^2}-\langle\mathrm{Re} f(x,t),e_k^\alpha\rangle_{\mathrm{L}^2} \end{array} \right. \end{eqnarray*}

等价于

\frac{\mathrm{d}}{\mathrm{d}t}\left[\begin{array}{c}\hat{\mathbf{z}}_{k,0} \\\breve{\mathbf{z}}_{k,0} \\\end{array}\right](t)=\frac{1}{\hbar}\left[\begin{array}{cc}-a & \frac{1}{2}c_{\alpha}\hbar^2\lambda_k^\alpha \\ -\frac{1}{2}c_{\alpha}\hbar^2\lambda_k^\alpha & -a \\\end{array}\right]\left[\begin{array}{c}\hat{\mathbf{z}}_{k,0}\\\breve{\mathbf{z}}_{k,0} \\\end{array}\right](t)+\frac{1}{\hbar}\left[\begin{array}{c}-\mu\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)+\mathrm{Im}f_k \\\mu\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\mathrm{Re}f_k \\\end{array}\right](t),
(3.1)

其中 \hat{\mathbf{z}}_{k,0}(0)=\hat{\varphi}_k, \breve{\mathbf{z}}_{k,0}(0)=\breve{\varphi}_k, t\in \mathbf{R}_+, k=1,2,\cdots .

结合方程 (3.1) 可得

\begin{aligned} {\left[\begin{array}{l} \hat{\mathbf{z}}_{k, 0} \\ \breve{\mathbf{z}}_{k, 0} \end{array}\right](t)=} & e^{-\frac{a}{\hbar} t}\left[\begin{array}{cc} \cos \left(\dot{\lambda}_{k}^{\alpha} t\right) & \sin \left(\dot{\lambda}_{k}^{\alpha} t\right) \\ -\sin \left(\dot{\lambda}_{k}^{\alpha} t\right) & \cos \left(\dot{\lambda}_{k}^{\alpha} t\right) \end{array}\right]\left[\begin{array}{l} \hat{\varphi}_{k} \\ \breve{\varphi}_{k} \end{array}\right]+\frac{1}{\hbar} \int_{0}^{t} e^{-\frac{a}{\hbar}(t-s)} \\ & \times\left[\begin{array}{ll} \cos \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) & \sin \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) \\ \sin \left(\dot{\lambda}_{k}^{\alpha}(s-t)\right) & \cos \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) \end{array}\right]\left[\begin{array}{c} -\mu \widehat{\operatorname{Sat}}_{1, k}\left(\mathbf{z}_{0} \mathbf{w}_{0}\right)+\operatorname{Im} f_{k} \\ \mu \widetilde{\mathbf{S a t}}_{1, k}\left(\mathbf{z}_{0} \mathbf{w}_{0}\right)-\operatorname{Re} f_{k} \end{array}\right](s) \mathrm{d} s, \end{aligned}
(3.2)

其中 t\in \mathbf{R}_0, k=1,2,\cdots . 由式 (3.2), 可知 \mathbf{z}_0=(\hat{\mathbf{z}}_0,\breve{\mathbf{z}}_0) 可以表示为 Fourier 级数 (1.3).

引理3.1 若定理 1.2 的所有假设均成立. 则 \max\limits_{t\in\mathbf{R}_0}|\mathbf{z}_0(t)|_2\leq\mathbf{z}_{\infty}.

考虑部分和

\hat{\mathbf{z}}_0^{n}(t)=\sum\limits_{k=1}^{n}\hat{\mathbf{z}}_{k,0}(t)e_k^\alpha,\quad \breve{\mathbf{z}}_0^{n}(t)=\sum\limits_{k=1}^{n}\breve{\mathbf{z}}_{k,0}(t)e_k^\alpha,\quad t\in\mathbf{R}_+, n=1,2,\cdots.

显然,

\max\limits_{t\in\bar{I}_T}\{|\hat{\mathbf{z}}_0^{n}(t)|_{2}^2,|\breve{\mathbf{z}}_0^{n}(t)|_{2}^2\}\leq M_{\mathbf{z}}^T,

并且在 \{\mathrm{L}^2(\Omega)\}^2 中, \{(\hat{\mathbf{z}}_0^{n}(t),\breve{\mathbf{z}}_0^{n}(t) \}_{n\in\mathbf{Z}_+} 收敛到 (\hat{\mathbf{z}}_0(t),\breve{\mathbf{z}}_0(t) ), \forall t\in \bar{I}_T.

根据式 (1.3)、Minkowski 不等式、Hölder 不等式和 Bessel 不等式, 可得

\begin{aligned} \max\limits_{t\in\bar{I}_T}|\hat{\mathbf{z}}_0^n(t)|_{2}&=&\max\limits_{t\in\bar{I}_T}\Bigg\{\sum\limits_{k=1}^{n}\Bigg\{ e^{-\frac{a}{\hbar}t}\left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha t) \\ \sin(\acute{\lambda}_k^\alpha t) \end{array} \right]^\top \left[ \begin{array}{c} \hat{\varphi}_k\\ \breve{\varphi}_k \\ \end{array} \right] + \frac{1}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \\ &&\times\left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \bigg[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\mathrm{Re}f_k \\ \end{array} \bigg](s)\mathrm{d}s\Bigg\}^2\Bigg\}^{\frac{1}{2}} \\ &\leq&|\varphi|_{2}+\max\limits_{t\in\bar{I}_T}\bigg\{\sum\limits_{k=1}^{n}\bigg\{ \frac{1}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \\ &&\times\left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \bigg[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\mathrm{Re}f_k \\ \end{array} \bigg](s)\mathrm{d}s \bigg\}^2\bigg\}^{\frac{1}{2}} \\ &\leq&|\varphi|_{2} +\frac{1}{\hbar}\max\limits_{t\in\bar{I}_T}\bigg\{\sum\limits_{k=1}^{n}\bigg[\int_{0}^te^{-\frac{a}{\hbar}(t-s)}\mathrm{d}s \int_{0}^te^{-\frac{a}{\hbar}(t-s)} \\ &&\times \bigg( \left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \bigg[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\mathrm{Re}f_k \\ \end{array} \bigg](s) \bigg)^2\mathrm{d}s\bigg]\bigg\}^{\frac{1}{2}} \\ &\leq&|\varphi|_{2} +\frac{1}{a}\Big[\frac{\mu}{\varrho}\max\limits_{t\in\bar{I}_T}|\mathbf{z}_0(t)|_{2}+f_{\infty}\Big]. \end{aligned}

同理,

\max\limits_{t\in\bar{I}_T}|\breve{\mathbf{z}}_0^n(t)|_{2}\leq|\varphi|_{2} +\frac{1}{a}\Big[\frac{\mu}{\varrho}\max\limits_{t\in\bar{I}_T}|\mathbf{z}_0(t)|_{2}+f_{\infty}\Big], \quad \forall n\in\mathbf{Z}_+.

在上述两个不等式中令 n\rightarrow\infty, 则

\max\limits_{t\in\bar{I}_T}|\mathbf{z}_0(t)|_2 \leq \frac{2\varrho(a|\varphi|_{2}+f_{\infty})}{a\varrho-2\mu} =\mathbf{z}_{\infty}.

进而, 令 T\rightarrow\infty, 则 \max\limits_{t\in\mathbf{R}_0}|\mathbf{z}_0(t)|_2\leq\mathbf{z}_{\infty}. 证毕.

由 (2.10) 式的第二个方程可知

\frac{\mathrm{d}^2}{\mathrm{d}t^2} \mathbf{w} _{k,0}(t) +b\frac{\mathrm{d}}{\mathrm{d}t} \mathbf{w} _{k,0}(t) +\frac{1}{2}c_{\beta}\lambda_k^\beta \mathbf{w} _{k,0}(t) +c \mathbf{w} _{k,0}(t)-\nu \mathbf{Sat} _{2,k}(|\mathbf{z}_0(t)|^2)=g_k(t),
(3.3)

其中 \mathbf{w} _{k,0}(0)=\phi_k, \frac{\mathrm{d}}{\mathrm{d}t} \mathbf{w} _{k,0}(t)\Big|_{t=0}=\psi_k, t\in \mathbf{R}_+, k=1,2,\cdots.

结合不等式 (2.2) 计算得到,

\begin{aligned} \frac{\mathrm{d}}{\mathrm{d}t}|\mathbf{z}_n(t)|_2^2&\leq&\frac{2f_\infty^2}{a\hbar} \Rightarrow |\mathbf{z}_n(t)|_2^2\leq 4|\varphi|_2^2+\frac{2f_\infty^2}{a\hbar}t\leq h_0e^{t}, \end{aligned}

其中 h_0:=4|\varphi|_2^2+\frac{2f_\infty^2}{a\hbar}, t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+. 由不等式 (2.3) 可得

\frac{\mathrm{d}}{\mathrm{d}t}\left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_2^2 + \frac{c_{\beta}}{2}\frac{\mathrm{d}}{\mathrm{d}t}\left| \mathbf{w} _n(t)\right|_{\mathrm{X}_0^\beta}^2 +c\frac{\mathrm{d}}{\mathrm{d}t}\left| \mathbf{w} _n(t)\right|_2^2 \leq\frac{4}{b}\Big[\frac{\nu^2}{\varepsilon^2}|\mathbf{z}_n(t)|_{2}^2+g_{\infty}^2\Big],

因此,

\begin{aligned} \left|\frac{\partial}{\partial t} \mathbf{w} _n(t)\right|_2^2 +c\left| \mathbf{w} _n(t)\right|_2^2 &\leq&\frac{4\nu^2h_0}{b\varepsilon^2}\int_{0}^te^{s}\mathrm{d}s+\frac{4g_\infty^2 t}{b} +h_1 \\ &\leq&\left[\frac{4\nu^2h_0}{b\varepsilon^2}+\frac{4g_\infty^2}{b} +h_1\right]e^{t} :=h_2e^{t}, \end{aligned}

其中 h_1:=4\left|\psi\right|_2^2+2c_{\beta}|\phi|_{\mathrm{X}_0^\beta}^2+4c\left|\phi\right|_2^2, h_2:=\frac{4\nu^2h_0}{b\varepsilon^2}+\frac{4g_\infty^2}{b} +h_1, t\in \bar{I}_T\backslash\{0\}, n\in\mathbf{Z}_+. 由于在 \mathrm{L}^2(\Omega) 中, 当 n\rightarrow\infty 时对每个 t\in\mathbf{R}_+ 都有 \mathbf{w} _n\rightarrow \mathbf{w} _0, \frac{\partial}{\partial t} \mathbf{w} _n\rightarrow\frac{\partial}{\partial t} \mathbf{w} _0, 所以

\begin{aligned} \left|\frac{\partial}{\partial t} \mathbf{w} _0(t)\right|_2^2 +c\left| \mathbf{w} _0(t)\right|_2^2 &\leq&h_2e^{t}, \quad \forall t\in\mathbf{R}_+. \end{aligned}
(3.4)

由不等式 (3.4) 可知, \mathbf{w} _{k,0}, \frac{\mathrm{d}}{\mathrm{d}t} \mathbf{w} _{k,0} 是有限增长的. 若 (\mathcal{K}_3) 成立, 对式 (3.3) 两边同时进行 Laplace 变换可得

\begin{aligned} \mathbf{w} _{k,0}(t)&=&e^{-\frac{b}{2}t}\bigg[\cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t)\bigg]\phi_k +\frac{1}{\grave{\lambda}_k^\beta}e^{-\frac{b}{2}t}\sin(\grave{\lambda}_k^\beta t)\psi_k \\ &&+\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \left[\nu \mathbf{Sat} _{2,k}(|\mathbf{z}_0(t)|^2)+g_k(s)\right]\mathrm{d}s, \end{aligned}

其中 t\in \mathbf{R}_0, k=1,2,\cdots . 因此, \mathbf{w} _0 可以表示成 Fourier 级数 (1.4).

引理3.2 设定理 1.2 的所有条件均成立. 则 \max\limits_{t\in\mathbf{R}_0}| \mathbf{w} _0(t)|_{2}\leq \mathbf{w} _{\infty}.

考虑部分和

\mathbf{w} _0^{n}(t)=\sum\limits_{k=1}^{n} \mathbf{w} _{k,0}(t)e_k^\beta,\quad t\in\mathbf{R}_+, n=1,2,\cdots.

显然,

\max\limits_{t\in\bar{I}_T}\{| \mathbf{w} _0^{n}(t)|_{2}^2\}_{n\in\mathbf{Z}_+}\leq M_{\mathbf{z}}^T,

而且在 \mathrm{L}^2(\Omega) 中, \{ \mathbf{w} _0^{n}(t))\}_{n\in\mathbf{Z}_+} 收敛于 \mathbf{w} _0(t), \forall t\in \bar{I}_T. 由方程 (1.4) 可知,

\begin{aligned} \max\limits_{t\in\bar{I}_T}| \mathbf{w} _0^n(t)|_{2} &\leq&\max\limits_{t\in\bar{I}_T}\bigg\{\sum\limits_{k=1}^{n}\bigg\{e^{-\frac{b}{2}t}\bigg[ \cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t) \bigg]\phi_k\bigg\}^2\bigg\}^{\frac{1}{2}} \\ &&+\max\limits_{t\in\bar{I}_T}\bigg\{\sum\limits_{k=1}^{n}\bigg[\frac{1}{\grave{\lambda}_k^\beta} e^{-\frac{b}{2}t}\sin(\grave{\lambda}_k^\beta t)\psi_k\bigg]^2\bigg\}^{\frac{1}{2}} +\max\limits_{t\in\bar{I}_T}\bigg\{\sum\limits_{k=1}^{n}\bigg[ \frac{1}{\grave{\lambda}_k^\beta} \\ &&\times\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \left[\nu \mathbf{Sat} _{2,k}(|\mathbf{z}_0(t)|^2)+g_k(s)\right]\mathrm{d}s \bigg]^2\bigg\}^{\frac{1}{2}} \\ &\leq&\frac{2\grave{\lambda}_1^\beta+b}{2\grave{\lambda}_1^\beta}|\phi|_{2} +\frac{1}{\grave{\lambda}_1^\beta}|\psi|_{2} +\frac{2}{\grave{\lambda}_1^\beta b}\Big[\frac{\nu}{\varepsilon}\max\limits_{t\in\bar{I}_T}|\mathbf{z}_0(t)|_2+g_{\infty}\Big] \\ &\leq&\frac{2\grave{\lambda}_1^\beta+b}{2\grave{\lambda}_1^\beta}|\phi|_{2} +\frac{1}{\grave{\lambda}_1^\beta}|\psi|_{2} +\frac{2}{\grave{\lambda}_1^\beta b}\Big[\frac{\nu}{\varepsilon}\mathbf{z}_\infty+g_{\infty}\Big],\quad \forall n\in\mathbf{Z}_+. \end{aligned}

T 的任意性可知, 结论成立. 证毕.

3.2 定理 1.2 的证明

我们运用反证法来证明唯一性. 设 (\mathbf{z}_*, \mathbf{w} _*)=(\hat{\mathbf{z}}_*,\breve{\mathbf{z}}_*, \mathbf{w} _*)\in\mathrm{C}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) \cap\{\mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} }\} 也是方程 (1.1) 的一个全局弱解. 定义

\hat{\mathbf{z}}_*(t)=\sum\limits_{k=1}^{\infty}\hat{\mathbf{z}}_{k,*}(t)e_k^\alpha,\quad \breve{\mathbf{z}}_*(t)=\sum\limits_{k=1}^{\infty}\breve{\mathbf{z}}_{k,*}(t)e_k^\alpha,\quad \mathbf{w} _*(t)=\sum\limits_{k=1}^{\infty} \mathbf{w} _{k,*}(t)e_k^\beta,

其中 \hat{\mathbf{z}}_{k,*}(t)=\langle\hat{\mathbf{z}}_{*}(t), e_k^\alpha\rangle_{\mathrm{L}^2}, \breve{\mathbf{z}}_{k,*}(t)=\langle\breve{\mathbf{z}}_{*}(t), e_k^\alpha\rangle_{\mathrm{L}^2}, \mathbf{w} _{k,*}(t)=\langle \mathbf{w} _{*}(t), e_k^\beta\rangle_{\mathrm{L}^2}, t\in\mathbf{R}_0, k=1,2,\cdots . 令 \hat{\mathbf{z}}_*^n(t), \breve{\mathbf{z}}_*^n(t), \mathbf{w} _*^n(t) 分别表示 \hat{\mathbf{z}}_*(t), \breve{\mathbf{z}}_*(t), \mathbf{w} _*(t) 的部分和, 其表达式为

\hat{\mathbf{z}}_*^n(t)=\sum\limits_{k=1}^{n}\hat{\mathbf{z}}_{k,*}(t)e_k^\alpha,\quad \breve{\mathbf{z}}_*^n(t)=\sum\limits_{k=1}^{n}\breve{\mathbf{z}}_{k,*}(t)e_k^\alpha,\quad \mathbf{w} _*^n(t)=\sum\limits_{k=1}^{n} \mathbf{w} _{k,*}(t)e_k^\beta,

其中 t\in\mathbf{R}_0, n=1,2,\cdots . 显然, \{(\hat{\mathbf{z}}_*^n,\breve{\mathbf{z}}_*^n, \mathbf{w} _*^n)\}_{n\in\mathbf{Z}_+}\{\mathrm{L}^2(\Omega)\}^3 中收敛到 (\hat{\mathbf{z}}_*,\breve{\mathbf{z}}_*, \mathbf{w} _*), \forall t\in \mathbf{R}_0. 进而, (\hat{\mathbf{z}}_*,\breve{\mathbf{z}}_*, \mathbf{w} _*) 可以表示成相应的 Fourier 形式 (1.3) 和 (1.4). 因此,

\begin{aligned} |\hat{\mathbf{z}}_0^{n}(t)-\hat{\mathbf{z}}_*^{n}(t)|_{2}^2&=&\sum\limits_{k=1}^{n}\big[\hat{\mathbf{z}}_{k,0}^{n}(t)-\hat{\mathbf{z}}_{k,*}^{n}(t)\big]^2 \\ &=&\sum\limits_{k=1}^{n}\bigg\{\frac{\mu}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \\ \end{array} \right]^\top \\ &&\times \bigg[ \begin{array}{c} \widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_* \mathbf{w} _*) \\ \widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_* \mathbf{w} _*) \\ \end{array} \bigg](s)\mathrm{d}s \bigg\}^2 \\ &\leq&\frac{\mu^2}{\hbar^2} \int_{0}^te^{-\frac{a}{\hbar}(t-s)}\mathrm{d}s \int_{0}^te^{-\frac{a}{\hbar}(t-s)} \sum\limits_{k=1}^{n}\bigg\{ \left|\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_* \mathbf{w} _*)\right| \\ && + \left|\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_0 \mathbf{w} _0)-\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_* \mathbf{w} _*)\right| \bigg\}^2(s)\mathrm{d}s \\ &\leq&\frac{32\mu^2}{a\hbar\rho_0^2} \int_{0}^t \bigg[ |\mathbf{z}_0(s)-\mathbf{z}_*(s)|_{2}^2+ | \mathbf{w} _0(s)- \mathbf{w} _*(s)|_{2}^2 \bigg]\mathrm{d}s, \end{aligned}

其中 t\in\mathbf{R}_0, n=1,2,\cdots. 注意到 \langle\cdot\rangle_{\mathrm{L}^2} 关于 |\cdot|_{2} 是连续的, 在上述不等式中令 n\rightarrow\infty, 则

|\hat{\mathbf{z}}_0(t)-\hat{\mathbf{z}}_*(t)|_{2}^2 \leq\frac{32\mu^2}{a\hbar\rho_0^2} \int_{0}^t \bigg[ |\mathbf{z}_0(s)-\mathbf{z}_*(s)|_{2}^2+ | \mathbf{w} _0(s)- \mathbf{w} _*(s)|_{2}^2 \bigg]\mathrm{d}s,\quad \forall t\in\mathbf{R}_0.

同理,

|\breve{\mathbf{z}}_0(t)-\breve{\mathbf{z}}_*(t)|_{2}^2 \leq\frac{32\mu^2}{a\hbar\rho_0^2} \int_{0}^t \bigg[ |\mathbf{z}_0(s)-\mathbf{z}_*(s)|_{2}^2+ | \mathbf{w} _0(s)- \mathbf{w} _*(s)|_{2}^2 \bigg]\mathrm{d}s,\quad \forall t\in\mathbf{R}_0.

所以,

|\mathbf{z}_0(t)-\mathbf{z}_*(t)|_{2}^2 \leq\frac{64\mu^2}{a\hbar\rho_0^2} \int_{0}^t \bigg[ |\mathbf{z}_0(s)-\mathbf{z}_*(s)|_{2}^2+ | \mathbf{w} _0(s)- \mathbf{w} _*(s)|_{2}^2 \bigg]\mathrm{d}s,\quad \forall t\in\mathbf{R}_0.

利用方程 (1.4) 可得,

\begin{aligned} | \mathbf{w} _0^{n}(t)- \mathbf{w} _*^{n}(t)|_{2}^2&=&\sum\limits_{k=1}^{n}\big[ \mathbf{w} _{k,0}^{n}(t)- \mathbf{w} _{k,*}^{n}(t)\big]^2 \\ &=&\sum\limits_{k=1}^{n}\bigg\{\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \\&& \times\left[\nu \mathbf{Sat} _{2,k}(|\mathbf{z}_0|^2)-\nu \mathbf{Sat} _{2,k}(|\mathbf{z}_*|^2)\right](s)\mathrm{d}s \bigg\}^2 \\ &\leq&\frac{2\nu^2}{b(\grave{\lambda}_1^\beta)^2} \int_{0}^te^{-\frac{b}{2}(t-s)} \left| \mathbf{Sat} _2(|\mathbf{z}_0|^2)- \mathbf{Sat} _2(|\mathbf{z}_*|^2)\right|^2(s)\mathrm{d}s \\ &\leq&\frac{9\nu^2}{2\varepsilon^2b(\grave{\lambda}_1^\beta)^2} \int_{0}^t |\mathbf{z}_0(s)-\mathbf{z}_*(s)|_{2}^2\mathrm{d}s,\quad \forall t\in\mathbf{R}_0, n=1,2,\cdots. \end{aligned}

在上述不等式中令 n\rightarrow\infty, 有

| \mathbf{w} _0(t)- \mathbf{w} _*(t)|_{2}^2 \leq\frac{9\nu^2}{2\varepsilon^2b(\grave{\lambda}_1^\beta)^2} \int_{0}^t \bigg[ |\mathbf{z}_0(s)-\mathbf{z}_*(s)|_{2}^2+ | \mathbf{w} _0(s)- \mathbf{w} _*(s)|_{2}^2 \bigg]\mathrm{d}s,\quad \forall t\in\mathbf{R}_0.

定义 \mathcal{U}(t)=|\mathbf{z}_0(t)-\mathbf{z}_*(t)|_{2}^2+| \mathbf{w} _0(t)- \mathbf{w} _*(t)|_{2}^2, \forall t\in\mathbf{R}_0. 则

\mathcal{U}(t) \leq \left\{ \frac{64\mu^2}{a\hbar\rho_0}^2+\frac{9\nu^2}{2\varepsilon^2b(\grave{\lambda}_1^\beta)^2} \right\} \int_{0}^t \mathcal{U}(s)\mathrm{d}s,\quad \forall t\in\mathbf{R}_0.

利用 Gronwall 不等式可知, \mathcal{U}(t)\equiv0, \forall t\in\mathbf{R}_0. 证毕.

3.3 定理 1.3 的证明

(\mathcal{K}_4) 可知, 存在足够小的 \epsilon>0 使得

\min\left\{\frac{a}{\hbar},\frac{b}{2}\right\}>\max\left\{ \frac{64\mu^2(1+\epsilon)}{a \hbar\rho_0^2},\frac{9(1+\epsilon)\nu^2}{2b(\grave{\lambda}_1^\beta)^2\varepsilon^2}\right\}.

(\mathbf{z}_*, \mathbf{w} _*)=(\hat{\mathbf{z}}_*,\breve{\mathbf{z}}_*, \mathbf{w} _*)\in\mathrm{C}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) \cap\{\mathbb{E}_{\mathbf{z}}\times\mathbb{E}_{ \mathbf{w} }\} 也是方程 (1.1) 的一个全局弱解且其初始条件为

\hat{\mathbf{z}}_*(x,0)=\hat{\varphi}_*(x),\quad \breve{\mathbf{z}}_*(x,0)=\breve{\varphi}_*(x),\quad \mathbf{w} _*(x,0)=\phi_*(x),\quad \dot{ \mathbf{w} }_*(x,0)=\psi_*(x),\quad \forall x\in\Omega.\varphi_*=(\hat{\varphi}_*,\breve{\varphi}_*), \hat{\mathbf{z}}_*^n(t), \breve{\mathbf{z}}_*^n(t), \mathbf{w} _*^n(t) 分别表示如上节所述的 \hat{\mathbf{z}}_*(t), \breve{\mathbf{z}}_*(t), \mathbf{w} _*(t) 的部分和, 其中 t\in\mathbf{R}_0, n=1,2,\cdots . 而且, \{(\hat{\mathbf{z}}_*^n,\breve{\mathbf{z}}_*^n, \mathbf{w} _*^n)\}_{n\in\mathbf{Z}_+}\{\mathrm{L}^2(\Omega)\}^3 中收敛于 (\hat{\mathbf{z}}_*,\breve{\mathbf{z}}_*, \mathbf{w} _*), \forall t\in \mathbf{R}_0, (\hat{\mathbf{z}}_*,\breve{\mathbf{z}}_*, \mathbf{w} _*) 可以用相应的 Fourier 级数 (1.3) 和 (1.4) 来表示. 因此,

\begin{aligned} |\hat{\mathbf{z}}_0^{n}(t)-\hat{\mathbf{z}}_*^{n}(t)|_{2}^2 &\leq&(1+\epsilon^{-1})e^{-\frac{2a}{\hbar}t} |\varphi-\varphi_*|_2^2 \\ &&+ \sum\limits_{k=1}^{n}(1+\epsilon)\bigg\{\frac{\mu}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \\ && \times\bigg[ \begin{array}{c} -\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_{0} \mathbf{w} _{0})+\widehat{ \mathbf{Sat} }_{1,k}(\mathbf{z}_{*} \mathbf{w} _{*}) \\ \widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_{0} \mathbf{w} _{0})-\widetilde{ \mathbf{Sat} }_{1,k}(\mathbf{z}_{*} \mathbf{w} _{*}) \\ \end{array} \bigg](s)\mathrm{d}s\bigg\}^2 \\ &\leq&(1+\epsilon^{-1})e^{-\frac{2a}{\hbar}t} |\varphi-\varphi_*|_2^2 \\ &&+ \frac{(1+\epsilon)\mu^2}{a\hbar} \int_{0}^te^{-\frac{a}{\hbar}(t-s)}\Big| \widehat{ \mathbf{Sat} }_{1}(\mathbf{z}_{0} \mathbf{w} _{0})-\widehat{ \mathbf{Sat} }_{1}(\mathbf{z}_{*} \mathbf{w} _{*}) \Big|_2^2\mathrm{d}s \\ &&+\frac{(1+\epsilon)\mu^2}{a\hbar} \int_{0}^te^{-\frac{a}{\hbar}(t-s)}\Big| \widetilde{ \mathbf{Sat} }_{1}(\mathbf{z}_{0} \mathbf{w} _{0})-\widetilde{ \mathbf{Sat} }_{1}(\mathbf{z}_{*} \mathbf{w} _{*}) \Big|_2^2\mathrm{d}s \\ &\leq&(1+\epsilon^{-1})e^{-\frac{2a}{\hbar}t} |\varphi-\varphi_*|_2^2+\frac{16\mu^2(1+\epsilon)}{a \hbar\rho_0^2} \\ &&\times\int_{0}^te^{-\frac{a}{\hbar}(t-s)}\left[\big|\mathbf{z}_{0}(s)-\mathbf{z}_{*}(s)\big|_{2}^2 +\big| \mathbf{w} _{0}(s)- \mathbf{w} _{*}(s)\big|_{2}^2\right]\mathrm{d}s. \end{aligned}

在上述不等式中令 n\rightarrow\infty, 结合 Bohr 不等式

(a+b)^2\leq (1+\epsilon^{-1})a^2+(1+\epsilon)b^2,\quad \forall\epsilon>0, a,b\in\mathbf{R}

可得

\begin{aligned} |\hat{\mathbf{z}}_0(t)-\hat{\mathbf{z}}_*(t)|_{2}^2 &\leq&(1+\epsilon^{-1})e^{-\frac{2a}{\hbar}t} |\varphi-\varphi_*|_2^2+\frac{16\mu^2(1+\epsilon)}{a \hbar\rho_0^2} \\ &&\times\int_{0}^te^{-\frac{a}{\hbar}(t-s)}\left[\big|\mathbf{z}_{0}(s)-\mathbf{z}_{*}(s)\big|_{2}^2 +\big| \mathbf{w} _{0}(s)- \mathbf{w} _{*}(s)\big|_{2}^2\right]\mathrm{d}s,\quad \forall t\in\mathbf{R}_0. \end{aligned}

同理,

\begin{aligned} |\breve{\mathbf{z}}_0(t)-\breve{\mathbf{z}}_*(t)|_{2}^2 &\leq&(1+\epsilon^{-1})e^{-\frac{2a}{\hbar}t} |\varphi-\varphi_*|_2^2+\frac{16\mu^2(1+\epsilon)}{a \hbar\rho_0^2} \\ &&\times\int_{0}^te^{-\frac{a}{\hbar}(t-s)}\left[ \big|\mathbf{z}_{0}(s)-\mathbf{z}_{*}(s)\big|_{2}^2 +\big| \mathbf{w} _{0}(s)- \mathbf{w} _{*}(s)\big|_{2}^2\right]\mathrm{d}s,\quad \forall t\in\mathbf{R}_0. \end{aligned}

所以,

\begin{aligned} |\mathbf{z}_0(t)-\mathbf{z}_*(t)|_{2}^2 &\leq&2(1+\epsilon^{-1})e^{-\frac{2a}{\hbar}t} |\varphi-\varphi_*|_2^2+\frac{32\mu^2(1+\epsilon)}{a \hbar\rho_0^2} \\ &&\times\int_{0}^te^{-\frac{a}{\hbar}(t-s)}\left[\big|\mathbf{z}_{0}(s)-\mathbf{z}_{*}(s)\big|_{2}^2 +\big| \mathbf{w} _{0}(s)- \mathbf{w} _{*}(s)\big|_{2}^2\right]\mathrm{d}s,\ \forall t\in\mathbf{R}_0. \end{aligned}

另一方面, 由方程 (1.4) 可知,

\begin{aligned} | \mathbf{w} _0^{n}(t)- \mathbf{w} _*^{n}(t)|_{2}^2 &\leq&2(1+\epsilon^{-1})\left(1+\frac{b}{2\grave{\lambda}_1^\beta}\right)^2 |\phi-\phi_*|_2^2e^{-bt} +2(1+\epsilon^{-1})\frac{1}{(\grave{\lambda}_1^\beta)^2} |\psi-\psi_*|_2^2e^{-bt} \\ &&+ \sum\limits_{k=1}^{n}(1+\epsilon)\bigg[ \frac{\nu}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \\ &&\times \left[ \mathbf{Sat} _{2,k}(|\mathbf{z}_{0}(s)|^2)- \mathbf{Sat} _{2,k}(|\mathbf{z}_{*}(s)|^2)\right]\mathrm{d}s\bigg]^2 \\ &\leq&2(1+\epsilon^{-1})\left(1+\frac{b}{2\grave{\lambda}_1^\beta}\right)^2 |\phi-\phi_*|_2^2e^{-bt} +2(1+\epsilon^{-1})\frac{1}{(\grave{\lambda}_1^\beta)^2} |\psi-\psi_*|_2^2e^{-bt} \\ &&+ \frac{2(1+\epsilon)\nu^2}{b(\grave{\lambda}_1^\beta)^2} \int_{0}^te^{-\frac{b}{2}(t-s)}\Big| \mathbf{Sat} _{2}(|\mathbf{z}_{0}(s)|^2)- \mathbf{Sat} _{2}(|\mathbf{z}_{*}(s)|^2) \Big|_2^2\mathrm{d}s \\ &\leq&2(1+\epsilon^{-1})\left(1+\frac{b}{2\grave{\lambda}_1^\beta}\right)^2 |\phi-\phi_*|_2^2e^{-bt} +2(1+\epsilon^{-1})\frac{1}{(\grave{\lambda}_1^\beta)^2} |\psi-\psi_*|_2^2e^{-bt} \\ &&+\frac{9(1+\epsilon)\nu^2}{2b(\grave{\lambda}_1^\beta)^2\varepsilon^2} \int_{0}^te^{-\frac{b}{2}(t-s)}\big|\mathbf{z}_{0}(s)-\mathbf{z}_{*}(s)\big|_{2}^2\mathrm{d}s. \end{aligned}

在上述不等式在令 n\rightarrow\infty 可得

\begin{aligned} | \mathbf{w} _0(t)- \mathbf{w} _*(t)|_{2}^2 &\leq&2(1+\epsilon^{-1})\left(1+\frac{b}{2\grave{\lambda}_1^\beta}\right)^2 |\phi-\phi_*|_2^2e^{-bt} +2(1+\epsilon^{-1})\frac{1}{(\grave{\lambda}_1^\beta)^2} |\psi-\psi_*|_2^2e^{-bt} \\ &&+\frac{9(1+\epsilon)\nu^2}{2b(\grave{\lambda}_1^\beta)^2\varepsilon^2} \int_{0}^te^{-\frac{b}{2}(t-s)}|\mathbf{z}_{0}(s)-\mathbf{z}_{*}(s)|_{2}^2\mathrm{d}s,\quad \forall t\in\mathbf{R}_0. \end{aligned}

定义

\mathcal{V}(t)=\max\left\{\big|\mathbf{z}_{0}(t)-\mathbf{z}_{*}(t)\big|_{2}^2, \big| \mathbf{w} _{0}(t)- \mathbf{w} _{*}(t)\big|_{2}^2\right\},\quad \forall t\in \mathbf{R}_0.

结合不等式 (3.5) 和 (3.6) 可得,

\mathcal{V}(t)\leq \sigma_1 e^{-\varpi t}+\sigma_2\int_{0}^te^{-\varpi(t-s)}\mathcal{V}(s)\mathrm{d}s, \quad\forall t\in \mathbf{R}_0,

其中

\sigma_1:=\max\bigg\{2(1+\epsilon^{-1}) |\varphi-\varphi_*|_2^2, 2(1+\epsilon^{-1})\bigg(1+\frac{b}{2\grave{\lambda}_1^\beta}\bigg)^2 |\phi\!-\!\phi_*|_2^2\!+\! 2(1+\epsilon^{-1})\frac{1}{(\grave{\lambda}_1^\beta)^2} |\psi\!-\!\psi_*|_2^2\bigg\},
\sigma_2:=\max\left\{ \frac{64\mu^2(1+\epsilon)}{a \hbar\rho_0^2},\frac{9(1+\epsilon)\nu^2}{2b(\grave{\lambda}_1^\beta)^2\varepsilon^2}\right\},\quad \varpi=\min\left\{\frac{a}{\hbar},\frac{b}{2}\right\}.

由文献 [引理 13] 可得

\mathcal{V}(t)\leq \sigma_1e^{-(\varpi-\sigma_2)t}\rightarrow0 (t\rightarrow\infty).

证毕.

4 概自守弱解

这里我们介绍概自守向量值函数的概念, 详情请参阅文献 [30].

假设 \mathbb{H} 表示某个 Hilbert 空间. 如果对于每一个序列 \{\bar{t}_p\}_{p\in\mathbf{Z}_+}, 都存在一个子序列 \{t_p\}_{p\in\mathbf{Z}_+}\subseteq\{\bar{t}_p\}_{p\in\mathbf{Z}_+} 和一个函数 \tilde{f}:\mathbf{R}\rightarrow\mathbb{H} 使得对任意的 t\in\mathbf{R}, 在 \mathbb{H} 中有

\tilde{f}(t)=\lim\limits_{p\rightarrow\infty}f(t+t_p),\quad \lim\limits_{p\rightarrow\infty}\tilde{f}(t-t_p)=f(t),

则称 \mathbb{H}-值函数 f\in\mathrm{C}(\mathbf{R},\mathbb{H}) 为概自守函数. 所有这些函数的集合用 \mathbb{AA}(\mathbf{R},\mathbb{H}) 表示. 设 \mathbb{B}\subseteq\mathbb{H} 为任意有界集. 如果映射 f=f(\eta,t):\mathbb{H}\times\mathbf{R}\rightarrow \mathbb{H}, \forall(\eta,t)\in \mathbb{H}\times\mathbf{R} 关于变量 t 是概自守的, 对 \eta\in\mathbb{B} 是一致的, 则称映射 f=f(\eta,t) 关于变量 t 是概自守的. 这类映射的集合记为 \mathbb{AA}(\mathbb{H}\times\mathbf{R},\mathbb{H}).

\aleph(\mathbf{R}_0,\mathbb{H})=\{\mathbf{h}\in\mathrm{C}(\mathbf{R}_0,\mathbb{H}): \lim\limits_{t\rightarrow\infty}\|\mathbf{h}(t)\|_{\mathbb{H}}=0\}. 若存在 \mathbf{f}\in \mathbb{AA}(\mathbf{R},\mathbb{H})\mathbf{h}\in \aleph(\mathbf{R}_0, \mathbb{H}) 满足 f=\mathbf{f}+\mathbf{h}, 则称 \mathbb{H}-值连续函数 f:\mathbf{R}_0\rightarrow \mathbb{H} 为渐近概自守函数. 所有这些函数组成的集合用 \mathbb{AAA}(\mathbf{R}_0,\mathbb{H})表示. 特别地, 若 \mathbb{H} 是 Banach 空间, 则 \mathbb{AAA}(\mathbf{R}_0,\mathbb{H}) 也是 Banach 空间, 其范数为 \|f\|_{\mathbb{AAA}}=\sup\limits_{t\in\mathbf{R}}\|\mathbf{f}\|_{\mathbb{H}}+\sup\limits_{t\in\mathbf{R}_0}\|\mathbf{h}\|_{\mathbb{H}}, 其中 f=\mathbf{f}+\mathbf{h}\in \mathbb{AAA}(\mathbf{R}_0,\mathbb{H}), \mathbf{f}\in \mathbb{AA}(\mathbf{R},\mathbb{H}), \mathbf{h}\in \aleph(\mathbf{R}_0, \mathbb{H}).

设连续函数 \mathbf{h}:\mathbb{H}\times\mathbf{R}_0\rightarrow\mathbb{H} 对所有的 \eta\in\mathbb{B} 满足 \lim\limits_{t\rightarrow\infty}\|\mathbf{h}(\eta,t)\|_{\mathbb{H}}=0. 所有这类函数组成的集合用 \aleph(\mathbb{H}\times\mathbf{R}_0, \mathbb{H}) 表示. 若函数 f=f(\eta,t):\mathbb{H}\times\mathbf{R}_0\rightarrow \mathbb{H}, \forall(\eta,t)\in \mathbb{H}\times\mathbf{R}_0 对任意的 \eta\in\mathbb{B} 关于变量 t 是渐近概自守的, 则称函数 f=f(\eta,t) 关于变量 t 是渐近概自守的. 即 f=\mathbf{f}+\mathbf{h}, 其中主项 \mathbf{f}\in\mathbb{AA}(\mathbb{H}\times\mathbf{R},\mathbb{H}), \mathbf{h}\in \aleph(\mathbb{H}\times\mathbf{R}_0, \mathbb{H}). 这类函数用 \mathbb{AAA}(\mathbb{X}\times\mathbf{R}_0,\mathbb{X}) 表示.

4.1 Picard 序列

本节我们将使用 Picard 迭代方法. 基于式 (1.3) 和 (1.4), 构造一个 Picard 迭代序列 (\delta_m,\eta_m) =(\hat{\delta}_m,\breve{\delta}_m,\eta_m)\in\{\mathrm{L}^2(\Omega)\}^3, 如下所示

\begin{matrix}\label{px1} \left\{ \begin{array}{lll} \left[ \begin{array}{c} \hat{\delta}_{0} \\ \breve{\delta}_{0} \\ \end{array} \right](t)&=&\left[ \begin{array}{c} \hat{\varphi} \\ \breve{\varphi} \\ \end{array} \right]\in \left[\{\mathrm{L}^2(\Omega)\}^2\right]^\top,\\[6mm] \left[ \begin{array}{c} \hat{\delta}_{m} \\ \breve{\delta}_{m} \\ \end{array} \right](t) &=& \sum\limits_{k=1}^\infty\Bigg\{ e^{-\frac{a}{\hbar}t}\left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha t) & \sin(\acute{\lambda}_k^\alpha t) \\ -\sin(\acute{\lambda}_k^\alpha t) & \cos(\acute{\lambda}_k^\alpha t) \\ \end{array} \right] \left[ \begin{array}{c} \hat{\varphi}_k\\ \breve{\varphi}_k \\ \end{array} \right] \\[5mm] && + \frac{1}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) & \sin(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (s-t)) & \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \end{array} \right] \\[5mm] && \times\left[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})-\mathrm{Re}f_k \\ \end{array} \right](s)\mathrm{d}s\Bigg\}e_k^\alpha, \end{array} \right. \end{matrix}
(4.1)
\begin{matrix}\label{px2} \left\{ \begin{array}{lll} \eta_{0}(t)&=&\phi\in \mathrm{L}^2(\Omega), \\[2mm] \eta_{m}(t)&=& \sum\limits_{k=1}^\infty\Bigg\{e^{-\frac{b}{2}t}\left[ \cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t) \right]\phi_k + \frac{1}{\grave{\lambda}_k^\beta}e^{-\frac{b}{2}t}\sin(\grave{\lambda}_k^\beta t)\psi_k\\[5mm] && +\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \left[\nu \mathbf{Sat} _{2,k}(|\delta_{m-1}(s)|^2)+g_k(s)\right]\mathrm{d}s\Bigg\}e_k^\beta, \end{array} \right. \end{matrix}
(4.2)

其中 k=1,2,\cdots , m=1,2,\cdots, t\in\mathbf{R}_0.

定义 |\delta_m|_2=\sqrt{|\hat{\delta}_m|_2^2+|\breve{\delta}_m|_2^2}, \forall m=0,1,\cdots .

命题4.1 设定理 1.4 的所有条件都成立. 则 \{(\delta_m,\eta_m)=(\hat{\delta}_m,\breve{\delta}_m,\eta_m): m=1,2,\cdots \}\{\mathrm{L}^2(\Omega)\}^3 中是有定义的并且是 \mathrm{L}^2-连续的.

结合方程 (4.1), 利用 Minkowski 不等式和 Hölder 不等式可得,

\begin{aligned} |\hat{\delta}_1(t)|_2^2 &=&\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\Bigg\{ e^{-\frac{a}{\hbar}t}\left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha t) \\ \sin(\acute{\lambda}_k^\alpha t) \end{array} \right]^\top \left[ \begin{array}{c} \hat{\varphi}_k\\ \breve{\varphi}_k \\ \end{array} \right] \\ &&+ \frac{1}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \left[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\delta_{0}\eta_{0})+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{0}\eta_{0})-\mathrm{Re}f_k \\ \end{array} \right](s)\mathrm{d}s\Bigg\}^2 \\ &\leq&\lim\limits_{n\rightarrow\infty}\bigg\{e^{-\frac{a}{\hbar}t}|\varphi|_{2} + \frac{\mu}{\hbar}\bigg[ \int_{0}^{t}e^{-\frac{a}{\hbar}(t-s)}\mathrm{d}s \\ &&\times\int_{0}^{t}e^{-\frac{a}{\hbar}(t-s)} \sum\limits_{k=1}^{n}\Big( \widehat{ \mathbf{Sat} }_{1,k}^2(\delta_{0}\eta_{0}) + \widetilde{ \mathbf{Sat} }_{1,k}^2(\delta_{0}\eta_{0}) \Big)\mathrm{d}s\bigg]^{\frac{1}{2}} \\ &&+ \frac{1}{\hbar}\bigg[ \int_{0}^{t}e^{-\frac{a}{\hbar}(t-s)}\mathrm{d}s\int_{0}^{t}e^{-\frac{a}{\hbar}(t-s)}\sum\limits_{k=1}^{n}\Big( \mathrm{Im}f_k^2 + \mathrm{Re}f_k^2 \Big)(s)\mathrm{d}s\bigg]^{\frac{1}{2}} \bigg\}^2 \\ &\leq&\bigg( |\varphi|_{2}+\frac{\mu}{a\varrho}|\varphi|_{2}+\frac{1}{a}f_\infty \bigg)^2,\quad \forall t\in\mathbf{R}_0. \end{aligned}

同理,

|\breve{\delta}_1(t)|_2^2\leq\bigg( |\varphi|_{2}+\frac{\mu}{a\varrho}|\varphi|_{2}+\frac{1}{a}f_\infty \bigg)^2,\quad \forall t\in\mathbf{R}_0.

所以,

|\delta_1(t)|_2^2\leq2\bigg( |\varphi|_{2}+\frac{\mu}{a\varrho}|\varphi|_{2}+\frac{1}{a}f_\infty \bigg)^2,\quad \forall t\in\mathbf{R}_0.

另一方面, 有

\begin{aligned} |\hat{\delta}_2(t)|_2^2 &=&\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\Bigg\{ e^{-\frac{a}{\hbar}t}\left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha t) \\ \sin(\acute{\lambda}_k^\alpha t) \end{array} \right]^\top \left[ \begin{array}{c} \hat{\varphi}_k\\ \breve{\varphi}_k \\ \end{array} \right] \\ &&+ \frac{1}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \left[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\delta_{1}\eta_{1})+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{1}\eta_{1})-\mathrm{Re}f_k \\ \end{array} \right](s)\mathrm{d}s\Bigg\}^2 \\ &\leq&\bigg[|\varphi|_{2}+ \frac{\mu\sup\limits_{t\in\mathbf{R}_0}|\delta_1(t)|_{2}}{a\varrho} +\frac{f_\infty}{a} \bigg]^2 \\ &\leq&\bigg\{ |\varphi|_{2}\bigg[ 1+\frac{\sqrt{2}\mu}{a\varrho} +\bigg(\frac{\sqrt{2}\mu}{a\varrho}\bigg)^2 \bigg]+\frac{f_\infty}{a}\bigg( 1+\frac{\sqrt{2}\mu}{a\varrho} \bigg) \bigg\}^2,\quad \forall t\in\mathbf{R}_0. \end{aligned}

同理,

|\breve{\delta}_2(t)|_2^2\leq \bigg\{ |\varphi|_{2}\bigg[ 1+\frac{\sqrt{2}\mu}{a\varrho} +\bigg(\frac{\sqrt{2}\mu}{a\varrho}\bigg)^2 \bigg]+\frac{f_\infty}{a}\bigg( 1+\frac{\sqrt{2}\mu}{a\varrho}\bigg)\bigg\}^2,
|\delta_2(t)|_2^2\leq 2\bigg\{ |\varphi|_{2}\bigg[ 1+\frac{\sqrt{2}\mu}{a\varrho} +\bigg(\frac{\sqrt{2}\mu}{a\varrho}\bigg)^2 \bigg]+\frac{f_\infty}{a}\bigg( 1+\frac{\sqrt{2}\mu}{a\varrho}\bigg)\bigg\}^2, \quad\forall t\in\mathbf{R}_0.

通过数学归纳法可得,

|\delta_m(t)|_2^2\leq 2\bigg\{ |\varphi|_{2}\sum\limits_{k=0}^{m}\bigg(\frac{\sqrt{2}\mu}{a\varrho}\bigg)^{k} +\frac{f_\infty}{a}\sum\limits_{k=0}^{m-1}\bigg(\frac{\sqrt{2}\mu}{a\varrho}\bigg)^{k} \bigg\}^2\leq2\bigg[ \frac{a\varrho|\varphi|_{2}+\varrho f_\infty}{a\varrho-\sqrt{2}\mu} \bigg]^2:=\delta_\infty^2,

其中 t\in\mathbf{R}_0, m=3,4,\cdots. 因此, \delta_m=(\hat{\delta}_m,\breve{\delta}_m)\in\{\mathrm{L}^2(\Omega)\}^2(m=1,2,\cdots ) 是有定义的.

另一方面, 基于方程 (4.2) 可知

\begin{aligned} |\eta_m(t)|_2^2 &=&\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\Bigg\{ e^{-\frac{b}{2}t}\bigg[\cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t)\bigg]\phi_k +\frac{e^{-\frac{b}{2}t}}{\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t)\psi_k\\ &&+\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \left[\nu \mathbf{Sat} _{2,k}(|\delta_{m-1}(s)|^2)+g_k(s)\right]\mathrm{d}s\Bigg\}^2 \\ &\leq&\lim\limits_{n\rightarrow\infty}\bigg\{e^{-\frac{b}{2}t}\bigg[\sum\limits_{k=1}^{n}\bigg[ \cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t) \bigg]^2\phi_k^2\bigg]^{\frac{1}{2}} \\&&+\frac{e^{-\frac{b}{2}t}}{\grave{\lambda}_1^\beta}\bigg[\sum\limits_{k=1}^{n}\psi_k^2\bigg]^{\frac{1}{2}} +\bigg[\sum\limits_{k=1}^{n}\bigg[\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^{t}e^{-\frac{b}{2}(t-s)} \nu \mathbf{Sat} _{2,k}(|\delta_{m-1}(s)|^2)\mathrm{d}s\bigg]^2\bigg]^{\frac{1}{2}} \\&&+\bigg[\sum\limits_{k=1}^{n} \bigg[\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^{t}e^{-\frac{b}{2}(t-s)} g_k(s)\mathrm{d}s\bigg]^2\bigg]^{\frac{1}{2}}\bigg\}^2 \\ &\leq&\lim\limits_{n\rightarrow\infty}\bigg\{\frac{e^{-\frac{b}{2}t}(2\grave{\lambda}_1^\beta+b)}{2\grave{\lambda}_1^\beta}|\phi|_2 +\frac{1}{\grave{\lambda}_1^\beta}|\psi|_2 \\ &&+\frac{1}{\grave{\lambda}_1^\beta}\bigg[ \int_{0}^{t}e^{-\frac{b}{2}(t-s)}\mathrm{d}s\int_{0}^{t}e^{-\frac{b}{2}(t-s)} \sum\limits_{k=1}^{n}\nu^2 \mathbf{Sat} _{2,k}^2(|\delta_{m-1}(s)|^2)\mathrm{d}s\bigg]^{\frac{1}{2}} \\ &&+\frac{1}{\grave{\lambda}_1^\beta}\bigg[ \int_{0}^{t}e^{-\frac{b}{2}(t-s)}\mathrm{d}s\int_{0}^{t}e^{-\frac{b}{2}(t-s)}\sum\limits_{k=1}^{n} g_k^2(s)\mathrm{d}s\bigg]^{\frac{1}{2}}\bigg\}^2 \\ &\leq&\bigg[\frac{(2\grave{\lambda}_1^\beta+b)}{2\grave{\lambda}_1^\beta}|\phi|_2 +\frac{1}{\grave{\lambda}_1^\beta}|\psi|_2 +\frac{2\nu}{\grave{\lambda}_1^\beta b\varepsilon}\delta_\infty +\frac{2}{\grave{\lambda}_1^\beta b}g_\infty \bigg]^2:=\eta_\infty, \end{aligned}

其中 t\in\mathbf{R}_0, m=1,2,\cdots . 因此, \{\eta_m:m=1,2,\cdots \}\subseteq\mathrm{L}^2(\Omega) 是有定义的.

对任意的 \epsilon\in(0,1), 取任意的 t_0, t_1\in\mathbf{R}_0 满足 t_1\geq t_0 以及

\max\bigg\{\bigg[1-e^{-\frac{a}{\hbar}(t_1-t_0)}\bigg]^2, \bigg[1-e^{-\frac{a}{\hbar}(t_1-t_0)} +e^{-\frac{a}{\hbar}t_1}-e^{-\frac{a}{\hbar}t_0}\bigg]^2\bigg\} <\frac{a^2\varrho^2\epsilon^2}{4\mu^2\delta_\infty^2},
\max\bigg\{\bigg[1-e^{-\frac{b}{2}(t_1-t_0)}\bigg]^2, \bigg[1-e^{-\frac{b}{2}(t_1-t_0)} +e^{-\frac{b}{2}t_1}-e^{-\frac{b}{2}t_0}\bigg]^2\bigg\} <\frac{(\grave{\lambda}_k^\beta)^2\varepsilon^2b^2\epsilon^2}{16\nu^2\delta_\infty^2}.

利用迭代序列 (4.1) 和 Hölder 不等式, 直接计算得到

\begin{aligned} |\hat{\delta}_m(t_1)-\hat{\delta}_m(t_0)|_2^2 &=&\frac{1}{\hbar^2}\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\bigg\{ \int_{0}^{t_1} e^{-\frac{a}{\hbar}(t_1-s)} \bigg[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t_1-s)) \\ \sin(\acute{\lambda}_k^\alpha (t_1-s)) \end{array} \bigg]^\top \\&&\times \bigg[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})\\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})\\ \end{array} \bigg](s)\mathrm{d}s-\int_{0}^{t_0} e^{-\frac{a}{\hbar}(t_0-s)} \\&&\times\bigg[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t_0-s)) \\ \sin(\acute{\lambda}_k^\alpha (t_0-s)) \end{array} \bigg]^\top \bigg[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})\\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})\\ \end{array} \bigg](s)\mathrm{d}s\bigg\}^2 \\ &\leq&\frac{2}{\hbar^2}\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\bigg[ \int_{t_0}^{t_1} e^{-\frac{a}{\hbar}(t_1-s)} \bigg[ \begin{array}{c} 1 \\ 1 \end{array} \bigg]^\top \bigg[ \begin{array}{c} \mu|\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})|\\ \mu|\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})|\\ \end{array} \bigg](s) \mathrm{d}s\bigg]^2 \\ &&+\frac{2}{\hbar^2}\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\bigg[\int_{0}^{t_0}\bigg[e^{-\frac{a}{\hbar}(t_0-s)} -e^{-\frac{a}{\hbar}(t_1-s)}\bigg] \bigg[ \begin{array}{c} 1 \\ 1 \end{array} \bigg]^\top \\&&\times \bigg[ \begin{array}{c} \mu|\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})|\\ \mu|\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})|\\ \end{array} \bigg](s) \mathrm{d}s\bigg]^2 \\ &\leq&\frac{2\mu^2}{\hbar^2\varrho^2} \int_{t_0}^{t_1}e^{-\frac{a}{\hbar}(t_1-s)}\mathrm{d}s \int_{t_0}^{t_1}e^{-\frac{a}{\hbar}(t_1-s)}|\delta_{m-1}(s)|_2^2\mathrm{d}s +\frac{2\mu^2}{\hbar^2\varrho^2}\int_{0}^{t_0} \\ &&\times\bigg[e^{-\frac{a}{\hbar}(t_0-s)} -e^{-\frac{a}{\hbar}(t_1-s)}\bigg]\mathrm{d}s\int_{0}^{t_0} \bigg[e^{-\frac{a}{\hbar}(t_0-s)} -e^{-\frac{a}{\hbar}(t_1-s)}\bigg]|\delta_{m-1}(s)|_2^2\mathrm{d}s \\ &\leq&\frac{2\mu^2\delta_\infty^2}{a^2\varrho^2} \bigg[1-e^{-\frac{a}{\hbar}(t_1-t_0)}\bigg]^2 +\frac{2\mu^2\delta_\infty^2}{a^2\varrho^2}\bigg[1-e^{-\frac{a}{\hbar}(t_1-t_0)} +e^{-\frac{a}{\hbar}t_1}-e^{-\frac{a}{\hbar}t_0}\bigg]^2 \\ &\leq&\epsilon^2,\quad \forall m=1,2,\cdots. \end{aligned}

同理, |\breve{\delta}_m(t_1)-\breve{\delta}_m(t_0)|_2^2\leq \epsilon^2, \forall m=1,2,\cdots .

类似地, 结合方程 (4.2) 可得

\begin{aligned} |\eta_m(t_1)-\eta_m(t_0)|_2^2 &=&\frac{\nu^2}{(\grave{\lambda}_1^\beta)^2}\lim\limits_{n\rightarrow\infty}\sum\limits_{k=1}^{n}\bigg\{ \int_{0}^{t_1}e^{-\frac{b}{2}(t_1-s)}\sin(\grave{\lambda}_k^\beta(t_1-s)) \mathbf{Sat} _{2,k}(|\delta_m(s)|^2)\mathrm{d}s \\&&-\int_{0}^{t_0} e^{-\frac{b}{2}(t_0-s)}\sin(\grave{\lambda}_k^\beta(t_0-s)) \mathbf{Sat} _{2,k}(|\delta_m(s)|^2)\mathrm{d}s\bigg\}^2 \\ &\leq&\frac{8\nu^2\delta_\infty^2}{(\grave{\lambda}_1^\beta)^2\varepsilon^2b^2}\bigg\{ \bigg[1-e^{-\frac{b}{2}(t_1-t_0)}\bigg]^2 +\bigg[1-e^{-\frac{b}{2}(t_1-t_0)} +e^{-\frac{b}{2}t_1}-e^{-\frac{b}{2}t_0}\bigg]^2\bigg\} \\ &\leq&\epsilon^2,\quad \forall m=1,2,\cdots. \end{aligned}

综上所述, \{(\hat{\delta}_m,\breve{\delta}_m,\eta_m): m=0,1,\cdots \}\mathrm{L}^2-连续的. 证毕.

4.2 概自守

考虑 (\hat{\delta}_m,\breve{\delta}_m,\eta_m) 的部分和, 其表达式为

\begin{aligned} \label{415.1} \left[ \begin{array}{c} \hat{\delta}_{m}^n\\ \breve{\delta}_{m}^n\\ \end{array} \right](t)&=&\sum\limits_{k=1}^{n}\Bigg\{ e^{-\frac{a}{\hbar}t}\left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha t) & \sin(\acute{\lambda}_k^\alpha t) \\ -\sin(\acute{\lambda}_k^\alpha t) & \cos(\acute{\lambda}_k^\alpha t) \\ \end{array} \right] \left[ \begin{array}{c} \hat{\varphi}_k\\ \breve{\varphi}_k \\ \end{array} \right] \\ && + \frac{1}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) & \sin(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (s-t)) & \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \end{array} \right] \\ && \times\left[ \begin{array}{c} -\mu\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})+\mathrm{Im}f_k \\ \mu\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1})-\mathrm{Re}f_k \\ \end{array} \right](s)\mathrm{d}s\Bigg\}e_k^\alpha, \end{aligned}
(4.3)
\begin{aligned} \label{415.2} \eta_{m}^n(t)&=& \sum\limits_{k=1}^n\Bigg\{e^{-\frac{b}{2}t}\left[ \cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t)\right]\phi_k +\frac{1}{\grave{\lambda}_k^\beta}e^{-\frac{b}{2}t}\sin(\grave{\lambda}_k^\beta t)\psi_k \\ &&+\frac{1}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \left[\nu \mathbf{Sat} _{2,k}(|\delta_{m-1}(s)|^2)+g_k(s)\right]\mathrm{d}s\Bigg\}e_k^\beta, \end{aligned}
(4.4)

其中 t\in\mathbf{R}_0, m,n=1,2,\cdots. 通过命题 4.1 的证明可知 \{(\hat{\delta}_m^n,\breve{\delta}_m^n,\eta_m^n): n=1,2,\cdots \}\{\mathrm{L}^2(\Omega)\}^3 中对任意的 t\in\bar{I}_T 一致收敛于 (\hat{\delta}_m,\breve{\delta}_m,\eta_m), m=1,2,\cdots .

命题4.2 若定理 1.4 所有假设均成立. 则 \{(\delta_m,\eta_m)=(\hat{\delta}_m,\breve{\delta}_m,\eta_m): m=0,1,\cdots \} \subseteq\mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3).

简记

\hat{\mathcal{F}}(\varphi,\phi,t)=-\mu\widehat{ \mathbf{Sat} }_{1}(\varphi\phi)+\mathrm{Im}f(\cdot,t),\quad \breve{\mathcal{F}}(\varphi,\phi,t)=\mu\widetilde{ \mathbf{Sat} }_{1}(\varphi\phi)-\mathrm{Re}f(\cdot,t),
\mathcal{G}(\varphi,t)=\nu \mathbf{Sat} _{2}(|\varphi|^2)+g(\cdot,t),\quad \forall t\in\mathbf{R}_0.

由于 (\varphi,\phi)=(\hat{\varphi},\breve{\varphi},\phi)\in\mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3), 利用文献 [30,定理 3.6] 可知,

\hat{\mathcal{F}}(\varphi,\phi,t), \breve{\mathcal{F}}(\varphi,\phi,t) \in\mathbb{AAA}(\{\mathrm{L}^2(\Omega)\}^3\times\mathbf{R}_0,\mathrm{L}^2(\Omega)),
\mathcal{G}(\varphi,t)\in\mathbb{AAA}(\{\mathrm{L}^2(\Omega)\}^2\times\mathbf{R}_0,\mathrm{L}^2(\Omega)),\quad \forall t\in\mathbf{R}_0.

因此,

\hat{\mathcal{F}}(\varphi,\phi,\cdot)=\hat{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,\cdot) +\hat{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,\cdot),\quad \breve{\mathcal{F}}(\varphi,\phi,\cdot)=\breve{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,\cdot) +\breve{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,\cdot),
\mathcal{G}(\varphi,\cdot)=\mathcal{G}_{\mathbb{A}}(\varphi,\cdot)+\mathcal{G}_{\mathbb{N}}(\varphi,\cdot),

其中 \hat{\mathcal{F}}_{\mathbb{A}}, \breve{\mathcal{F}}_{\mathbb{A}} \in\mathbb{AA}(\{\mathrm{L}^2(\Omega)\}^3\times\mathbf{R}_0,\mathrm{L}^2(\Omega)), \hat{\mathcal{F}}_{\mathbb{N}}, \breve{\mathcal{F}}_{\mathbb{N}} \in\aleph(\{\mathrm{L}^2(\Omega)\}^3\times\mathbf{R}_0,\mathrm{L}^2(\Omega)), \mathcal{G}_{\mathbb{A}}\in\mathbb{AA}(\{\mathrm{L}^2(\Omega)\}^2\times\mathbf{R}_0,\mathrm{L}^2(\Omega)), \mathcal{G}_{\mathbb{N}}\in \aleph(\{\mathrm{L}^2(\Omega)\}^2\times\mathbf{R}_0,\mathrm{L}^2(\Omega)).

m=1, 则 \hat{\delta}_{1}^n(t)=\sum\limits_{i=1}^4\hat{\delta}_{1,i}^n(t), 其中

\left[ \begin{array}{c} \hat{\delta}_{1,1}^n\\ \breve{\delta}_{1,1}^n\\ \end{array} \right](t)=\sum\limits_{k=1}^{n} e^{-\frac{a}{\hbar}t}\left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha t) & \sin(\acute{\lambda}_k^\alpha t) \\ -\sin(\acute{\lambda}_k^\alpha t) & \cos(\acute{\lambda}_k^\alpha t) \\ \end{array} \right] \left[ \begin{array}{c} \hat{\varphi}_k\\ \breve{\varphi}_k \\ \end{array} \right]e_k^\alpha,
\left[ \begin{array}{c} \hat{\delta}_{1,2}^n\\ \breve{\delta}_{1,2}^n\\ \end{array} \right](t)=\frac{1}{\hbar}\sum\limits_{k=1}^{n} \int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) & \sin(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (s-t)) & \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \end{array} \right] \left[ \begin{array}{c} \hat{\mathcal{F}}_{\mathbb{N},k}(\varphi,\phi,s) \\ \breve{\mathcal{F}}_{\mathbb{N},k}(\varphi,\phi,s) \\ \end{array} \right]\mathrm{d}s e_k^\alpha,
\left[ \begin{array}{c} \hat{\delta}_{1,3}^n\\ \breve{\delta}_{1,3}^n\\ \end{array} \right](t)=\sum\limits_{k=1}^{n} \int_{-\infty}^0 \frac{-e^{-\frac{a}{\hbar}(t-s)}}{\hbar} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) & \sin(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (s-t)) & \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \end{array} \right] \left[ \begin{array}{c} \hat{\mathcal{F}}_{\mathbb{A},k}(\varphi,\phi,s) \\ \breve{\mathcal{F}}_{\mathbb{A},k}(\varphi,\phi,s) \\ \end{array} \right]\mathrm{d}s e_k^\alpha,
\left[ \begin{array}{c} \hat{\delta}_{1,4}^n\\ \breve{\delta}_{1,4}^n\\ \end{array} \right](t)=\frac{1}{\hbar}\sum\limits_{k=1}^{n} \int_{-\infty}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) & \sin(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (s-t)) & \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \end{array} \right] \left[ \begin{array}{c} \hat{\mathcal{F}}_{\mathbb{A},k}(\varphi,\phi,s) \\ \breve{\mathcal{F}}_{\mathbb{A},k}(\varphi,\phi,s) \\ \end{array} \right]\mathrm{d}s e_k^\alpha,
\eta_{1,1}^n(t)=\sum\limits_{k=1}^{n}\Bigg\{e^{-\frac{b}{2}t}\left[ \cos(\grave{\lambda}_k^\beta t) +\frac{b}{2\grave{\lambda}_k^\beta}\sin(\grave{\lambda}_k^\beta t) \right]\phi_k+ \frac{1}{\grave{\lambda}_k^\beta}e^{-\frac{b}{2}t}\sin(\grave{\lambda}_k^\beta t)\psi_k\Bigg\} e_k^\beta,
\eta_{1,2}^n(t)=\frac{1}{\grave{\lambda}_k^\beta}\sum\limits_{k=1}^{n}\int_{0}^t e^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \mathcal{G}_{\mathbb{N},k}(\varphi,s)\mathrm{d}s e_k^\beta,
\eta_{1,3}^n(t)=\frac{-1}{\grave{\lambda}_k^\beta}\sum\limits_{k=1}^{n}\int_{-\infty}^0 e^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \mathcal{G}_{\mathbb{A},k}(\varphi,s)\mathrm{d}s e_k^\beta,
\eta_{1,4}^n(t)=\frac{1}{\grave{\lambda}_k^\beta}\sum\limits_{k=1}^{n}\int_{-\infty}^t e^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \mathcal{G}_{\mathbb{A},k}(\varphi,s)\mathrm{d}s e_k^\beta,\quad n\in\mathbf{Z}_+\cup\{\infty\}, t\in\mathbf{R}_0.

与命题 4.1 类似, \{(\hat{\delta}_{1,i}^n(\cdot),\breve{\delta}_{1,i}^n(\cdot),\eta_{1,i}^n(\cdot))\}\{\mathrm{L}^2(\Omega)\}^3 中收敛于 (\hat{\delta}_{1,i}^\infty(\cdot),\breve{\delta}_{1,i}^\infty(\cdot),\eta_{1,i}^\infty(\cdot)), i=1,2,3. 此外,

\begin{aligned} \lim\limits_{t\rightarrow\infty}|\hat{\delta}_{1,1}^\infty(t)|_2^2&\leq& \lim\limits_{t\rightarrow\infty}\lim\limits_{n\rightarrow\infty}e^{-\frac{2a}{\hbar}t}\sum\limits_{k=1}^{n}(\hat{\varphi}_k^2+\breve{\varphi}_k^2) \leq \lim\limits_{t\rightarrow\infty}e^{-\frac{2a}{\hbar}t}|\varphi|_2^2=0, \\ \lim\limits_{t\rightarrow\infty}|\hat{\delta}_{1,2}^\infty(t)|_2^2 &\leq& \lim\limits_{t\rightarrow\infty}\lim\limits_{n\rightarrow\infty}\frac{1}{a\hbar} \int_{0}^te^{-\frac{a}{\hbar}(t-s)}\sum\limits_{k=1}^{n}\left[\hat{\mathcal{F}}_{\mathbb{N},k}^2(\varphi,\phi,s) +\breve{\mathcal{F}}_{\mathbb{N},k}^2(\varphi,\phi,s)\right]\mathrm{d}s \\ &\leq& \frac{1}{a\hbar}\lim\limits_{t\rightarrow\infty} \int_{0}^{\frac{t}{2}}e^{-\frac{a}{\hbar}(t-s)}\left[\big|\hat{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2 +\big|\breve{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2\right]\mathrm{d}s \\ &&+\frac{1}{a\hbar}\lim\limits_{t\rightarrow\infty} \int_{\frac{t}{2}}^te^{-\frac{a}{\hbar}(t-s)}\left[\big|\hat{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2 +\big|\breve{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2\right]\mathrm{d}s \\ &\leq&\frac{1}{a^2}\lim\limits_{t\rightarrow\infty}(e^{-\frac{at}{2\hbar}}-e^{-\frac{at}{\hbar}}) \sup\limits_{s\in\mathbf{R}_0}\left[\big|\hat{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2 +\big|\breve{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2\right] \\ &&+\frac{1}{a^2}\lim\limits_{t\rightarrow\infty} \sup\limits_{s\in[\frac{t}{2},\infty)}\left[\big|\hat{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2 +\big|\breve{\mathcal{F}}_{\mathbb{N}}(\varphi,\phi,s)\big|_2^2\right]=0, \\ \lim\limits_{t\rightarrow\infty}|\hat{\delta}_{1,3}^\infty(t)|_2^2 &\leq&\frac{1}{a\hbar} \lim\limits_{t\rightarrow\infty}\lim\limits_{n\rightarrow\infty} \int_{-\infty}^0e^{-\frac{a}{\hbar}(t-s)}\sum\limits_{k=1}^{n}\left[\hat{\mathcal{F}}_{\mathbb{A},k}^2(\varphi,\phi,s) +\breve{\mathcal{F}}_{\mathbb{A},k}^2(\varphi,\phi,s)\right]\mathrm{d}s \\ &\leq&\frac{1}{a^2} \lim\limits_{t\rightarrow\infty}e^{-\frac{at}{\hbar}} \sup\limits_{s\in\mathbf{R}_0}\left[\big|\hat{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,s)\big|_2^2 +\big|\breve{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,s)\big|_2^2\right]=0, \end{aligned}

因此, \hat{\delta}_{1,i}^\infty\in\aleph(\mathbf{R}_0, \mathrm{L}^2(\Omega)), i=1,2,3.

由于 \hat{\mathcal{F}}_{\mathbb{A}}, \breve{\mathcal{F}}_{\mathbb{A}} \in\mathbb{AA}(\{\mathrm{L}^2(\Omega)\}^3\times\mathbf{R},\mathrm{L}^2(\Omega)), 因而对于每个序列 \{\bar{t}_p\}_{p\in\mathbf{Z}_+}, 都存在一个子列 \{t_p\}_{p\in\mathbf{Z}_+}\subseteq\{\bar{t}_p\}_{p\in\mathbf{Z}_+} 和函数 \hat{\mathcal{F}}_{\mathbb{A}}^\circ, \breve{\mathcal{F}}_{\mathbb{A}}^\circ: \{\mathrm{L}^2(\Omega)\}^3\times\mathbf{R}\rightarrow\mathrm{L}^2(\Omega) 使得在 \mathrm{L}^2(\Omega) 中, 对于每个 t\in\mathbf{R}

\hat{\mathcal{F}}_{\mathbb{A}}^\circ(\delta,\eta,t) =\lim\limits_{p\rightarrow\infty}\hat{\mathcal{F}}_{\mathbb{A}}(\delta,\eta,t+t_p),\quad \breve{\mathcal{F}}_{\mathbb{A}}^\circ(\delta,\eta,t) =\lim\limits_{p\rightarrow\infty}\breve{\mathcal{F}}_{\mathbb{A}}(\delta,\eta,t+t_p),
\lim\limits_{p\rightarrow\infty}\hat{\mathcal{F}}_{\mathbb{A}}^\circ(\delta,\eta,t-t_p) =\hat{\mathcal{F}}_{\mathbb{A}}(\delta,\eta,t),\quad \lim\limits_{p\rightarrow\infty}\breve{\mathcal{F}}_{\mathbb{A}}^\circ(\delta,\eta,t-t_p) =\breve{\mathcal{F}}_{\mathbb{A}}(\delta,\eta,t)

\hat{\delta}_{1,4}^{\circ,n}(t)= \frac{1}{\hbar}\sum\limits_{k=1}^{n} \int_{-\infty}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{c} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \left[ \begin{array}{c} \hat{\mathcal{F}}_{\mathbb{A},k}^\circ(\varphi,\phi,s) \\ \breve{\mathcal{F}}_{\mathbb{A},k}^\circ(\varphi,\phi,s) \\ \end{array} \right]\mathrm{d}s e_k^\alpha,

其中 n\in\mathbf{Z}_+\cup\{\infty\}, t\in\mathbf{R}. 与方程 (4.3) 和 (4.4) 的方法类似, 有 \{\hat{\delta}_{1,4}^{\circ,n}(t):n=1,2,\cdots \}\mathrm{L}^2(\Omega) 中关于 t\in\bar{I}_T 一致收敛于 \hat{\delta}_{1,4}^{\circ,\infty}(t). 因此,

\begin{aligned} \Big|\hat{\delta}_{1,4}^{n}(t+t_p)-\hat{\delta}_{1,4}^{\circ,n}(t)\Big|_2^2 &=&\frac{1}{\hbar^2}\int_{-\infty}^te^{-\frac{a}{\hbar}(t-s)}\mathrm{d}s\int_{-\infty}^te^{-\frac{a}{\hbar}(t-s)} \\ &&\times\bigg[\sum\limits_{k=1}^{n}\Big(\hat{\mathcal{F}}_{\mathbb{A},k}(\varphi,\phi,s+t_p) -\hat{\mathcal{F}}_{\mathbb{A},k}^\circ(\varphi,\phi,s)\Big)^2 \\&&+ \sum\limits_{k=1}^{n}\Big(\breve{\mathcal{F}}_{\mathbb{A},k}(\varphi,\phi,s+t_p) -\breve{\mathcal{F}}_{\mathbb{A},k}^\circ(\varphi,\phi,s)\Big)^2 \bigg]\mathrm{d}s \\ &\leq&\frac{1}{a\hbar}\int_{-\infty}^te^{-\frac{a}{\hbar}(t-s)} \Big|\hat{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,s+t_p) -\hat{\mathcal{F}}_{\mathbb{A}}^\circ(\varphi,\phi,s)\Big|_2^2\mathrm{d}s \\ &&+\frac{1}{a\hbar}\int_{-\infty}^te^{-\frac{a}{\hbar}(t-s)} \Big|\breve{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,s+t_p) -\breve{\mathcal{F}}_{\mathbb{A}}^\circ(\varphi,\phi,s)\Big|_2^2\mathrm{d}s. \end{aligned}

在上述不等式中令 n\rightarrow\infty 可得

\begin{aligned} \Big|\hat{\delta}_{1,4}^{\infty}(t+t_p)-\hat{\delta}_{1,4}^{\circ,\infty}(t)\Big|_2^2 &\leq&\frac{1}{a\hbar}\int_{-\infty}^te^{-\frac{a}{\hbar}(t-s)} \Big|\hat{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,s+t_p) -\hat{\mathcal{F}}_{\mathbb{A}}^\circ(\varphi,\phi,s)\Big|_2^2\mathrm{d}s \\ &&+\frac{1}{a\hbar}\int_{-\infty}^te^{-\frac{a}{\hbar}(t-s)} \Big|\breve{\mathcal{F}}_{\mathbb{A}}(\varphi,\phi,s+t_p) -\breve{\mathcal{F}}_{\mathbb{A}}^\circ(\varphi,\phi,s)\Big|_2^2\mathrm{d}s. \end{aligned}

由 Lebesgue 控制收敛定理得到

\lim\limits_{p\rightarrow\infty}\Big|\hat{\delta}_{1,4}^{\infty}(t+t_p)-\hat{\delta}_{1,4}^{\circ,\infty}(t)\Big|_2^2=0, \quad \forall t\in\mathbf{R}.

同理,

\lim\limits_{p\rightarrow\infty}\Big|\hat{\delta}_{1,4}^{\circ,\infty}(t-t_p)-\hat{\delta}_{1,4}^{\infty}(t)\Big|_2^2=0, \quad \forall t\in\mathbf{R}.

因此, \hat{\delta}_{1,4}^\infty(\cdot)\in\mathbb{AA}(\mathbf{R},\mathrm{L}^2(\Omega)) 并且当 n\rightarrow\infty 时, 有

\hat{\delta}_{1}^n(\cdot)=\hat{\delta}_{1,4}^n(\cdot) +\sum\limits_{i=1}^3\hat{\delta}_{1,i}^n(\cdot)\xrightarrow[]{\mathrm{L}^2(\Omega)} \hat{\delta}_{1}(\cdot)=\hat{\delta}_{1,4}^\infty(\cdot) +\sum\limits_{i=1}^3\hat{\delta}_{1,i}^\infty(\cdot)\in\mathbb{AAA}(\mathbf{R}_0,\mathrm{L}^2(\Omega))

同理, 当 n\rightarrow\infty 时, 有

\breve{\delta}_{1}^n(\cdot)=\breve{\delta}_{1,4}^n(\cdot) +\sum\limits_{i=1}^3\breve{\delta}_{1,i}^n(\cdot)\xrightarrow[]{\mathrm{L}^2(\Omega)} \breve{\delta}_{1}(\cdot)=\breve{\delta}_{1,4}^\infty(\cdot) +\sum\limits_{i=1}^3\breve{\delta}_{1,i}^\infty(\cdot)\in\mathbb{AAA}(\mathbf{R}_0,\mathrm{L}^2(\Omega)),
\eta_{1}^n(\cdot)=\eta_{1,4}^n(\cdot)+\sum\limits_{i=1}^3\eta_{1,i}^n(\cdot)\xrightarrow[]{\mathrm{L}^2(\Omega)} \eta_{1}(\cdot)=\eta_{1,4}^\infty(\cdot) +\sum\limits_{i=1}^3\eta_{1,i}^\infty(\cdot)\in\mathbb{AAA}(\mathbf{R}_0,\mathrm{L}^2(\Omega)).

由数学归纳法可知 \{(\delta_m,\eta_m)=(\hat{\delta}_m,\breve{\delta}_m,\eta_m): m=2,3,\cdots \} \subseteq\mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3). 证毕.

定义范数 |\xi|_{\sup}=\sup\limits_{t\in\mathbf{R}_0}|\xi(t)|_2, \forall \xi\in\mathbb{AAA}(\mathbf{R}_0,\mathrm{L}^2(\Omega)). 则根据文献 [30] 可知 (\mathbb{AAA}(\mathbf{R}_0, \mathrm{L}^2(\Omega)), |\cdot|_{\sup}) 是 Banach 空间.

命题4.3 若定理 1.4 的所有假设都成立. 则 \{(\delta_m,\eta_m)=(\hat{\delta}_m,\breve{\delta}_m,\eta_m): m=0,1,\cdots \}\mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) 中的 Cauchy 序列.

\{\hat{\delta}_m: m=1,2,\cdots \} 的部分和得,

\begin{aligned} \big|\hat{\delta}_{m+1}^n(t)-\hat{\delta}_{m}^n(t)\big|_{2}^2&=&\sum\limits_{k=1}^{n}\bigg\{ \frac{\mu}{\hbar}\int_{0}^t e^{-\frac{a}{\hbar}(t-s)} \left[ \begin{array}{cc} \cos(\acute{\lambda}_k^\alpha (t-s)) \\ \sin(\acute{\lambda}_k^\alpha (t-s)) \end{array} \right]^\top \\ && \times\bigg[ \begin{array}{c} -\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m}\eta_{m})+\widehat{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1}) \\ \widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m}\eta_{m})-\widetilde{ \mathbf{Sat} }_{1,k}(\delta_{m-1}\eta_{m-1}) \\ \end{array} \bigg](s)\mathrm{d}s\bigg\}^2 \\ &\leq&\frac{\mu^2}{a\hbar} \int_{0}^te^{-\frac{a}{\hbar}(t-s)}\Big| \widehat{ \mathbf{Sat} }_{1}(\delta_{m}\eta_{m})-\widehat{ \mathbf{Sat} }_{1}(\delta_{m-1}\eta_{m-1}) \Big|_2^2\mathrm{d}s \\ &&+\frac{\mu^2}{a\hbar} \int_{0}^te^{-\frac{a}{\hbar}(t-s)}\Big| \widetilde{ \mathbf{Sat} }_{1}(\delta_{m}\eta_{m})-\widetilde{ \mathbf{Sat} }_{1}(\delta_{m-1}\eta_{m-1}) \Big|_2^2\mathrm{d}s \\ &\leq&\frac{16\mu^2}{a^2\rho_0^2} \left(\big|\delta_{m}-\delta_{m-1}\big|_{\sup}^2+\big|\eta_{m}-\eta_{m-1}\big|_{\sup}^2\right), \end{aligned}

其中

\big|\delta_{m}-\delta_{m-1}\big|_{\sup}^2:=\big|\hat{\delta}_{m}-\hat{\delta}_{m-1}\big|_{\sup}^2 +\big|\breve{\delta}_{m}-\breve{\delta}_{m-1}\big|_{\sup}^2,\quad t\in\mathbf{R}_0, m,n=1,2,\cdots.

在上述不等式中令 n\rightarrow\infty, 可得

\big|\hat{\delta}_{m+1}-\hat{\delta}_{m}\big|_{\sup}^2\leq\frac{16\mu^2}{a^2\rho_0^2} \left(\big|\delta_{m}-\delta_{m-1}\big|_{\sup}^2+\big|\eta_{m}-\eta_{m-1}\big|_{\sup}^2\right), \quad m=1,2,\cdots.

同理,

\big|\breve{\delta}_{m+1}-\breve{\delta}_{m}\big|_{\sup}^2\leq\frac{16\mu^2}{a^2\rho_0^2} \left(\big|\delta_{m}-\delta_{m-1}\big|_{\sup}^2+\big|\eta_{m}-\eta_{m-1}\big|_{\sup}^2\right), \quad m=1,2,\cdots.

综上所述,

\big|\delta_{m+1}-\delta_{m}\big|_{\sup}\leq\frac{4\sqrt{2}\mu}{a\rho_0} \left(\big|\delta_{m}-\delta_{m-1}\big|_{\sup}+\big|\eta_{m}-\eta_{m-1}\big|_{\sup}\right), \quad m=1,2,\cdots.

同理, 由方程 (4.4) 可得

\begin{aligned} \big|\eta_{m+1}^n(t)-\eta_{m}^n(t)\big|_{2}^2&=&\sum\limits_{k=1}^{n}\Bigg\{ \frac{\nu}{\grave{\lambda}_k^\beta}\int_{0}^te^{-\frac{b}{2}(t-s)}\sin(\grave{\lambda}_k^\beta(t-s)) \\ &&\times \left[ \mathbf{Sat} _{2,k}(|\delta_{m}(s)|^2)- \mathbf{Sat} _{2,k}(|\delta_{m-1}(s)|^2)\right]\mathrm{d}s\Bigg\}^2 \\ &\leq&\frac{2\nu^2}{b(\grave{\lambda}_1^\beta)^2} \int_{0}^te^{-\frac{b}{2}(t-s)}\Big| \mathbf{Sat} _{2}(|\delta_{m}(s)|^2)- \mathbf{Sat} _{2}(|\delta_{m-1}(s)|^2) \Big|_2^2\mathrm{d}s \\ &\leq&\frac{9\nu^2}{b^2(\grave{\lambda}_1^\beta)^2\varepsilon^2} \big|\delta_{m}-\delta_{m-1}\big|_{\sup}^2,\quad \forall t\in\mathbf{R}_0. \end{aligned}

所以,

\big|\eta_{m+1}-\eta_{m}\big|_{\sup}\leq\frac{3\nu}{b\grave{\lambda}_1^\beta\varepsilon}\big|\delta_{m}-\delta_{m-1}\big|_{\sup},\quad m=1,2,\cdots.
(4.6)

定义

\Pi_0=0,\quad \Pi_m:=\Pi_{m-1}+\max\{\big|\delta_{m}-\delta_{m-1}\big|_{0}, \big|\eta_{m}-\eta_{m-1}\big|_{0}\},\quad m=1,2,\cdots.

结合不等式 (4.5) 和 (4.6) 可知,

\Pi_{m+1}-\Pi_{m}\leq \max\bigg\{\frac{8\sqrt{2}\mu}{a\rho_0}, \frac{3\nu}{b\grave{\lambda}_1^\beta\varepsilon} \bigg\}(\Pi_{m}-\Pi_{m-1})\leq\gamma^m\Pi_{1},\quad m=1,2,\cdots.

对任意的 p\in\mathbf{Z}_+, 当 m\rightarrow\infty 时, 有

\max\left\{\big|\delta_{m+p}-\delta_{m}\big|_{0}, \big|\eta_{m+p}-\eta_{m}\big|_{0} \right\}\leq\sum\limits_{k=m}^{m+p-1}\left(\Pi_{k+1}-\Pi_{k} \right)\leq\sum\limits_{k=m}^{m+p-1}\gamma^k \Pi_{1}=\frac{\gamma^m\Pi_{1}}{1-\gamma} \rightarrow0.

因此, \{\hat{\delta}_m\}, \{\breve{\delta}_m\}\{\eta_m\}\mathbb{AAA}(\mathbf{R}_0,\mathrm{L}^2(\Omega)) 中的 Cauchy 序列. 证毕.

由命题 4.3 和 \mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) 的完备性可知, 存在 (\delta_*,\eta_*)=(\hat{\delta}_*,\breve{\delta}_*,\eta_*) 使得 \{(\hat{\delta}_m,\breve{\delta}_m,\eta_m)\}\mathbb{AAA}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) 中收敛于 (\hat{\delta}_*,\breve{\delta}_*,\eta_*). 取 (\tilde{\delta}_*,\tilde{\eta}_*)=(\hat{\tilde{\delta}}_*,\breve{\tilde{\delta}}_*,\tilde{\eta}_*)

\begin{array}{l} {\left[\begin{array}{c} \hat{\tilde{\delta}}_{*} \\ \breve{\tilde{\delta}}_{*} \end{array}\right](t)=\sum_{k=1}^{\infty}\left\{e^{-\frac{a}{\hbar} t}\left[\begin{array}{cc} \cos \left(\dot{\lambda}_{k}^{\alpha} t\right) & \sin \left(\dot{\lambda}_{k}^{\alpha} t\right) \\ -\sin \left(\dot{\lambda}_{k}^{\alpha} t\right) & \cos \left(\dot{\lambda}_{k}^{\alpha} t\right) \end{array}\right]\left[\begin{array}{c} \hat{\varphi}_{k} \\ \breve{\varphi}_{k} \end{array}\right]\right.} \\ +\frac{1}{\hbar} \int_{0}^{t} e^{-\frac{a}{\hbar}(t-s)}\left[\begin{array}{ll} \cos \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) & \sin \left(\dot{\lambda}_{k}^{\alpha}(t-s)\right) \\ \sin \left(\hat{\lambda}_{k}^{\alpha}(s-t)\right) & \cos \left(\hat{\lambda}_{k}^{\alpha}(t-s)\right) \end{array}\right] \\ \left.\times\left[\begin{array}{c} -\mu \widehat{\boldsymbol{S a t}}_{1, k}\left(\delta_{*} \eta_{*}\right)+\operatorname{Im} f_{k} \\ \mu \widetilde{\mathbf{S a t}}_{1, k}\left(\delta_{*} \eta_{*}\right)-\operatorname{Re} f_{k} \end{array}\right](s) \mathrm{d} s\right\} e_{k}^{\alpha}, \quad \forall t \in \mathbf{R}_{0}, \\ \tilde{\eta}_{*}(t)=\sum_{k=1}^{\infty}\left\{e^{-\frac{b}{2} t}\left[\cos \left(\grave{\lambda}_{k}^{\beta} t\right)+\frac{b}{2 \grave{\lambda}_{k}^{\beta}} \sin \left(\grave{\lambda}_{k}^{\beta} t\right)\right] \phi_{k}+\frac{1}{\grave{\lambda}_{k}^{\beta}} e^{-\frac{b}{2} t} \sin \left(\grave{\lambda}_{k}^{\beta} t\right) \psi_{k}\right. \\ \left.+\frac{1}{\grave{\lambda}_{k}^{\beta}} \int_{0}^{t} e^{-\frac{b}{2}(t-s)} \sin \left(\grave{\lambda}_{k}^{\beta}(t-s)\right)\left[\nu \mathbf{S a t}_{2, k}\left(\left|\delta_{*}(s)\right|^{2}\right)+g_{k}(s)\right] \mathrm{d} s\right\} e_{k}^{\beta}, \quad \forall t \in \mathbf{R}_{0}. \\ \end{array}

与命题 4.1 类似, (\hat{\tilde{\delta}}_*,\breve{\tilde{\delta}}_*,\tilde{\eta}_*)\{\mathrm{L}^2(\Omega)\}^3 中是有定义的.

定义 (\tilde{\delta}_*^n,\tilde{\eta}_*^n)=(\hat{\tilde{\delta}}_*^n,\breve{\tilde{\delta}}_*^n,\tilde{\eta}_*^n)(\hat{\tilde{\delta}}_*,\breve{\tilde{\delta}}_*,\tilde{\eta}_*) 的前 n 项的部分和, n=1,2,\cdots . 利用与方程 (4.3) 和 (4.4) 类似的方法可知, \{(\hat{\tilde{\delta}}_*^n(t),\breve{\tilde{\delta}}_*^n(t),\tilde{\eta}_*^n(t))\}\{\mathrm{L}^2(\Omega)\}^3 中收敛于 (\hat{\tilde{\delta}}_*(t),\breve{\tilde{\delta}}_*(t),\tilde{\eta}_*(t)), \forall t\in\mathbf{R}_0. 类似于不等式 (4.5) 和 (4.6) 的讨论可得,

\big|\delta_{m}^n(t)-\tilde{\delta}_{*}^n(t)\big|_{2}\leq\frac{4\sqrt{2}\mu}{a\rho_0} \left[\big|\delta_{m}-\delta_{*}\big|_{\sup}+\big|\eta_{m}-\eta_{*}\big|_{\sup}\right],
\big|\eta_{m}^n(t)-\tilde{\eta}_{*}^n(t)\big|_2\leq\frac{\sqrt{3}\nu}{b\grave{\lambda}_1^\beta\varepsilon} \big|\delta_{m}-\delta_{*}\big|_{\sup},

其中

\big|\delta_{m}^n(t)-\tilde{\delta}_{*}^n(t)\big|_{2}:= \sqrt{\big|\hat{\delta}_{m}^n(t)-\hat{\tilde{\delta}}_{*}^n(t)\big|_{2}^2 +\big|\breve{\delta}_{m}^n(t)-\breve{\tilde{\delta}}_{*}^n(t)\big|_{2}^2},\quad t\in\mathbf{R}_0, m, n=1,2,\cdots.

在上述最后两个不等式中依次取 n\rightarrow\infty, m\rightarrow\infty, 得

\big|\hat{\delta}_{*}(t)-\hat{\tilde{\delta}}_{*}(t)\big|_{2}=0,\quad \big|\breve{\delta}_{*}(t)-\breve{\tilde{\delta}}_{*}(t)\big|_{2}=0,\quad \big|\eta_{*}(t)-\tilde{\eta}_{*}(t)\big|_{2}=0,\quad\forall t\in\mathbf{R}_0.

定理 1.4 的证明 由定理 1.2 知, (\mathbf{z}_0, \mathbf{w} _0)=(\hat{\mathbf{z}}_0,\breve{\mathbf{z}}_0, \mathbf{w} _0) 是方程 (1.1) 在 \mathrm{C}(\mathbf{R}_0,\{\mathrm{L}^2(\Omega)\}^3) 中的唯一解, 并且该解满足 Fourier 级数 (1.3) 和 (1.4). 类似与定理 1.2 的证明, 有(\hat{\delta}_*,\breve{\delta}_*,\eta_*)=(\hat{\mathbf{z}}_0,\breve{\mathbf{z}}_0, \mathbf{w} _0). 证毕.

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