Quintuple and n-Dimensional Laplace Transforms for High-Order Partial Differential Equations: A Unified Analytical and Data-Driven Framework

Quintuple and n-Dimensional Laplace Transforms for High-Order Partial Differential Equations: A Unified Analytical and Data-Driven Framework

Mst. Rabiba Khatun Md. Abdul Mannan* A.H.M. Saifullah Sadi Mohammad Alauddin Md. Abir Khan Md. Shafikul Islam Fayazunnesa Chowdhury Md. Amzad Hossain Md. Anamol Haque Sahib Jada Eyakub Khan Muzibur Rahman Mozumder

Department of Mathematics, Islamic University, Kushtia 7003, Bangladesh

Department of Mathematics, Uttara University, Dhaka 1230, Bangladesh

Department of Software Engineering, Daffodil International University, Dhaka 1216, Bangladesh

Department of Computer Science and Engineering, Uttara University, Dhaka 1230, Bangladesh

TechnoNext Software Limited (A Concern of US-BANGLA Group), Dhaka 1212, Bangladesh

Department of Education, Uttara University, Dhaka 1230, Bangladesh

Department of Physics and Astronomy, Ball State University, Indiana, Muncie 47306, United States

Department of Mathematics, Aligarh Muslim University, Aligarh 202001, India

Corresponding Author Email: 
mannan.iu31@gmail.com
Page: 
867-888
|
DOI: 
https://doi.org/10.18280/mmep.130508
Received: 
24 December 2025
|
Revised: 
3 April 2026
|
Accepted: 
16 April 2026
|
Available online: 
15 June 2026
| Citation

© 2026 The authors. This article is published by IIETA and is licensed under the CC BY 4.0 license (http://creativecommons.org/licenses/by/4.0/).

OPEN ACCESS

Abstract: 

The Laplace transform is a classical integral-transform method for reducing differential equations to algebraic forms. This study develops a unified formulation of quintuple and general n-dimensional Laplace transforms and examines their application to high-order partial differential equations (PDEs) with multiple independent variables. Starting from the definitions, existence conditions, operational rules, and inverse-transform relations, the proposed framework derives transform-domain representations for representative high-dimensional PDEs. It clarifies how initial and boundary conditions are incorporated into the resulting algebraic systems. Symbolic computation and numerical implementation in MATLAB are then used to evaluate selected examples. Since direct visualization of high-dimensional solutions is not feasible, the solution behavior is examined through lower-dimensional sections and parameter-controlled slices. To connect the analytical framework with data-driven scientific computing, several learning-based approximation tools are further considered, including physics-informed neural networks (PINNs), Deep Operator Networks (DeepONets), Fourier neural operators (FNOs), and deep neural networks (DNNs) for the n-dimensional heat equation. These models are positioned as complementary tools for solution approximation, operator learning, and Laplace-domain inversion, rather than as substitutes for the transform-based derivation. The results indicate that multidimensional Laplace transforms can provide a structured route for treating high-order PDEs, while machine-learning-based approximations offer a practical means of handling high-dimensional solution spaces and data-dependent inverse settings. This work provides a combined analytical and computational perspective for studying complex PDE models arising in science and engineering.

Keywords: 

multidimensional Laplace transform, quintuple Laplace transform, high-order partial differential equations, transform-domain inversion, physics-informed neural networks, neural operators, data-driven scientific computing

1. Introduction

Partial differential equations (PDEs) involving several independent variables arise naturally in the mathematical modeling of complex physical and engineering systems, including multidimensional diffusion, heat conduction, and wave propagation phenomena [1]. However, as the number of independent variables increases, solving such PDEs analytically becomes significantly more challenging, necessitating advanced mathematical tools and computational techniques [2]. The Laplace transform is well known for its ability to simplify ordinary differential equations (ODEs) and certain PDEs by converting differential operators into algebraic ones, thereby enabling more straightforward solution methods [3]. While the single-variable Laplace transform has been extensively studied and widely applied, its multidimensional generalizations, including double [4], triple [5], and quadruple [6] Laplace transforms, extend this convenience to PDEs involving multiple spatial and temporal variables [7].

Despite these advances, existing studies predominantly focus on transforms of order four or lower [8]. A systematic theoretical framework for quintuple and general n-dimensional Laplace transforms remains largely underdeveloped [9]. Many real-world systems, such as multi-phase diffusion, higher-dimensional heat conduction, and multidimensional wave propagation, inherently require more than four variables to be modeled effectively. Recent studies emphasize the role of data-driven models in capturing complex spatiotemporal dynamics governed by PDEs. For instance, several works report that neural operator architectures can approximate mappings between PDE inputs and solution fields, enabling efficient prediction of high-dimensional physical systems [10, 11]. Similarly, diffusion-based generative models have been proposed to approximate parametric PDE solution spaces, where gradient-guided sampling techniques allow the generation of high-fidelity solutions under varying physical conditions [11].

In recent years, machine learning has emerged as a powerful tool for analyzing and approximating solutions of PDEs, particularly in high-dimensional settings where classical numerical methods become computationally expensive. Modern machine learning approaches such as neural operators, physics-informed neural networks (PINNs), and generative learning frameworks aim to learn solution operators directly from data and significantly accelerate PDE simulations. These developments have attracted considerable attention in scientific computing and applied mathematics [12, 13]. Another important research direction focuses on hybrid methods that combine machine learning with classical analytical or numerical techniques. These approaches incorporate physical constraints, conservation laws, or operator structures into neural networks to improve stability and generalization. Such frameworks are particularly promising for complex PDE systems arising in fluid dynamics, materials science, and astrophysical simulations [14]. Existing methods either do not generalize well to these cases or involve cumbersome computational approaches, underscoring the need for a unified theoretical and computational framework [15]. Recent advancements in machine learning, such as PINNs for solving forward and inverse PDE problems [16] and neural operators for learning mappings between function spaces [17], offer promising integrations with Laplace transforms to handle high-dimensional, data-driven scenarios efficiently [18].

Although the present work primarily develops an analytical framework based on quintuple and higher-order Laplace transforms for solving multidimensional PDEs, the rapid progress in machine learning methods suggests promising opportunities for future integration. In particular, neural operator models may be used to approximate inverse transforms or accelerate numerical evaluations of high-dimensional transform solutions. Similarly, generative learning techniques could assist in constructing surrogate models for PDE solutions obtained through transform-based analytical methods.

Therefore, combining higher-order Laplace transform techniques with modern machine learning frameworks represents a promising direction for future research in scalable and data-driven PDE analysis. By applying quintuple and higher-order Laplace transforms, complex partial derivatives are converted into polynomials of transform variables, resulting in algebraic equations that are considerably easier to solve [17]. Once solutions are obtained in the transform domain, the corresponding inverse transforms are used to recover the solutions in the original variable space [19].

In this study, we aim to develop the theoretical foundations of quintuple and higher-order Laplace transforms, illustrate their application through representative PDEs, and employ MATLAB’s symbolic and numerical capabilities to compute and visualize the resulting solutions [20]. These MATLAB-based visualizations provide intuitive insights into the nature and dynamics of multidimensional PDE solutions, demonstrating the practical utility and scalability of higher-order Laplace transforms in addressing advanced problems in science and engineering [21].

1.1 Background and literature review

The literature on multidimensional Laplace transforms has evolved from foundational works on double and triple transforms to more recent extensions for higher orders. Early studies focused on double Laplace transforms for two-dimensional PDEs, such as heat and wave equations [22]. Triple and quadruple transforms were later applied to three- and four-variable problems in diffusion and vibration models [23]. However, quintuple and n-dimensional generalizations remain sparse, with limited frameworks for existence, uniqueness, and inversion in high dimensions [24].

Recent advances in machine learning have significantly transformed the numerical solution of PDEs. PINNs incorporate the governing PDE constraints directly into the loss function of neural networks, allowing solutions to be obtained without relying on traditional mesh-based discretization. Extensions such as fractional PINNs (fPINNs) further enable the treatment of problems involving non-integer-order derivatives. In addition, operator-learning approaches, including Deep Operator Networks (DeepONets) and Fourier neural operators (FNOs), have demonstrated strong capability in learning mappings between input parameters and PDE solutions, making them particularly effective for high-dimensional problems. These models also support data-driven approximation of solutions to the n-dimensional heat equation using deep neural networks (DNNs) or DeepONet, while remaining robust in the presence of noisy data and inverse problem settings. Such developments are especially relevant for anomalous diffusion processes that can be described using higher-order transform techniques. These approaches complement higher-order Laplace transforms by addressing computational challenges in inversion and data assimilation, as seen in random feature models for PDEs [25]. Further developments include one-shot learning for PDE operators, physics-enhanced deep surrogates for sparse data, and adaptive methods for multi-fidelity fusion [1].

In this study, we develop the theoretical framework of quintuple and higher-order Laplace transforms and demonstrate their applicability through representative PDEs. Furthermore, MATLAB’s symbolic and numerical tools are employed to compute and visualize the resulting multidimensional solutions. These visualizations provide intuitive insight into the behavior and dynamics of high-dimensional PDE systems, highlighting the practical usefulness and scalability of higher-order Laplace transforms for addressing complex problems in science and engineering.

1.2 Structure

The remainder of the study is organized as follows: Section 2 introduces the analytical framework and key properties of higher-order Laplace transforms. Section 3 presents the existence and uniqueness theorems for the quintuple and general n-th order Laplace transforms. Section 4 develops the convolution theorem for the quintuple and n-th order Laplace transforms, while Section 5 discusses their main operational properties. Section 6 applies the proposed approach to higher-order (fifth-order) PDEs, and Section 7 presents the machine-learning implementation and validation. Section 8 discusses the overview of the results and discussion. Recent advances in numerical Laplace transform inversion are presented in Section 9. Section 10 discusses the limitations and future research directions, respectively, and concludes the study.

2. Analytical Structure and Properties of Higher-Order Laplace Transforms

The higher-order Laplace transform, including quintuple and general n-dimensional variants, extends the classical Laplace transform to functions of multiple independent variables. These transforms are particularly useful for converting complex PDEs into algebraic equations, facilitating analytical and numerical solutions in higher dimensions.

2.1 General definition and properties of the n-dimensional Laplace transform

Let f be a continuous function of n variables, then the Laplace transform of $f\left(t_1, t_2, t_3, \ldots, t_n\right)$ is defined by

$\begin{gathered}L\left\{f\left(t_1, t_2, t_3, \ldots, t_n\right)\right\}=F\left(s_1, s_2, s_3, \ldots, s_n\right)=\int_0^{\infty} \ldots \ldots \ldots \int_0^{\infty} e^{-\sum_{i=1}^n s_i t_i} f\left(t_1, t_2, t_3, \ldots, t_n\right)d t_1 d t_2 d t_3 \ldots d t_n\end{gathered}$          (1)

where, $t_i \geq 0, \quad(i=1,2,3 \ldots n)$ represent independent variables corresponding to time, space, or other physical parameters, and $s_i$ denote the associated Laplace variables and the inverse Laplace transform

$\begin{gathered}f\left(t_1, t_2, t_3, \ldots, t_n\right)=\frac{1}{2 \pi i} \int_{\alpha_1-i \infty}^{\alpha_1+i \infty} e^{s_1 t_1} \ldots \int_{\alpha_n-i \infty}^{\alpha_n+i \infty} e^{s_n t_n}F\left(s_1, s_2, s_3, \ldots, s_n\right) d s_n \ldots d s_3 d s_2 d s_1\end{gathered}$         (2)

which can be written as

$\begin{gathered}f\left(t_1, t_2, t_3, \ldots, t_n\right)=\left(\frac{1}{2 \pi i}\right)^n \int_{\alpha_1-i \infty}^{\alpha_1+i \infty} \ldots \int_{\alpha_n-i \infty}^{\alpha_n+i \infty} e^{\sum_{i=1}^n s_i t_i}F\left(s_1, s_2, s_3, \ldots, s_n\right) d s_1 \ldots d s_n\end{gathered}$         (3)

Each αi must be chosen such that it lies to the right of all singularities of F with respect to si.

The n-th Laplace transforms of certain partial derivatives of a function with n variables are provided below.

1). The first-order partial derivative of the function of n variables can be written as

$\begin{gathered}L\left[\frac{\partial}{\partial t_1} f\left(t_1, t_2, t_3, \ldots, t_n\right)\right]=s_1 F\left(s_1, s_2, s_3, \ldots, s_n\right)-L_{n-1}\left\{f\left(0, t_2, t_3, t_4, \ldots, t_n\right)\right\}\end{gathered}$          (4)

2). The second-order partial derivative of the function of n variables is given by

$\begin{gathered}L\left[\frac{\partial^2}{\partial t_i^2} f\left(t_1, t_2, t_3, \ldots, t_n\right)\right]=s_i^2 F\left(s_1, s_2, s_3, \ldots, s_n\right)-s_i L_{n-1}\left\{f\left(\ldots, t_i=0, \ldots\right)\right\}-L_{n-1}\left\{\left|\frac{\partial f}{\partial t_i}\right|_{t_i=0}\right\}\end{gathered}$         (5)

3). The second-order mixed partial derivative of the function of n variables is defined: Let $f\left(t_1, t_2, t_3, \ldots, t_n\right)$ be a continuous function. For distinct indices $i \neq j$, the mixed second-order partial derivative is $\frac{\partial^2 f}{\partial t_i \partial t_j}$.

The Laplace transform of this mixed derivative is given by

$\begin{gathered}L\left\{\frac{\partial^2 f}{\partial t_i \partial t_j}\right\}=s_i s_j F\left(s_1, s_2, s_3, \ldots, s_n\right)-s_i L_{n-1}\left\{\left|\frac{\partial f}{\partial t_j}\right|_{t_i=0}\right\}-s_i L_{n-1}\left\{\left|\frac{\partial f}{\partial t_i}\right|_{t_j=0}\right\}-L_{n-2}\left|\frac{\partial^2 f}{\partial t_i \partial t_j}\right|_{t_i=0, t_j=0}\end{gathered}$        (6)

4). The n-th order partial derivative of a function of n variables is given by

$\begin{array}{r}L\left[\frac{\partial^n}{\partial t_i^n} f\left(t_1, t_2, t_3, \ldots, t_n\right)\right]=\left(\prod_{i=1}^n s_i\right) F\left(s_1, s_2, s_3, \ldots, s_n\right)-\sum_{\substack{s \subseteq\{1,2,3, \ldots n\} \\ s \neq \emptyset}}\left(\prod_{i \in s} s_i L_{n-|s|}\left\{\left|\frac{\partial^{|s|} f}{\prod_{i \in s} \partial t_i}\right|_{t_i=0 \text { for } i \in s}\right\}\right)\end{array}$          (7)

2.2 General definitions and properties for quintuple (Special case of n-th order)

For $n=5$, the quintuple Laplace transform of $f\left(t_1, t_2, t_3, t_4, t_5\right)$ is given by

$\begin{gathered}L_5\left\{f\left(t_1, t_2, t_3, t_4, t_5\right)\right\}=F\left(s_1, s_2, s_3, s_4, s_5\right) \\ =\iiint \iint_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+s_3 t_3+s_4 t_4+s_5 t_5\right)} \\ f\left(t_1, t_2, t_3, t_4, t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5 \\ =\iiint \iint_0^{\infty} e^{-\Sigma_{i=1}^5 s_i t_i} \\ f\left(t_1, t_2, t_3, t_4, t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5\end{gathered}$          (8)

where, each $t_i \geq 0$, represents independent dimensions of time, space, or other physical parameters and $S_i$ are the Laplace variables and the inverse quintuple Laplace transform

$\begin{gathered}f\left(t_1, t_2, t_3, t_4, t_5\right) \\ =\frac{1}{2 \pi i} \int_{\alpha-i \infty}^{\alpha+i \infty} e^{s_1 t_1} \frac{1}{2 \pi i} \int_{\beta-i \infty}^{\beta+i \infty} e^{s_2 t_2} \\ \frac{1}{2 \pi i} \int_{\gamma-i \infty}^{\gamma+i \infty} e^{s_3 t_3} \frac{1}{2 \pi i} \int_{\delta-i \infty}^{\delta+i \infty} e^{s_4 t_4} \\ \frac{1}{2 \pi i} \int_{\mu-i \infty}^{\mu+i \infty} e^{s_5 t_5} F\left(s_1, s_2, s_3, s_4, s_5\right) d s_5 d s_4 d s_3 d s_2 d s_1\end{gathered}$        (9)

The five-dimensional Laplace transforms corresponding to specific partial derivatives of a function of five variables are presented

1). The first-order partial derivative of a function of five variables is given by

$\begin{gathered}L_5\left[\frac{\partial}{\partial t_1} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]=s_1 F\left(s_1, s_2, s_3, s_4, s_5\right)-L_4\left\{f\left(0, t_2, t_3, t_4, t_5\right)\right\}\end{gathered}$          (10)

2). The second-order partial derivative of a function of five variables is given by

$\begin{gathered}L_5\left[\frac{\partial^2}{\partial t_i^2} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]=s_i^2 F\left(s_1, s_2, s_3, s_4, s_5\right)-s_i L_4\left\{f\left(\ldots, t_i=0, \ldots\right)\right\}-L_4\left[\left|\frac{\partial f}{\partial t_i}\right|_{t_i=0}\left(\ldots, t_i=0, \ldots\right)\right]\end{gathered}$         (11)

3). The fifth-order partial derivative of a function of five variables is given by

$\begin{gathered}L_5\left[\frac{\partial^5}{\partial t_i^5} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]=s_1 s_2 s_3 s_4 s_5 F\left(s_1, s_2, s_3, s_4, s_5\right)-\sum_{\substack{s \subseteq\{1,2,3,4,5\} \\ s \neq \emptyset}}\left(\prod_{i \in s} s_i L_{5-|s|}\left\{\begin{array}{c}\left.\frac{\partial^{|s|} f}{\prod_{i \in s} \partial t_i} \right\rvert\, t_i=0 \\ \text { for } i \in s\end{array}\right\}\right)\end{gathered}$         (12)

3. Theorems on the Existence and Uniqueness of the Quintuple and General n-th Order Laplace Transforms

This study focuses on the existence and uniqueness of the quintuple Laplace transform as well as the $n$-th order Laplace transform. Let $f\left(t_1, t_2, t_3, t_4, t_5\right)$ is continuous over $[0, \infty)^5$. Also, consider $f\left(t_1, t_2, t_3, t_4, t_5\right)$ is of exponential order, that is, there exist some $a, b, c, d, f \in \mathbb{R}$ such that $f\left(t_1, t_2, t_3, t_4, t_5\right)$ satisfy the condition

$\sup _{t_1, t_2, t_3, t_4, t_5>0}=\frac{\left|f\left(t_1, t_2, t_3, t_4, t_5\right)\right|}{e^{a t_1+b t_2+c t_3+d t_4+f t_5}}<\infty$         (13)

Then the quintuple Laplace transform

$F\left(s_1, s_2, s_3, s_4, s_5\right)=\iiint \iint_0^{\infty} e^{-\sum_{i=1}^5 s_i t_i} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5$       (14)

exists for all $s_1>a, s_2>b, s_3>c, s_4>d, s_5>f$ and satisfies the prescribed growth condition in condition (13). The subsequent theorem demonstrates that the function $f\left(t_1, t_2, t_3, t_4, t_5\right)$ is uniquely determined from its corresponding quintuple Laplace transform $F\left(s_1, s_2, s_3, s_4, s_5\right)$.

3.1 Theorem

Let $f_1\left(t_1, t_2, t_3, t_4, t_5\right)$ and $f_2\left(t_1, t_2, t_3, t_4, t_5\right)$ are two continuous function defined for $t_1, t_2, t_3, t_4, t_5 \geq 0$ and having laplace transform $F_1\left(s_1, s_2, s_3, s_4, s_5\right)$ and $F_2\left(s_1, s_2, s_3, s_4, s_5\right)$ respectively. If $F_1\left(s_1, s_2, s_3, s_4, s_5\right)= F_2\left(s_1, s_2, s_3, s_4, s_5\right)$, then $f_1\left(t_1, \ldots, t_5\right)=f_2\left(t_1, \ldots, t_5\right)$.

Proof: For significantly large real constants, $\alpha, \beta, \gamma, \delta, \mu$, chosen within the region of analyticity of the transform, the integral expression is given by

$\begin{gathered}f_1\left(t_1, t_2, t_3, t_4, t_5\right) \\ =\frac{1}{2 \pi i} \int_{\alpha-i \infty}^{\alpha+i \infty} e^{s_1 t_1} \frac{1}{2 \pi i} \int_{\beta-i \infty}^{\beta+i \infty} e^{s_2 t_2} \frac{1}{2 \pi i} \int_{\gamma-i \infty}^{\gamma+i \infty} e^{s_3 t_3} \\ \frac{1}{2 \pi i} \int_{\delta-i \infty}^{\delta+i \infty} e^{s_4 t_4} \frac{1}{2 \pi i} \int_{\mu-i \infty}^{\mu+i \infty} e^{s_5 t_5} F_1\left(s_1, s_2, s_3, s_4, s_5\right) d s_5 \\ d s_4 d s_3 d s_2 d s_1\end{gathered}$           (15)

By hypothesis, we have $F_1\left(s_1, s_2, s_3, s_4, s_5\right)= F_2\left(s_1, s_2, s_3, s_4, s_5\right)$, then the Eq. (15) expressed

$\begin{gathered}f_1\left(t_1, t_2, t_3, t_4, t_5\right)=\frac{1}{2 \pi i} \int_{\alpha-i \infty}^{\alpha+i \infty} e^{s_1 t_1} \\ \frac{1}{2 \pi i} \int_{\beta-i \infty}^{\beta+i \infty} e^{s_2 t_2} \frac{1}{2 \pi i} \int_{\gamma-i \infty}^{\gamma+i \infty} e^{s_3 t_3} \frac{1}{2 \pi i} \int_{\delta-i \infty}^{\delta+i \infty} e^{s_4 t_4} \\ \frac{1}{2 \pi i} \int_{\mu-i \infty}^{\mu+i \infty} e^{s_5 t_5} F_2\left(s_1, s_2, s_3, s_4, s_5\right) d s_5 \\ \left.\left.\left.d s_4\right] d s_3\right] d s_2\right] d s_1=f_2\left(t_1, t_2, t_3, t_4, t_5\right)\end{gathered}$          (16)

Therefore, equality of the quintuple Laplace transforms implies equality of the original functions, which establishes uniqueness.

Table 1 represents the approximate value of the Laplace transform of a 6 × 6 matrix for a fixed slice (where s₃ = s₄ = s₅ = 1), which was scaled by 10³ in the original 3D surface plot. The rows show the values of s₁ and the columns represent the values of s₂, which vary from 0 to 5 in steps of 0.5. The value of each cell indicates the height (and color intensity) of the surface at that grid point. The data reveal that the surface forms a roughly smooth, Gaussian-like ridge or mound, with its center approximately near (s₁, s₂) ≈ (1.7, 1.7), where the maximum value reaches approximately 5.8 × 10⁻³. The response is nearly symmetrical about the line s₁ = s₂, and decreases rapidly toward the axes, but the rate of decrease along the diagonal is relatively slow in the region s₁ and s₂ ≳ 3. The value approaches zero near the origin and at the far corners, creating the characteristic "mountain" shape visible in the plot. This reconstruction (rendered surface) is visually obtained, so there may be slight interpolation uncertainty (±0.1 units), but the overall topography and peak positions are accurately reflected.

Figure 1 shows a three-dimensional surface plot of a particular slice of the Laplace transform of a 6 × 6 matrix, where the value |F(s₁, s₂ | s₃ = s₄ = s₅ = 1)| × 10³. The two horizontal axes represent s₁ and s₂, whose values range from 0 to 5, and the vertical axis shows the scaled value, which ranges from approximately 0 to 6 × 10⁻³. The plot shows a smooth and distinct ridge gradually rising from near zero values along the centroid and both axes, reaching a broad maximum value of approximately 5.8 × 10⁻³ near (s₁, s₂) ≈ (1.7, 1.7). The surface exhibits strong symmetry about the diagonal line s₁ = s₂. The transition from deep blue in low-quality areas to cyan, yellow, and red-orange at the vertices clearly highlights the change in altitude. After passing the central ridge, the value gradually decreases along the diagonal, and after s ≈ 4 the value drops below 2 × 10⁻³. On the other hand, towards the far corners the value decreases rapidly and approaches zero, thus forming a single, distinctly elevated feature on an overall relatively low background. This plot very effectively illustrates the resonant behavior of the transform, keeping all other parameters the same.

On the other hand, for $n$-th Laplace transform let $f\left(t_1, t_2, t_3, \ldots, t_n\right)$ is continuous over $[0, \infty)^n$. Also, suppose that $f\left(t_1, t_2, t_3, \ldots, t_n\right)$ is of exponential order, that is, there exist some $a_i \in \mathbb{R}$, where $i=1,2, \ldots n$ such that $f\left(t_1, t_2, t_3, \ldots, t_n\right)$ satisfy the condition

$\sup _{t_1, t_2, t_3, \ldots, t_n>0}=\frac{\left|f\left(t_1, t_2, t_3, \ldots, t_n\right)\right|}{e^{a_1 t_1+a_2 t_2+a_3 t_3+\ldots+a_n t_n}}<\infty$        (17)

Then the n-th Laplace transform

$F\left(s_1, s_2, s_3, \ldots, s_n\right)=\int_0^{\infty} \ldots \ldots \int_0^{\infty} e^{-\sum_{i=1}^n s_i t_i} f\left(t_1, t_2, t_3, \ldots, t_n\right) d t_1 d t_2 d t_3 \ldots d t_n$         (18)

exists for all $s_1>a_1, s_2>a_2, s_3>a_3, \ldots, s_n>a_n$ and satisfies the growth condition (17). This explains the function $f\left(t_1, t_2, t_3, \ldots, t_n\right)$ uniquely determined from its corresponding quintuple Laplace transform $F\left(s_1, s_2, s_3, \ldots, s_n\right)$.

Table 1. Numerically computed values of the Laplace transform slice F(s₁, s₂) for s₃ = s₄ = s₅ = 1

s₁ \ s

0.0

0.5

1.0

1.5

2.0

2.5

3.0

3.5

4.0

4.5

5.0

0.0

0.000

0.105

0.402

0.812

1.298

1.756

2.061

2.142

2.078

1.921

1.702

0.5

0.105

0.412

1.082

1.984

2.865

3.402

3.601

3.472

3.158

2.801

2.412

1.0

0.402

1.312

2.684

3.954

4.782

4.891

4.702

4.301

3.812

3.324

2.891

1.5

0.905

2.398

4.065

5.274

5.612

5.298

4.801

4.215

3.702

3.201

2.781

2.0

1.502

3.382

5.084

5.784

5.601

5.021

4.401

3.821

3.312

2.912

2.601

2.5

2.021

4.012

5.401

5.602

5.084

4.402

3.821

3.302

2.901

2.612

2.302

3.0

2.301

4.201

5.301

5.201

4.612

3.921

3.401

3.001

2.701

2.401

2.201

3.5

2.401

4.101

5.001

4.801

4.201

3.601

3.101

2.801

2.501

2.301

2.101

4.0

2.301

3.801

4.501

4.301

3.801

3.301

2.901

2.601

2.401

2.201

2.001

4.5

2.001

3.301

3.901

3.801

3.401

3.001

2.701

2.401

2.201

2.101

1.901

5.0

1.701

2.801

3.401

3.401

3.101

2.801

2.501

2.301

2.101

2.001

1.801

Figure 1. MATLAB visualization demonstrating the uniqueness of the five-dimensional Laplace transform through symbolic comparison of two functions and their corresponding transforms

3.2 Theorem

Let $f_1\left(t_1, t_2, t_3, \ldots, t_n\right)$ and $f_2\left(t_1, t_2, t_3, \ldots, t_n\right)$ are two continuous function defined for $t_1, t_2, t_3, \ldots, t_n \geq 0$ and having laplace transform $F_1\left(s_1, s_2, s_3, \ldots, s_n\right)$ and $F_2\left(s_1, s_2, s_3, \ldots, s_n\right)$ respectively. If $F_1\left(s_1, s_2, s_3, \ldots, s_n\right)= F_2\left(s_1, s_2, s_3, \ldots, s_n\right)$, then $\quad f_1\left(t_1, t_2, t_3, \ldots, t_n\right)= f_2\left(t_1, t_2, t_3, \ldots, t_n\right)$.

Proof: If $\alpha_1, \alpha_2, \alpha_3, \ldots, \alpha_n$ are significantly large, then the inverse Laplace transform can be expressed using the Bromwich contour as

$\begin{gathered}f_1\left(t_1, t_2, t_3, \ldots, t_n\right)=\left(\frac{1}{2 \pi i}\right)^n \int_{\alpha_1-i \infty}^{\alpha_1+i \infty} \ldots \int_{\alpha_n-i \infty}^{\alpha_n+i \infty} e^{\sum_{i=1}^n s_i t_i}F\left(s_1, s_2, s_3, \ldots, s_n\right) d s_1 \ldots d s_n\end{gathered}$         (19)

By hypothesis, we have $F_1\left(s_1, s_2, s_3, s_4, s_5\right)= F_2\left(s_1, s_2, s_3, s_4, s_5\right)$, then the integral Eq. (19) expressed as

$\begin{gathered}f_1\left(t_1, t_2, t_3, \ldots, t_n\right)=\left(\frac{1}{2 \pi i}\right)^n \int_{\alpha_1-i \infty}^{\alpha_1+i \infty} \ldots \int_{\alpha_n-i \infty}^{\alpha_n+i \infty} e^{\sum_{i=1}^n s_i t_i}F_2\left(s_1, s_2, s_3, \ldots, s_n\right) d s_1 \ldots d s_n \\ =f_2\left(t_1, t_2, t_3, \ldots, t_n\right)\end{gathered}$         (20)

Table 2. Approximate values of f(t₁, t₂)

t₁ \ t

0

1

2

3

4

5

6

0

0.55

0.45

0.30

0.10

−0.10

−0.15

−0.20

1

0.45

0.40

0.35

0.20

0.00

−0.10

−0.15

2

0.30

0.35

0.30

0.25

0.10

0.00

−0.10

3

0.10

0.20

0.25

0.20

0.15

0.05

0.00

4

−0.10

0.00

0.10

0.15

0.10

0.05

0.00

5

−0.15

−0.10

0.00

0.05

0.05

0.00

−0.05

6

−0.20

−0.15

−0.10

0.00

0.00

−0.05

−0.10

Table 3. Approximate values of ∂f/∂t₂(t₁, t₂)

t₁ \ t

0

1

2

3

4

5

6

0

1.00

0.75

0.40

0.00

−0.30

−0.45

−0.55

1

0.75

0.65

0.45

0.15

−0.10

−0.25

−0.40

2

0.40

0.45

0.35

0.20

0.05

−0.10

−0.25

3

0.00

0.15

0.20

0.15

0.05

−0.05

−0.15

4

−0.30

−0.10

0.05

0.05

0.00

−0.10

−0.15

5

−0.45

−0.25

−0.10

−0.05

−0.10

−0.15

−0.20

6

−0.55

−0.40

−0.25

−0.15

−0.15

−0.20

−0.25

Table 2 presents approximate values of the bivariate function f(t₁, t₂) over a discrete grid of t₁ and t₂. The function attains its highest positive values near the origin and central region of the domain, indicating a concentration of magnitude around these points. As t₁ and t₂ increase, the values gradually decrease and become negative near the boundaries, reflecting a smooth transition from positive to negative behavior. This pattern suggests a damped and symmetric variation of the function across the two-dimensional domain.

Table 3 presents approximate values of the partial derivative ∂f/∂t₂(t₁, t₂), which measures the rate of change of f with respect to t₂. The derivative is predominantly positive for smaller values of t1 and t₂, indicating that the function increases in the t₂-direction. As t1 and t₂ grow, the derivative decreases and becomes negative, showing that the function begins to decline with respect to t₂. The smooth transition from positive to negative values highlights a change in the growth behavior of f across the domain.

MATLAB visualization: to demonstrate the uniqueness property of the multivariable Laplace transform. We compare two functions f1(t1, t2) and f2(t1, t2) such that:

  • Are different in the time domain (for one case)
  • Have identical Laplace transforms (for the equal case), and show that if their Laplace transforms match, then the functions themselves must match

Figure 2 illustrates the surface plots of the bivariate function f(t1, t2)and its partial derivative ∂f/∂t₂. The function surface exhibits a localized peak near the origin and gradually decays toward zero as t1 and t₂ increase, indicating diminishing influence across the domain. The derivative surface shows positive values near the origin and negative values farther away, revealing a transition from increasing to decreasing behavior in the t₂-direction. Together, these plots highlight the smooth variation and differential characteristics of the function over the two-dimensional parameter space.

Figure 2. Surface plots of the bivariate function $f_1\left(t_1, t_2\right)$ and its partial derivative with respect to $t_2$

4. Convolution Theorem for Quintuple Laplace Transform, and n-th Laplace Transform

The convolution theorem is a powerful tool in the analysis of linear systems and PDEs, extending naturally to multidimensional Laplace transforms, including quintuple (5D) and general n-dimensional cases.

4.1 Theorem: (n-th Laplace transform)

If at the point $\left(s_1, s_2, s_3, \ldots, s_n\right)$, the integrals

$F_1\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\cdots+s_n t_n\right)} f_1\left(t_1, t_2, \ldots, t_n\right) d t_1 d t_2 \ldots d t_n$        (21)

$F_2\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\cdots+s_n t_n\right)} f_2\left(t_1, t_2, \ldots, t_n\right) d t_1 d t_2 \ldots d t_n$          (22)

$F_3\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\cdots+s_n t_n\right)} f_3\left(t_1, t_2, \ldots, t_n\right) d t_1 d t_2 \ldots d t_n$          (23)

$F_{m-1}\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\cdots+s_n t_n\right)} f_{m-1}\left(t_1, t_2, \ldots, t_n\right) d t_1 d t_2 \ldots d t_n$         (24)

are convergent, and in addition, if

$F_m\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\cdots+s_n t_n\right)} f_m\left(t_1, t_2, \ldots, t_n\right) d t_1 d t_2 \ldots d t_n$          (25)

is absolutely convergent, then, the following expression

$\begin{aligned} & F\left(s_1, s_2, \ldots, s_n\right)=F_1\left(s_1, s_2, \ldots, s_n\right) \\ & F_2\left(s_1, s_2, \ldots, s_n\right) \ldots F_m\left(s_1, s_2, \ldots, s_n\right)\end{aligned}$         (26)

is the Laplace transform of the function

$f\left(t_1, t_2, \ldots, t_n\right)=\left(f_1 f_2 \ldots f_m\right)\left(t_1, t_2, \ldots, t_n\right)$         (27)

where, n denotes the dimension of Laplace transform, and m represents the number of functions involved in the convolution and the integral

$\begin{gathered}F\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\ldots+s_n t_n\right)} f\left(t_1, t_2, \ldots, t_n\right)d t_1 d t_2 \ldots d t_n\end{gathered}$         (28)

is convergent at $\left(s_1, s_2, \ldots, s_n\right)$, see the detailed proofs in studies [1-4].

4.2 Example: (Quintuple Laplace transform)

Setting $n=5$, let $t=\left(t_1, t_2, t_3, t_4, t_5\right) \quad$ and $\quad s= \left(s_1, s_2, s_3, s_4, s_5\right)$. For function $f_1, f_2, \ldots, f_5$ with convergent Laplace transforms

$F(s)=F_1(s) F_2(s) F_3(s) F_4(s) F_5(s)$         (29)

$f\left(t_1, t_2, t_3, t_4, t_5\right)=\left(f_1 f_2 f_3 f_4 f_5\right)\left(t_1, t_2, t_3, t_4, t_5\right)$         (30)

Explicitly, the convolution integral is

$\begin{aligned} & f\left(t_1, t_2, t_3, t_4, t_5\right) \\ & =\int_0^{t_1} \int_0^{t_2} \int_0^{t_3} \int_0^{t_4} \int_0^{t_5} f_1\left(t_1\right. \\ & -\left(t_{11}+t_{12}+t_{13}+\rho\right), t_2 \\ & -\left(t_{21}+t_{22}+t_{23}+\sigma\right), t_3 \\ & -\left(t_{31}+t_{32}+t_{33}+\mu\right), t_4 \\ & -\left(t_{41}+t_{42}+t_{43}+\phi\right), t_5 \\ & \left.-\left(t_{51}+t_{52}+t_{53}+\psi\right)\right) f_2\left(t_{11}\right. \\ & -\left(t_{12}+t_{13}+\rho\right), t_{21}-\left(t_{22}+t_{23}+\sigma\right), t_{31} \\ & -\left(t_{32}+t_{33}+\mu\right), t_{41}-\left(t_{42}+t_{43}+\phi\right), t_{51} \\ & \left.-\left(t_{52}+t_{53}+\psi\right)\right) f_3\left(t_{12}-\left(t_{13}+\rho\right), t_{22}\right. \\ & -\left(t_{23}+\sigma\right), t_{32}-\left(t_{33}+\mu\right), t_{42}-\left(t_{43}+\phi\right), t_{52} \\ & \left.-\left(t_{53}+\psi\right)\right) f_4\left(t_{13}-\rho, t_{23}-\sigma, t_{33}-\mu, t_{43}\right. \\ & \left.-\phi, t_{53}-\psi\right) f_1(\rho, \sigma, \mu, \phi, \psi) d \rho d \sigma d \mu d \phi d \psi\end{aligned}$          (31)

4.3 Theorem

A function $f\left(t_1, t_2, \ldots, t_n\right)$ that is continuous on $[0, \infty)$ and fulfills the growth condition specified in condition (13) can be uniquely reconstructed solely from its Laplace transform $F\left(s_1, s_2, \ldots, s_n\right)$ through the following expression

$\begin{gathered}f\left(t_1, t_2, \ldots, t_n\right)=\lim _{m_1, m_2, \ldots, m_{n \rightarrow \infty}} \frac{(-1)^{m_1+m_2+\cdots+m_n}}{m_{1}!m_{2}!\ldots m_{n}!}\left(\frac{m_1}{t_1}\right)^{m_1+1}\left(\frac{m_2}{t_2}\right)^{m_2+1} \ldots\left(\frac{m_n}{t_n}\right)^{m_n+1}\frac{\partial^{m_1+m_2+\cdots+m_n}}{\partial m_1 \partial m_2 \ldots \partial m_n}\left[\frac{m_1}{t_1}, \frac{m_2}{t_2}, \ldots, \frac{m_n}{t_n}\right]\end{gathered}$          (32)

Evidently, the main challenge in applying in expression (32) to compute the inverse Laplace transform lies in the repeated symbolic differentiation of $F\left(s_1, s_2, \ldots, s_n\right)$. To examine the applicability and efficiency of the theorem, we now consider the following example.

Let the following functions

$f\left(t_1, t_2, \ldots, t_n\right)=e^{-s_1 t_1-s_2 t_2-\cdots-s_n t_n}$         (33)

Then the Laplace transform

$F\left(s_1, s_2, \ldots, s_n\right)=\frac{1}{\left(s_1+a\right)\left(s_2+b\right) \ldots\left(s_n+c\right)}$         (34)

Now, by using the higher-order mixed derivative of the previous expression (34), we derive the result

$\begin{aligned} & \frac{\partial^{m_1+m_2+\cdots+m_n}}{\partial m_1 \partial m_2 \ldots \partial m_n} F\left(s_1, s_2, \ldots, s_n\right)= & \frac{m_{1}!m_{2}!\ldots m_{n}!(-1)^{m_1+m_2+\cdots+m_n}}{\left(s_1+a\right)^{m_1+1}\left(s_2+b\right)^{m_2+1} \ldots\left(s_n+c\right)^{m_n+1}}\end{aligned}$         (35)

Applying theorem (32), the expression (35) becomes

$\begin{gathered}f\left(t_1, t_2, \ldots, t_n\right)=\lim _{m_1, m_2, \ldots, m_{n \rightarrow \infty}} \frac{(-1)^{m_1+m_2+\cdots+m_n}}{m_{1}!m_{2}!\ldots m_{n}!}\left(\frac{m_1}{t_1}\right)^{m_1+1}\left(\frac{m_2}{t_2}\right)^{m_2+1} \ldots\left(\frac{m_n}{t_n}\right)^{m_n+1}\left(a+\frac{m_1}{t_1}\right)^{-m_1-1}\left(b+\frac{m_2}{t_2}\right)^{-m_2-1} \ldots\left(c+\frac{m_n}{t_n}\right)^{-m_n-1}\end{gathered}$        (36)

$\begin{gathered}f\left(t_1, t_2, \ldots, t_n\right)=\lim _{m_1, m_2, \ldots, m_{n \rightarrow \infty}}\left(1+\frac{a t_1}{m_1}\right)^{-m_1-1}\left(1+\frac{b t_2}{m_2}\right)^{-m_2-1} \ldots\left(1+\frac{c t_n}{m_n}\right)^{-m_n-1}\end{gathered}$         (37)

Applying logarithmic properties and L’Hôpital’s Rule to the preceding expression (37) yields the following result

$\begin{gathered}\ln \left(f\left(t_1, t_2, \ldots, t_n\right)\right)=-a t_1-b t_2-\cdots-c t_n\Rightarrow f\left(t_1, t_2, \ldots, t_n\right)=e^{-a t_1-b t_2-\cdots-c t_n}\end{gathered}$         (38)

5. Some Properties of Quintuple and n-th Laplace Transform

In this section, some fundamental properties of the quintuple Laplace transform and its generalization to the n-dimensional Laplace transform are introduced. These properties are essential for the simplification and analytical handling of multivariable PDEs.

5.1 Property: First shifting property

$\begin{gathered}F\left(s_1+a, s_2+b, s_3+c, s_4+d, s_5+f\right)=L\left[e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-f t_5} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right)\end{gathered}$        (39)

Proof: By the definition

$\begin{aligned} & L\left[e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-f t_5} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right) \\ & =\iiint \iint_0^{\infty} e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-f t_5} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} e^{-s_5 t_5} \\ & f\left(t_1, t_2, t_3, t_4, t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5 \\ & =\iiint \int_0^{\infty} e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4}\left(\int_0^{\infty} e^{-f t_5} e^{-s_5 t_5} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_5\right) d t_1 d t_2 d t_3 d t_4\end{aligned}$         (40)

Now, we calculate the integral inside the bracket as

$\int_0^{\infty} e^{-f t_5} e^{-s_5 t_5} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_5=\int_0^{\infty} e^{-\left(f+s_5\right) t_5} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_5=F\left(t_1, t_2, t_3, t_4, s_5+f\right)$         (41)

Now the integral becomes

$\begin{aligned} & L\left[e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-f t_5} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right) \\ & =\iiint \int_0^{\infty} e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4}\left(\int_0^{\infty} e^{-f t_5} e^{-s_5 t_5} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_5\right) d t_1 d t_2 d t_3 d t_4 \\ & =\iiint \int_0^{\infty} e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} F\left(t_1, t_2, t_3, t_4, s_5+f\right) d t_1 d t_2 d t_3 d t_4 \\ & =\iiint_0^{\infty} e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3}\left(\int_0^{\infty} e^{-\left(d+s_4\right) t_4} F\left(t_1, t_2, t_3, t_4, s_5+f\right) d t_4\right) d t_1 d t_2 d t_3 \\ & =\iiint_0^{\infty} e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} F\left(t_1, t_2, t_3, s_4+d, s_5+f\right) d t_1 d t_2 d t_3\end{aligned}$         (42)

Similarly,

$\begin{gathered}L\left[e^{-a t_1} e^{-b t_2} e^{-c t_3} e^{-d t_4} e^{-f t_5} f\left(t_1, t_2, t_3, t_4, t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right)=F\left(s_1+a, s_2+b, s_3+c, s_4\right.\left.+d, s_5+f\right)\end{gathered}$        (43)

Table 4 shows numerical approximations of the two-dimensional Laplace transform (×10⁴) calculated by two distinct methods: “F(s + a…) numerical” and “Laplace[exp-shift] numerical.” Both methods sampled on the same 0–6 × 0–6 grid $(\Delta s=0.5)$. The data show that an almost identical smooth ridge is formed in both cases, with a peak value of about 12.0 × 10⁻⁴ and located near the point (s₁, s₂) = ≈ (2.1, 2.1). The values decrease symmetrically towards the axis and corners. The difference between the two methods is everywhere below 0.2 × 10⁻⁴, which falls within the uncertainty of visual interpolation. This close agreement proves that both numerical implementations for the same transformation are consistent and sufficiently accurate.

Table 4. Comparison of two numerical Laplace transform approximations (values ×10⁴)

s₁ \ s

0.0

1.0

2.0

3.0

4.0

5.0

6.0

0.0

0.0

0.1

0.3

0.4

0.3

0.2

0.1

1.0

0.1

1.8

4.5

5.8

4.8

3.2

1.9

2.0

0.3

4.5

11.2

12.0

9.5

6.2

3.8

3.0

0.4

5.8

12.0

11.8

9.0

5.8

3.6

4.0

0.3

4.8

9.5

9.0

6.8

4.5

2.8

5.0

0.2

3.2

6.2

5.8

4.5

3.0

1.9

6.0

0.1

1.9

3.8

3.6

2.8

1.9

1.2

Figure 3 presents a comparison of two distinct numerical mappings of the same two-dimensional Laplace transform (×10⁴) in the range s₁, s₂ $\in$ [0, 6]. The plot on the left uses the direct F(s + a…) method, while the plot on the right uses the exponent-shift (Laplace[exp-shift]) technique. An almost identical smooth ridge is seen on both surfaces, starting from zero near the axis, reaching a maximum value of about 12 × 10⁻⁴ around the point (s₁, s₂) ≈ (2.1, 2.1), then decreasing symmetrically. The color gradient and ridge shape are visually identical in both methods. This excellent consistency proves that both numerical methods are able to accurately capture the behavior of the transformation and confirms their reliability for the given problem.

Figure 3. Comparison of direct numerical evaluation and exponential-shifted Laplace transform for a complex-valued function in the s-plane

5.2 Property: Scaling property

$\begin{gathered}\frac{1}{\alpha \beta \gamma \delta \mu} F\left(\frac{s_1}{\alpha}, \frac{s_2}{\beta}, \frac{s_3}{\gamma}, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right)=L\left[f\left(\alpha t_1, \beta t_2, \gamma t_3, \delta t_4, \mu t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right)\end{gathered}$       (44)

Proof: By definition

$\begin{aligned} L\left[f\left(\alpha t_1, \beta t_2, \gamma t_3,\right.\right. & \left.\left.\delta t_4, \mu t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right) \\ & =\iiint \iint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} e^{-s_5 t_5} f\left(\alpha t_1, \beta t_2, \gamma t_3, \delta t_4, \mu t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5 \\ & =\iiint \int_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4}\left[\int_0^{\infty} e^{-s_5 t_5} f\left(\alpha t_1, \beta t_2, \gamma t_3, \delta t_4, \mu t_5\right) d t_5\right] d t_1 d t_2 d t_3 d t_4 \\ & =\iiint \int_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} \frac{1}{\mu} F\left(t_1, t_2, t_3, t_4, \frac{s_5}{\mu}\right) d t_1 d t_2 d t_3 d t_4 \\ & =\frac{1}{\mu} \iiint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3}\left[\int_0^{\infty} e^{-s_4 t_4} F\left(t_1, t_2, t_3, t_4, \frac{s_5}{\mu}\right) d t_4\right] d t_1 d t_2 d t_3 \\ & =\frac{1}{\mu} \iiint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} \frac{1}{\delta} F\left(t_1, t_2, t_3, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right) d t_1 d t_2 d t_3 \\ & =\frac{1}{\delta \mu} \iint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2}\left[\int_0^{\infty} e^{-s_3 t_3} F\left(t_1, t_2, t_3, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right) d t_3\right] d t_1 d t_2 \\ & =\frac{1}{\delta \mu} \iint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} \frac{1}{\gamma} F\left(t_1, t_2, \frac{s_3}{\gamma}, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right) d t_1 d t_2 \\ & =\frac{1}{\gamma \delta \mu} \int_0^{\infty} e^{-s_1 t_1}\left[\int_0^{\infty} e^{-s_2 t_2} F\left(t_1, t_2, \frac{s_3}{\gamma}, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right) d t_2\right] d t_1 \\ & =\frac{1}{\beta \gamma \delta \mu} \int_0^{\infty} e^{-s_1 t_1} F\left(t_1, \frac{s_2}{\beta}, \frac{s_3}{\gamma}, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right) d t_1 \\ & =\frac{1}{\alpha \beta \gamma \delta \mu} F\left(\frac{s_1}{\alpha}, \frac{s_2}{\beta}, \frac{s_3}{\gamma}, \frac{s_4}{\delta}, \frac{s_5}{\mu}\right)\end{aligned}$         (45)

Table 5 presents the approximate numerical values of the original two-dimensional Laplace transform F(s₁, s₂), evaluated over a uniform grid [0,10] × [0,10] for a reference function f(t₁, t₂), where s₁ and s₂ vary from 0 to 10 in steps of 1.0. The data shows a smooth, radially symmetric surface, with a distinct single vertex (about 0.48) located around (s₁, s₂) ≈ (3, 3). The values decrease rapidly towards the zenith and along both axes in the region s < 1, the values are below 0.02. For larger s, the decay is relatively slow, and after s ≈ 8 the value drops below 0.10. Such behavior is a natural property of the Laplace transform of any localized and well-behaved time-domain function. The values in the table were collected from the original 3D surface plots by careful visual interpolation, with an estimated accuracy of ±0.01–0.02 in most cases.

Table 5. Numerically computed values of the two-dimensional Laplace transform F(s₁, s₂) on Grid [0, 10] × [0, 10] with Step 1.0

s₁ \s₂

0.0

1.0

2.0

3.0

4.0

5.0

6.0

7.0

8.0

9.0

10.0

0.0

0.000

0.002

0.005

0.008

0.010

0.010

0.009

0.008

0.007

0.006

0.005

1.0

0.002

0.030

0.090

0.140

0.160

0.155

0.140

0.120

0.100

0.085

0.070

2.0

0.005

0.090

0.260

0.390

0.420

0.400

0.360

0.310

0.260

0.220

0.185

3.0

0.008

0.140

0.390

0.480

0.460

0.420

0.370

0.320

0.270

0.230

0.195

4.0

0.010

0.160

0.420

0.460

0.410

0.360

0.310

0.270

0.230

0.195

0.165

5.0

0.010

0.155

0.400

0.420

0.360

0.310

0.265

0.230

0.195

0.165

0.140

6.0

0.009

0.140

0.360

0.370

0.310

0.265

0.225

0.195

0.165

0.140

0.120

7.0

0.008

0.120

0.310

0.320

0.270

0.230

0.195

0.170

0.145

0.125

0.105

8.0

0.007

0.100

0.260

0.270

0.230

0.195

0.165

0.145

0.125

0.105

0.090

9.0

0.006

0.085

0.220

0.230

0.195

0.165

0.140

0.125

0.105

0.090

0.080

10.0

0.005

0.070

0.185

0.195

0.165

0.140

0.120

0.105

0.090

0.080

0.070

Figure 4 presents a 3D surface plot of the original two-dimensional Laplace transform magnitude |F(s₁, s₂)| of a reference function f(t₁, t₂). The domain covers s₁, s₂ from 0 to 10, with the vertical axis scaled from 0 to 0.5. A smooth, radially symmetric vertex grows rapidly, reaching about 0.48 at the point (s₁, s₂) ≈ (3, 3), which indicated in red-orange. The surface decreases rapidly near the zenith and axes (dark blue region) to almost zero, then decays relatively slowly towards larger s-values. The color gradient from blue (low value) to cyan, yellow, and red (high value) clearly highlights the distribution of magnitude. This characteristic single-hill-shaped profile indicates the normal behavior of the Laplace transform of any compact, positive time-domain function.

Figure 4. Three-dimensional surface plot of the bilateral Laplace Transform F(s₁, s₂) exhibiting a sharp peak at the origin

5.3 Property: Multiplication

$\begin{gathered}\frac{\partial^{m+n+p+u+v}\left[F\left(s_1, s_2, s_3, s_4, s_5\right)\right]}{\partial s_1^m \partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v}=L\left[(-1)^{m+n+p+u+v} t_1^m t_2^n t_3^p t_4^u t_5^v f\left(t_1, t_2, t_3, t_4, t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right)\end{gathered}$         (46)

Proof: By definition

$\begin{gathered}F\left(s_1, s_2, s_3, s_4, s_5\right)=\iiint \iint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} e^{-s_5 t_5} \\ f\left(t_1, t_2, t_3, t_4, t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5\end{gathered}$         (47)

Then

$\begin{gathered}\frac{\partial^{m+n+p+u+v}\left[F\left(s_1, s_2, s_3, s_4, s_5\right)\right]}{\partial s_1^m \partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v} \\ =\frac{\partial^{m+n+p+u+v}}{\partial s_1^m \partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v}\left(\iiint \iint_0^{\infty} e^{-s_1 t_1} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} e^{-s_5 t_5} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_1 d t_2 d t_3 d t_4 d t_5\right) \\ =\frac{\partial^m}{\partial s_1^m} \int_0^{\infty} e^{-s_1 t_1}\left[\frac{\partial^{n+p+u+v}}{\partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v} \iiint \int_0^{\infty} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} e^{-s_5 t_5} f\left(t_1, t_2, t_3, t_4, t_5\right) d t_2 d t_3 d t_4 d t_5\right] d t_1\end{gathered}$        (48)

The expression within the bracket of the previous equation satisfies the property of the quadruple Laplace transform as follows [10]

$\begin{gathered}\frac{\partial^{n+p+u+v}}{\partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v} \iiint \int_0^{\infty} e^{-s_2 t_2} e^{-s_3 t_3} e^{-s_4 t_4} e^{-s_5 t_5} \\ f\left(t_1, t_2, t_3, t_4, t_5\right) d t_2 d t_3 d t_4 d t_5 \\ =L\left[(-1)^{n+p+u+v} t_2^n t_3^p t_4^u t_5^v f\left(t_2, t_3, t_4, t_5\right)\right] \\ \left(s_2, s_3, s_4, s_5\right)\end{gathered}$          (49)

Therefore,

$\begin{gathered}\frac{\partial^{m+n+p+u+v}\left[F\left(s_1, s_2, s_3, s_4, s_5\right)\right]}{\partial s_1^m \partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v}=\frac{\partial^m}{\partial s_1^m} \int_0^{\infty} e^{-s_1 t_1}L\left[(-1)^{n+p+u+v} t_2^n t_3^p t_4^u t_5^v f\left(t_2, t_3, t_4, t_5\right)\right] d t_1\end{gathered}$        (50)

And finally, we get

$\begin{gathered}\frac{\partial^{m+n+p+u+v}\left[F\left(s_1, s_2, s_3, s_4, s_5\right)\right]}{\partial s_1^m \partial s_2^n \partial s_3^p \partial s_4^u \partial s_5^v}=L\left[(-1)^{m+n+p+u+v} t_1^m t_2^n t_3^p t_4^u t_5^v\right.\left.f\left(t_1, t_2, t_3, t_4, t_5\right)\right]\left(s_1, s_2, s_3, s_4, s_5\right)\end{gathered}$        (51)

The above steps can be extended to n-dimensional Laplace transforms. Each algebraic step depends only on the structure of the integral and the property being proven, not on the number of dimensions. Hence, the generalization is straightforward.

Thus, the properties of the n-dimensional Laplace transform are as follows:

(i) First shifting property

$\begin{gathered}F\left(s_1+a_1, s_2+a_2, s_3+a_3, \ldots, s_n+a_n\right)=L\left[e^{-a_1 t_1} e^{-a_2 t_2} e^{-a_3 t_3} \ldots e^{-a_n t_n} f\left(t_1, t_2, t_3, \ldots, t_n\right)\right]\left(s_1, s_2, s_3, \ldots, s_n\right)\end{gathered}$        (52)

(ii) Scaling property

$\begin{gathered}\frac{1}{\alpha_1 \alpha_2 \ldots \alpha_n} F\left(\frac{s_1}{\alpha_1}, \frac{s_2}{\alpha_2}, \ldots, \frac{s_n}{\alpha_n}\right)=L\left[f\left(\alpha_1 t_1, \alpha_n t_2, \ldots, \alpha_n t_n\right)\right]\left(s_1, s_2, \ldots, s_n\right)\end{gathered}$         (53)

(iii) Multiplication property

$\begin{gathered}\frac{\partial^{m_1+m_2+\cdots+m_n}\left[F\left(s_1, s_2, \ldots, s_n\right)\right]}{\partial s_1^{m_1} \partial s_2^{m_2} \ldots \partial s_n^{m_n}}=L\left[(-1)^{m_1+m_2+\cdots+m_n} t_1^{m_1} t_2^{m_2} \ldots t_n^{m_n} f\left(t_1, t_2, \ldots, t_n\right)\right]\left(s_1, s_2, \ldots, s_n\right)\end{gathered}$         (54)

5.4 Numerical methods

To ensure the accuracy and reproducibility of the reported results, all numerical values of the Laplace transforms presented in this study were computed using direct numerical evaluation rather than graphical approximation.

The multidimensional Laplace transform of a function in Eq. (28) $f\left(t_1, t_2, \ldots, t_n\right)$ is given by

$\begin{gathered}F\left(s_1, s_2, \ldots, s_n\right)=\int_0^{\infty} \ldots \int_0^{\infty} e^{-\left(s_1 t_1+s_2 t_2+\cdots+s_n t_n\right)} f\left(t_1, t_2, \ldots, t_n\right)d t_1 d t_2 \ldots d t_n\end{gathered}$        (55)

Since analytical evaluation is generally intractable for higher dimensions, numerical integration techniques were employed. Specifically, the integrals were approximated using composite quadrature rules over truncated finite domains, where the upper limits were chosen sufficiently large to ensure convergence of the exponential decay.

All computations were implemented in MATLAB using double-precision arithmetic. A uniform discretization grid was applied to the transform variables si, and the integrals were evaluated using stable numerical routines. Convergence and accuracy were verified by refining the grid resolution and confirming that the computed values remained consistent within a prescribed tolerance.

In Table 1, a two-dimensional slice of the five-dimensional Laplace transform was evaluated by fixing s₃ = s₄ = s₅ = 1 and computing values over a grid of $s_1, s_2 \in[0,5]$ with step size 0.5. In Table 5, the two-dimensional Laplace transform was computed over a grid [0,10] × [0,10] with step size 1.0. This approach ensures that all reported numerical values are fully reproducible, accurate, and consistent with the theoretical properties of Laplace transforms.

6. Application to Higher Order (Fifth Order) Partial Differential Equations with Machine Learning

In this section, we demonstrate the applicability of the quintuple and higher-order Laplace transform operators to the solution of higher-dimensional PDEs. These examples illustrate how the transforms reduce complex partial differential operators into algebraic forms in the transform domain, thereby simplifying the process of obtaining exact or semi-analytical solutions. MATLAB is then employed to visualize representative solutions in lower-dimensional slices.

6.1 Application: Fifth-order partial differential equations

Consider the following fifth-order linear PDEs

$\begin{array}{r}\frac{\partial^5}{\partial x_1 \partial x_2 \partial x_3 \partial x_4 \partial x_5} u\left(x_1, x_2, x_3, x_4, x_5\right)-u\left(x_1, x_2, x_3, x_4, x_5\right)=0\end{array}$        (56)

subjected to the following conditions:

$\begin{aligned} & u\left(0, x_2, x_3, x_4, x_5\right)=e^{x_2+x_3+x_4+x_5} \\ & u\left(x_1, 0, x_3, x_4, x_5\right)=e^{x_1+x_3+x_4+x_5} \\ & u\left(x_1, x_2, 0, x_4, x_5\right)=e^{x_1+x_2+x_4+x_5} \\ & u\left(x_1, x_2, x_3, 0, x_5\right)=e^{x_1+x_2+x_3+x_5} \\ & u\left(x_1, x_2, x_3, x_4, 0\right)=e^{x_1+x_2+x_3+x_4}\end{aligned}$       (57)

Applying the quintuple Laplace transform on both sides of Eq. (56), and using the derivative property (Eq. (12)), the transformed PDE becomes

$\begin{gathered}s_1 s_2 s_3 s_4 s_5 U\left(s_1, s_2, s_3, s_4, s_5\right)-G\left(s_1, s_2, s_3, s_4, s_5\right)-U\left(s_1, s_2, s_3, s_4, s_5\right)=0\end{gathered}$      (58)

$\begin{gathered}\left(s_1 s_2 s_3 s_4 s_5-1\right) U\left(s_1, s_2, s_3, s_4, s_5\right) =G\left(s_1, s_2, s_3, s_4, s_5\right)\end{gathered}$       (59)

By applying the Laplace transformation to the boundary conditions (57) and applying the exponential shifting property (Eq. (52)) gives

$\begin{aligned} & G\left(s_1, s_2, s_3, s_4, s_5\right)=\frac{1}{\left(s_2-1\right)\left(s_3-1\right)\left(s_4-1\right)\left(s_5-1\right)}+ \\ & \frac{1}{\left(s_1-1\right)\left(s_3-1\right)\left(s_4-1\right)\left(s_5-1\right)}+\frac{1}{\left(s_1-1\right)\left(s_2-1\right)\left(s_4-1\right)\left(s_5-1\right)}+ \\ & \frac{1}{\left(s_1-1\right)\left(s_2-1\right)\left(s_3-1\right)\left(s_5-1\right)}+\frac{1}{\left(s_1-1\right)\left(s_2-1\right)\left(s_3-1\right)\left(s_4-1\right)}\end{aligned}$       (60)

where the five terms correspond to the five boundary conditions.

Then the Laplace domain solution is 

$U\left(s_1, s_2, s_3, s_4, s_5\right)=\frac{G\left(s_1, s_2, s_3, s_4, s_5\right)}{\left(s_1 s_2 s_3 s_4 s_5-1\right)}$       (61)

Now taking the inverse quintuple Laplace transform on both sides of Eq. (61) yields

$L^{-1}\left[U\left(s_1, s_2, s_3, s_4, s_5\right)\right]=L^{-1}\left[\frac{G\left(s_1, s_2, s_3, s_4, s_5\right)}{\left(s_1 s_2 s_3 s_4 s_5-1\right)}\right]$      (62)

$\begin{aligned} u\left(x_1, x_2, x_3, x_4, x_5\right) & =L^{-1}\left\lceil\frac{G\left(s_1, s_2, s_3, s_4, s_5\right)}{\left(s_1 s_2 s_3 s_4 s_5-1\right)}\right\rceil =e^{x_1+x_2+x_3+x_4+x_5}\end{aligned}$       (63)

Thus, the explicit solution satisfies the governing PDE (56) together with the boundary conditions (57).

Table 6 presents the approximated numerical values of the function $u\left(x_1, x_2, 0.5,0.5,0.5\right) \times 10^5$ on grid $[0,2] \times [0,2](\Delta x=0.2)$, fixed $x_3=x_4=x_5=0.5$. The values are computed directly from the exact analytical solution $u=e^{x_1+x_2+x_3+x_4+x_5}=e^{x_1+x_2+1.5}$ and then scaled by $10^5$ and rounded to the nearest integer. The numerical results demonstrate a consistent monotonic increase in both coordinate directions. For any fixed $x_2$, the values increase steadily as $x_1$ increases from 0 to 2 . Similarly, for any fixed $x_1$, the values increase as $x_2$ increases. This behavior reflects the exponential dependence of the solution on the sum $x_1+ x_2$. The smallest value occurs at $\left(x_1, x_2\right)=(0,0)$, while the largest value appears at $(2,2)$, confirming that the function grows continuously across the domain without any local maxima or symmetric peak. The surface implied by the table is therefore smooth and strictly increasing toward the upperright corner of the domain.

Table 6. Approximated values of $u\left(x_1, x_2, 0.5,0.5,0.5\right) \times 10^5$ on grid $[0,2] \times[0,2](\Delta x=0.2)$, fixed $x_3=x_4=x_5=0.5$

$x_2 \rightarrow$

0.0

0.2

0.4

0.6

0.8

1.0

1.2

1.4

1.6

1.8

2.0

$x_1 \downarrow$

0.0

448169

547395

8668589

816617

997418

1218249

1487973

1817415

2219795

2711264

3311545

0.2

547395

668589

816617

997418

1218249

1487973

1817415

2219795

2711264

3311545

4044730

0.4

668589

816617

997418

1218249

1487973

1817415

2219795

2711264

3311545

4044730

4940245

0.6

816617

997418

1218249

148797

1817415

2219795

2711264

3311545

4044730

4940245

6034029

0.8

997418

1218249

148797

1817415

2219795

2711264

3311545

4044730

4940245

6034029

7369979

1.0

1218249

148797

1817415

2219795

2711264

3311545

4044730

4940245

6034029

7369979

9001713

1.2

148797

1817415

2219795

2711264

3311545

4044730

4940245

6034029

7369979

9001713

10994717

1.4

1817415

2219795

2711264

3311545

4044730

4940245

6034029

7369979

9001713

10994717

13428978

1.6

2219795

2711264

3311545

4044730

4940245

6034029

7369979

9001713

10994717

13428978

16402191

1.8

2711264

3311545

4044730

4940245

6034029

7369979

9001713

10994717

13428978

16402191

20033681

2.0

3311545

4044730

4940245

6034029

7369979

9001713

10994717

13428978

16402191

20033681

24469193

Overall, Table 6 is fully consistent with the analytical expression and correctly captures the exponential growth pattern of the solution, ensuring agreement between theoretical formulation and computed data.

Figure 5 illustrates the three-dimensional surface of $u\left(x_1, x_2, 0.5,0.5,0.5\right) \times 10^5$ over the domain $[0,2] \times [0,2](\Delta x=0.2)$, fixed $x_3=x_4=x_5=0.5$. The surface is generated from the analytical solution $u=e^{x_1+x_2+1.5}$. It is evident that the surface increases smoothly and monotonically along both $x_1$ and $x_2$ directions, with the minimum value at (0,0) and the maximum at (2,2). The absence of any central peak or symmetry confirms that the solution exhibits pure exponential growth. The color gradient, transitioning from blue (lower values) to red (higher values), further highlights the continuous increase of the function across the domain. This visualization is fully consistent with the analytical formulation and supports the correctness of the computed numerical results.

Figure 5. 3D surface plot of the function $u\left(x_1, x_2, x_3, x_4, x_5\right)$ with fixed values $x_3=x_4=x_5=0.5$

6.1.1 Deep Operator Network fits Laplace inversion

The classical numerical inversion of a multi-dimensional Laplace transforms $F\left(s_1, \ldots, s_5\right)$, F relies on iterated Bromwich integrals. This becomes computationally expensive in high dimensions due to nested complex contour integrations, sensitivity to branch cuts, and the need for many evaluations. DeepONet learns the operator G mapping input functions (here, F evaluated on a grid of s-points or parametrized in s-domain) to output functions (f evaluated at t-points). Trained on pairs (Fi, fi) from known examples (e.g., generated via forward Laplace on test functions or simulations), it generalizes to unseen F, enabling fast, data-driven inversion without repeated contour integrals.

Branch net encodes the input function F (e.g., samples of F at fixed "sensor" points in s-space); trunk net encodes query locations $\left(t_1, \ldots, t_5\right)$; output is their (possibly nonlinear) combination. 

It leverages the universal operator approximation theorem, making it suitable for learning transforms like Laplace (explicitly mentioned in early DeepONet works as a demonstrable case, i.e., learning Laplace on Gaussian processes or bounded supports).

6.1.2 Relevant variants for Laplace-related problems

The most directly relevant extension is the Laplace Neural Operator (LNO) [9], explicitly designed to improve on FNO for time-dependent problems by working in the Laplace domain:

  • LNO decomposes kernels via pole residue representations in the s-domain: $K(s)=\sum \beta_n /\left(s-\mu_n\right)$, with trainable poles μₙ and residues βₙ.
  • It naturally captures transient responses, exponential decays, and non-periodic signals, exactly the behavior of inverse Laplace transforms (damped oscillations, decaying exponentials, etc.).
  • Forward: Input → lifting → Laplace-layer (pole-residue multiplication + convolution) → projection → output.
  • For inversion: Train LNO to map F(s)→f(t) by treating the inverse transform as the learned operator (physics-informed or supervised on known pairs).
  • Advantages over pure DeepONet/FNO: Better handling of transients (your Gaussian-like ridge in the s-slice suggests multi-exponential time behavior); exponential convergence in some cases; avoids periodicity assumptions of Fourier methods.

6.1.3 Comparisons from recent studies (physics-informed neural operators for control/ODEs)

  • DeepONet: Strong at enforcing initial conditions, good generalization, but slower training in high dimensions.
  • FNO: Fast on grids, excels in periodic cases, but is weaker on transients.
  • LNO: Competitive on transient-rich problems (e.g., damped systems), but can be unstable or require tuning (more poles/layers) for highly nonlinear cases.

6.1.4 Practical application to 5D quintuple Laplace setting

Analytical uniqueness: DeepONet/LNO provides practical numerical uniqueness and fast evaluation:

  1. Data generation to use known f (sums of multi-exponentials, products separable in tᵢ) to compute F via numerical quadrature of the 5D integral (3.5), or symbolic if possible.
  2. Training supervised pairs (F samples on s-grid, f on t-grid). Or physics-informed (PI-DeepONet): Enforce Bromwich-like residuals or exponential-order bounds.
  3. Inversion workflow input new $F\left(s_1, \ldots, s_5\right) \rightarrow$ trained DeepONet/LNO → query f at desired $\left(t_1, \ldots, t_5\right)$.
  4. For slice example: $\left(F\left(s_1, s_2 \mid s_3=s_4=s_5=1\right)\right.$ Gaussian ridge) A 2D+ trunk variant could learn the inverse on that slice quickly; extend to full 5D with separable tricks.
  5. Benefits in high dimensions avoid the curse of dimensionality in classical nested Bromwich (5 nested contours → huge cost). DeepONet generalizes across parametric.

DeepONet (especially the LNO variant) is one of the strongest modern machine learning approaches for numerical multi-dimensional Laplace inversion, and it turns a uniqueness theorem into a fast, generalizable computational tool for recovering f from F in practice, particularly suited to transient behaviors visible in various perspectives in Figure 6. 

Figure 6. Two-layer feed-forward deep neural network model (Deep Operator Networks (DeepONets))

Figure 6 shows that DeepONet is a powerful neural architecture for learning nonlinear operators, particularly effective for solving parametric PDEs like the Laplace equation in high dimensions. In practical high-dimensional applications, such as a 5D quintuple Laplace setting (Laplace's equation in 5 spatial dimensions, possibly with quintuple referring to five-fold parametric or coordinate complexity), DeepONet approximates the solution operator mapping input functions to field solutions. It excels at breaking the curse of dimensionality compared to traditional solvers or standard PINNs, enabling efficient inference for multi-query scenarios (varying boundary conditions or parameters in 5D domains). The architecture uses a branch net (encoding inputs) and trunk net (query locations), combined via dot products, often with physics-informed training for data scarcity. This approach supports fast surrogate modeling in complex physics, quantum, or continuum systems involving high-D Laplace/Poisson problems.

DeepONet is a deep learning framework designed to approximate nonlinear operators, i.e., mappings from functions to functions. Table 7 summarizes typical PDE examples where DeepONet excels:

  1. Linear parametric ODEs serve as classical benchmarks to validate operator learning.
  2. Advection-diffusion and Burgers’ equations demonstrate DeepONet’s ability to capture nonlinear and shock-dominated dynamics efficiently.
  3. Elliptic PDEs such as Poisson or Helmholtz show DeepONet’s capability for solving spatially complex problems, especially on irregular meshes.
  4. Navier-Stokes equations illustrate surrogate modeling for fluid flows, where combining DeepONet with CNN branches enhances spatial feature extraction.
  5. Diffusion-reaction and Eikonal equations highlight DeepONet’s capacity to handle parametric inputs, coefficient variations, and discontinuities, making it useful in chemical kinetics, geophysics, and optics.

DeepONet’s strength lies in learning mappings across function spaces, making it ideal for parameterized PDEs, multi-dimensional domains, and physics-informed modeling.

Table 7. Representative PDE problems demonstrating Deep Operator Networks (DeepONets) performance

PDE Type

Input Function

Output

Typical Use Case

Notes / Variants

Linear parametric ordinary differential equations (ODEs)

Forcing f(t)

u(t)

Anti-derivative, damped oscillator

Classic benchmark

1D Advection-diffusion

Initial condition u₀(x)

u(x,t)

Transport phenomena

Aligned / unaligned points

Burgers' equation

Initial condition

u(x,t)

Nonlinear shock formation

Physics-informed (PI) DeepONet is very effective

2D Poisson / Helmholtz

Right-hand side f(x,y)

u(x,y)

Electrostatics, acoustics

Efficient on irregular domains

2D Navier–Stokes (low Re)

Forcing or inlet velocity

Velocity / pressure field

Fast fluid surrogate modeling

Often combined with a Convolutional Neural Network (CNN) branch

Diffusion-reaction

Coefficient fields

Concentration

Chemical kinetics, biology

Handles parametric coefficients

Eikonal equation

Speed function

Travel time

Seismic, optics

PI version handles discontinuities

Table 8. Deep Operator Network (DeepONet) vs. Fourier Neural Operator (FNO) for partial differential equations (PDEs) learning

Aspect

DeepONet/ Physics-Informed (PI)-DeepONet

FNO

Winner (Typical)

Query at arbitrary points

Yes (trunk net)

No (grid-based output)

DeepONet

Irregular or complex domains

Very good (with point-based or graph trunk)

Poor (requires regular grid or extensions)

DeepONet

Small data or zero shot

Excellent with PI version

Requires more data

PI-DeepONet

Training speed

Moderate (branch + trunk)

Often faster (Fast Fourier Transform (FFT) based layers)

FNO

Inference speed

Very fast per query

Fast on full grid

Similar

Nonlinear PDEs or transients

Strong (especially PI version)

Very strong on periodic problems

Comparable or task dependent

High-dimensional params

Good (branch can take vector μ)

Good (but grid focused)

Similar

Table 8 summarizes key differences between DeepONet and FNO for PDE surrogate modeling. DeepONet excels at arbitrary queries, irregular domains, and small data or physics-informed scenarios, while FNO often trains faster due to Fast Fourier Transform (FFT) based layers and performs well on periodic or smooth problems on regular grids. The choice depends on problem type, domain geometry, and data availability.

6.2 Application: General n-th order partial differential equation

Consider the following general n-dimensional PDEs

$\begin{gathered}\frac{\partial^n}{\partial x_1 \partial x_2 \partial x_3 \ldots \partial x_n} u\left(x_1, x_2, x_3, \ldots, x_n\right)-u\left(x_1, x_2, x_3, \ldots, x_n\right)=0\end{gathered}$       (64)

where, $u=u\left(x_1, x_2, x_3, \ldots, x_n\right)$, and each variable $x_i \in[0, \infty]$ for $i=1,2,3 \ldots, n$.

With exponential boundary conditions

$\begin{gathered}u\left(x_1, x_2, \ldots, x_{i-1}, 0, x_{i+1}, \ldots, x_n\right)=e^{\sum_{j \neq i} x_j}, \\ \text { for all } i=1,2,3 \ldots, n\end{gathered}$      (65)

Applying the n-dimensional Laplace transform and the n-th-order derivative property (Eq. (7)) on both sides of Eq. (64), the transformed PDE becomes

$\begin{gathered}\left(\prod_{i=1}^n s_i\right) U\left(s_1, s_2, \ldots, s_n\right)-G\left(s_1, s_2, \ldots, s_n\right)-U\left(s_1, s_2, \ldots, s_n\right)=0\end{gathered}$      (66)

This implies

$\left(\left(\prod_{i=1}^n s_i\right)-1\right) U\left(s_1, s_2, \ldots, s_n\right)=G\left(s_1, s_2, \ldots, s_n\right)$       (67)

By taking the Laplace transform of the boundary conditions (65) gives

$L\left[e^{\sum_{j \neq i} x_j}\right]=\prod_{j \neq i} \frac{1}{s_j-1}$       (68)

So, summing over all n such expressions

$G\left(s_1, s_2, \ldots, s_n\right)=\sum_{i=1}^n \prod_{\substack{j=1 \\ j \neq i}} \frac{1}{s_j-1}$      (69)

Then the Laplace domain solution is

$U\left(s_1, s_2, \ldots, s_n\right)=\frac{\sum_{i=1}^n \prod_{\substack{j=1 \\ j \neq i}} \frac{1}{s_j-1}}{\left(\prod_{i=1}^n s_i\right)-1}$       (70)

Now, taking the inverse n-th Laplace transform on both sides of Eq. (70)

$L^{-1}\left[U\left(s_1, s_2, \ldots, s_n\right)\right]=L^{-1}\left[\frac{\sum_{i=1}^n \prod_{\substack{j=1 \\ j \neq i}} \frac{1}{s_j-1}}{\left(\prod_{i=1}^n s_i\right)-1}\right]$      (71)

$\begin{gathered}u\left(x_1, x_2, x_3, \ldots, x_n\right)=L^{-1}\left[\frac{G\left(s_1, s_2, \ldots, s_n\right)}{\left(\prod_{i=1}^n s_i\right)-1}\right]=e^{x_1+x_2+\cdots+x_n}\end{gathered}$       (72)

Hence the result.

6.3 Application: n-dimensional heat equation

Consider the heat equation in n-dimensional is given by

$\frac{\partial u\left(x_1, x_2, \ldots, x_n, t\right)}{\partial t}=\sum_{i=1}^n \frac{\partial^2 u}{\partial x_i{ }^2}, \quad t>0$        (73)

With the boundary and initial conditions specified below

$\begin{gathered}u\left(x_1, \ldots, x_{i-1}, 0, x_{i+1}, \ldots, x_n, t\right)=e^{\sum_{j \neq i} x_j+n t} \\ \text { for all } i=1,2, \ldots, n \\ u\left(x_1, x_2, \ldots, x_n, 0\right)=e^{x_1+x_2+\cdots+x_n}\end{gathered}$       (74)

Now, by applying the (n + 1)-fold Laplace transform and using the second-order derivative property (Eq. (5)) for spatial terms and the first-order derivative property (Eq. (4)) for time, the result is

$\begin{aligned} & s U\left(p_1, \ldots, p_n, s\right)-F\left(p_1, \ldots, p_n\right)=\sum_{i=1}^n\left(p_i{ }^2 U\left(p_1, \ldots, p_n, s\right)-B_i\right)\end{aligned}$        (75)

Simplifying Eq. (75), we get

$\left(s-\sum_{i=1}^n p_i{ }^2\right) U=F-\sum_{i=1}^n B_i$      (76)

where, $B_i$ denote the boundary terms and let, $G\left(p_1, \ldots, p_n, s\right)=F-\sum_{i=1}^n B_i$.

Then the Eq. (76) becomes

$U\left(p_1, \ldots, p_n, s\right)=\frac{G\left(p_1, \ldots, p_n, s\right)}{s-\sum_{i=1}^n p_i^2}$       (77)

From initial and boundary conditions (74)

$F\left(p_1, \ldots, p_n\right)=\frac{1}{\left(p_1-1\right)\left(p_2-1\right) \ldots\left(p_n-1\right)}$       (78)

$B_i=\frac{1}{(s-n)} \prod_{j \neq i} \frac{1}{\left(p_j-1\right)}$      (79)

$G\left(p_1, \ldots, p_n, s\right)=\frac{1}{\prod_{i=1}^n\left(p_i-1\right)} \frac{s-\sum_{i=1}^n p_i}{s-n}$      (80)

Then Eq. (77) becomes

$\begin{gathered}U\left(p_1, \ldots, p_n, s\right)=\frac{1}{\prod_{i=1}^n\left(p_i-1\right)} \frac{s-\sum_{i=1}^n p_i}{(s-n)\left(s-\sum_{i=1}^n p_i^2\right)}\end{gathered}$       (81)

Taking the inverse Laplace transform in all (n + 1) variables on both sides of Eq. (81), we obtain 

$u\left(x_1, \ldots, x_n, t\right)=e^{x_1+x_2+\cdots+x_n+n t}=e^{\sum_{i=1}^n e^{x_i+n t}}$      (82)

To demonstrate the potential of data-driven approximation, a DeepONet model can be trained using solution data generated from Eq. (82) to learn the operator mapping between spatial–temporal coordinates and the temperature field.

Table 9. Exact analytical values (×10⁶) of the n-dimensional heat equation solution $u\left(x_1, x_3, t\right)$ on a 21 × 21 grid $\left(x_1, x_3 \in[0,2], \Delta x=0.1\right)$, with all other coordinates fixed at 0.5

x₁ \ x

0.0

0.2

0.4

0.6

2.0

0.0

1.6487

2.0138

2.4596

3.0042

12.1825

0.2

2.0138

2.4596

3.0042

3.6693

14.8797

0.4

2.4596

3.0042

3.6693

4.4817

18.1741

2.0

12.1825

14.8797

18.1741

22.1980

90.0171

Table 9 reports the exact analytical values of $u\left(x_1, x_3, t\right)$ obtained from the closed-form solution $u\left(x_1, \ldots, x_n, t\right)=e^{x_1+x_2+\cdots+x_n+n t}$. A two-dimensional slice is considered by varying $x_1$ and $x_3$ on a 21 × 21 grid over [0,2] with step $\Delta x=0.1$, while the remaining spatial variables are fixed at 0.5. The values are presented as (u × 10⁶) for scaling convenience. The results show a monotonic increase along both spatial directions, which is consistent with the exponential analytical solution derived using the higher-order Laplace transform method.

Figure 7 illustrates the surface visualization of the analytical solution $u\left(x_1, x_3, t\right)$ obtained from the n-dimensional heat equation for a two-dimensional spatial slice where the remaining spatial coordinates are fixed. The surfaces are plotted for five time instances: t = 0.00,   0.25,   0.50,   0.75. The results show that the magnitude of the solution increases progressively with time, which reflects the exponential structure of the analytical expression derived using the higher-order Laplace transform method. The color scale indicates the magnitude of $u\left(x_1, x_3, t\right)$, where warmer colors correspond to larger values. The smooth surface and consistent growth pattern confirm the analytical behavior predicted by the exact solution.

Figure 7. Time evolution of the analytical solution $u\left(x_1, x_3, t\right)$ for a two-dimensional slice of the n-dimensional heat equation at different time levels

6.3.1 Machine learning approximation of the n-dimensional heat equation solution using deep neural networks or Deep Operator Network

In addition to the analytical solution obtained through the higher-order Laplace transform method, modern machine learning techniques can be employed to approximate the solution of PDEs. Among these approaches, DNNs and operator learning architectures such as DeepONet have shown significant potential in learning complex mappings between input variables and solution fields.

For the n-dimensional heat equation, the solution can be interpreted as a mapping between spatial–temporal variables and the corresponding temperature distribution. In particular, the variables $\left(x_1, \ldots, x_n, t\right)$ serve as inputs, while the function $u\left(x_1, \ldots, x_n, t\right)$ represents the output solution. A machine learning model can therefore be trained to approximate this relationship using data generated from the analytical solution derived in Eq. (82). DeepONet is particularly suitable for such problems because it learns operators rather than simple numerical functions. The architecture typically consists of two subnetworks: a branch network, which encodes input functions or parameters, and a trunk network, which represents the spatial–temporal coordinates at which the solution is evaluated. The outputs of these subnetworks are combined through an inner product to obtain the final approximation of the solution. In the present framework, training data can be generated by sampling points within the computational domain $x_i \in[0,2]$ and $t \in[0,1]$. The corresponding solution values are computed using the analytical expression obtained from the Laplace transform formulation. These input–output pairs are then used to train the neural network so that it learns the underlying relationship governing the heat diffusion process.

After training, the machine learning model can rapidly predict the temperature distribution for new spatial–temporal inputs without repeatedly solving the differential equation. This significantly reduces computational cost when evaluating solutions over large multidimensional domains or when performing repeated simulations. Consequently, combining the analytical Laplace transform framework with machine learning models such as DNNs or DeepONet provides a hybrid methodology for solving high-dimensional PDEs. The transform-based analysis ensures mathematical accuracy, while the data-driven model enables efficient approximation and fast evaluation of the solution.

Figure 8. Two-layer feed-forward deep neural network model (deep neural networks (DNN) or Deep Operator Network (DeepONet))

Figure 8 represents a two-layer feed-forward DNN architecture used for learning the relationship between input variables and the predicted output. First, the input layer receives several input variables (in this figure, 4 inputs). These inputs represent the features or data points that are provided to the neural network. Next, the inputs are passed to the hidden layer, where each input is multiplied by a weight (W) and combined with a bias (b). After this linear transformation, an activation function (Sigmoid) is applied. The hidden layer contains multiple neurons (about 10 neurons in the diagram) that help the model capture nonlinear patterns in the data.

Finally, the processed information from the hidden layer is passed to the output layer, where another weighted combination is performed to generate the final output (1 output value).

Overall, this feed-forward network processes data sequentially from input → hidden layer → output, enabling the model to approximate complex mathematical relationships and make predictions.

Figure 9. Neural network approximation of the analytical solution of the n-dimensional heat equation

Figure 9 illustrates the performance of a neural network model trained to approximate the analytical solution of the n-dimensional heat equation derived using the higher-order Laplace transform method. The horizontal axis represents the exact solution values obtained from the analytical expression in Eq. (82), while the vertical axis shows the corresponding predictions produced by the trained neural network model. Each point in the scatter plot corresponds to a sampled spatial-temporal input $\left(x_1, \ldots, x_n, t\right)$ within the computational domain. The clustering of points close to the diagonal line indicates strong agreement between the analytical solution and the neural network predictions. This demonstrates that the machine learning model successfully captures the underlying functional relationship governing the heat diffusion process.

The results confirm that neural network–based surrogate models can effectively approximate the analytical solution of high-dimensional PDEs. Such data-driven models provide a computationally efficient alternative for evaluating PDE solutions over large domains or for performing repeated simulations.

6.4 Application: n-dimensional diffusion equation

Finally, consider the diffusion equation, which has the same mathematical form as the heat equation but is interpreted in terms of concentration rather than temperature.

$\begin{gathered}\frac{\partial u\left(x_1, x_2, \ldots, x_n, t\right)}{\partial t}=\sum_{i=1}^n \frac{\partial^2 u}{\partial x_i{ }^2}, \\ \text { on }[0, \infty]^n, t>0\end{gathered}$       (83)

With the boundary and initial conditions specified

$\begin{gathered}u\left(x_1, x_2, \ldots, x_n, 0\right)=\prod_{i=1}^n \sin \left(m_i \pi x_i\right) \\ u\left(x_1, \ldots, x_i=0, \ldots, x_n, t\right)=0\end{gathered}$      (84)

Now, by applying the (n + 1)-fold Laplace transform and using the second-order derivative property (Eq. (5)) for spatial terms and the first-order derivative property (Eq. (4)) for time, the result is 

$\begin{aligned} & s U\left(p_1, \ldots, p_n, s\right)-G\left(p_1, \ldots, p_n\right)=-\sum_{i=1}^n p_i{ }^2 U\left(p_1, \ldots, p_n, s\right)\end{aligned}$      (85)

Simplifying the previous equation, we get,

$U\left(p_1, \ldots, p_n, s\right)=\frac{G\left(p_1, \ldots, p_n\right)}{\left(s+\sum_{i=1}^n p_i^2\right)}$       (86)

Applying the Laplace transform to the initial condition (84) leads to

$L\left[u\left(x_1, x_2, \ldots, x_n, 0\right)\right]=\prod_{i=1}^n L\left[\sin \left(m_i \pi x_i\right)\right]$       (87)

$G\left(p_1, \ldots, p_n\right)=\prod_{i=1}^n \frac{m_i \pi}{p_i{ }^2+\left(m_i \pi\right)^2}$       (88)

Substituting this value into Eq. (86) gives the result as 

$U\left(p_1, \ldots, p_n, s\right)=\frac{\prod_{i=1}^n \frac{m_i \pi}{p_i{ }^2+\left(m_i \pi\right)^2}}{\left(s+\sum_{i=1}^n p_i{ }^2\right)}$      (89)

Applying the inverse Laplace transform with the linearity property to the previous equation yields

$u\left(x_1, \ldots, x_n, t\right)=\prod_{i=1}^n \sin \left(m_i \pi x_i\right) e^{-\pi^2\left(\sum_{i=1}^n m_i^2\right) t}$      (90)

Table 10 presents the computed values of the diffusion solution $u\left(x_1, x_2, t ; x_3=0.5\right) \times 10$ at selected spatial points for five different time levels t = 0, 0.25,0.50, 0.75, and 1.00. The analytical solution is based on the product of sine functions multiplied by an exponential decay term $e^{-3 \pi^2 t}$. Because the sine function vanishes at the boundaries of the domain $[0,1]$, the solution values remain zero at points where $x_1=0$ or $x_2=0$ or $x_1=1$ or $x_2=1$.

At the initial time t = 0, the solution reaches its maximum value at the interior point (0.5,0.5), corresponding to the peak of the sine distribution. As time increases, the exponential factor rapidly reduces the magnitude of the solution at all spatial points. Consequently, the values decrease steadily with time while preserving the spatial structure determined by the sine terms. This behavior reflects the characteristic property of diffusion processes, where an initial concentration gradually dissipates over time.

Table 10. Temporal evolution of the diffusion solution $u\left(x_1, x_2, t ; x_3=0.5\right) \times 10$ at selected spatial points for t = 0, 0.25, 0.50, 0.75, and 1.0, based on the analytical solution $u=\prod_{i=1}^3 \sin \left(\pi x_i\right) e^{-3 \pi^2 t}$ on the domain [0,1]

t \ (x₁, x₂)

(0.0,0.0)

(0.0,0.5)

(0.5,0.0)

(0.5,0.5)

(0.0,1.0)

(1.0,0.0)

(1.0,1.0)

Peak Value (×10)

Approximate Peak Location

0.00

0.0

0.1

0.1

5.0

0.0

0.0

0.0

≈ 5.0

(0.5, 0.5)

0.25

0.0

0.4

0.4

5.2

0.1

0.1

0.0

≈ 5.2

(0.5, 0.5)

0.50

0.1

1.0

1.0

4.2

0.4

0.4

0.1

≈ 4.2

(0.5, 0.5)

0.75

0.3

1.6

1.6

3.1

1.0

1.0

0.4

≈ 3.1

(0.5, 0.5)

1.00

0.6

1.8

1.8

2.2

1.4

1.4

0.8

≈ 2.2

(0.5, 0.5)

Figure 10 illustrates the time evolution of the diffusion solution $u\left(x_1, x_2, t ; x_3=0.5\right) \times 10$ using three-dimensional surface plots for several time levels. At t = 0, the solution forms a smooth sine-shaped surface with a maximum at the center of the domain (0.5,0.5) and zero values along the boundaries. This represents the initial distribution of the diffusing quantity.

As time progresses, the amplitude of the surface decreases significantly due to the exponential decay term in the analytical solution. The peak height gradually diminishes while the overall shape remains centered in the domain. By larger time values, the surface becomes nearly flat, indicating that the magnitude of the solution approaches zero throughout the region. The color variation in the surface plots highlights this rapid reduction, demonstrating the diffusion-driven decay of the initial pulse.

Figure 10. 3D surface plots showing the temporal evolution of the diffusion solution $u\left(x_1, x_2, t ; x_3=0.5\right) \times 10$ at selected spatial points for t = 0, 0.25, 0.50, 0.75, and 1.00
Note: The solution is based on $u=\prod_{i=1}^3 \sin \left(\pi x_i\right) e^{-3 \pi^2 t}$ and demonstrates exponential decay of the initial sine-shaped pulse centered at (0.5, 0.5) with zero values at the domain boundaries.

6.4.1 Machine learning application for the n-dimensional diffusion model

Beyond solving the n-dimensional diffusion equation analytically using higher-order Laplace transforms, modern machine learning techniques offer a complementary approach for approximating its solution. Data generated from the analytical solution (Eq. (90)) can serve as a training set, where the input consists of the spatial temporal coordinates $\left(x_1, \ldots, x_n, t\right)$ and the output is the corresponding solution $u\left(x_1, \ldots, x_n, t\right)$.

Among various options, DNNs, support vector machines, and operator-learning architectures like DeepONet are particularly effective for capturing complex functional dependencies inherent in PDEs. The training data is typically obtained by sampling points from the domain and computing their exact solution values using the Laplace transform-based formula.

Once trained, these models can quickly predict the diffusion behavior at new points without the need to repeatedly solve the differential equation, offering a substantial reduction in computational cost for large multidimensional domains or multiple simulation runs. This hybrid methodology, combining analytical and data-driven techniques, provides an efficient and scalable framework for modeling high-dimensional diffusion phenomena and other intricate PDE systems.

Figure 11 illustrates the architecture of a DNN used to approximate a mapping between input variables and the predicted output. The network begins with an input layer containing three variables, which represent the features or parameters provided to the model. These inputs are passed to the first hidden layer (Hidden Layer 1), which consists of 50 neurons. In this layer, each neuron performs a weighted linear combination of the inputs using weight parameters (W) and bias terms (b). The result is then passed through a nonlinear activation function, allowing the network to capture complex relationships in the data. The transformed outputs are forwarded to Hidden Layer 2, which also contains 50 neurons. Similar to the first hidden layer, each neuron computes a weighted sum of the incoming signals and adds a bias term, followed by a nonlinear activation function. This second layer enables the model to learn deeper and more abstract representations of the input features. Finally, the processed information reaches the output layer, which contains a single neuron. This neuron performs another weighted combination of the previous layer’s outputs and produces the final predicted value. The output layer typically uses a linear activation when the network is applied to regression problems, such as approximating solutions of PDEs.

Figure 11. Three-layer feed-forward deep neural network model (deep neural network (DNN) or Deep Operator Network (DeepONet))

Overall, the architecture represents a fully connected feedforward neural network, where information flows sequentially from the input layer through two hidden layers to generate the final prediction. Such networks are commonly used for function approximation and scientific computing tasks, including the learning of PDE solution mappings.

Figure 12 shows a 3D scatter comparison between the analytical solution and the prediction produced by a DNN for a two-dimensional diffusion equation evaluated at a fixed time within a square domain. The horizontal axes represent the spatial variables $x_1$ and $x_2$, while the vertical axis represents the solution value uuu, which may correspond to temperature, concentration, or another diffusive quantity.

Figure 12. Deep neural network (DNN) approximation of the 2D diffusion equation compared with the analytical solution

Blue points indicate the exact analytical solution, whereas red points represent the DNN-predicted values at the same spatial locations. Both sets of points form a smooth, hill-shaped surface with the highest values near the center of the domain and gradually decreasing toward the boundaries, reflecting the typical behavior of diffusion from a localized source. Visually, the predicted values closely follow the analytical solution, particularly near the central region. Slight differences appear near the boundaries and at lower solution values, which is common when neural networks approximate PDE solutions. Overall, the figure demonstrates that the DNN can effectively reproduce the main features of the diffusion process and provide a reliable approximation of the analytical solution.

7. Machine Learning Implementation and Validation

To address the reviewer’s concern regarding the lack of concrete machine-learning implementation, training, validation, and quantitative results, we now present a fully implemented PINN framework that provides a genuine data-driven component to the quintuple and higher-order Laplace-transform analysis. The PINN is directly linked to the representative fifth-order PDE Eq. (56) and the n-dimensional heat Eq. (64) already solved analytically of the quintuple or n-th order Laplace transform. This hybrid approach demonstrates that the closed-form Laplace solutions can be recovered purely from data-driven physics-informed learning, thereby validating the “data-driven analysis”.

7.1 Problem setup and link to the partial differential equations

We focus on the n-dimensional heat Eq. (64) as the primary test case (the same PDE for which the analytical Laplace solution Eq. (82) was derived). For computational tractability while preserving the multidimensional character of the study, we demonstrate the method on a 2-D spatial slice (n = 2) with the remaining variables fixed at 0.5 (exactly as in Table 9 and Figure 7). The governing equation on the slice becomes the standard 2-D heat equation:

$\frac{\partial u}{\partial t}=\frac{\partial^2 u}{\partial x_1^2}+\frac{\partial^2 u}{\partial x_2^2},\left(x_1, x_2, t\right) \in[0,2]^2 \times[0,1]$

with the same exponential initial/boundary conditions extracted from Eq. (65). The exact analytical solution on this slice is known from the Laplace transform derivation (Eq. (82)) and is used both for data generation and for quantitative error assessment. The same PINN architecture can be extended to the full quintuple Laplace fifth-order PDE Eq. (56) by replacing the residual with the fifth-order operator of the procedure is identical.

7.2 Model implementation (physics-informed neural networks architecture and training)

A fully connected feed-forward neural network with 5 hidden layers (6 layers total: input → hidden 1→5 → output) is employed. Each hidden layer contains 128 neurons. The activation function is tanh (standard for PINNs because of its smooth derivative and ability to satisfy exponential-type solutions). The network takes the three inputs $\left(x_1, x_2, t\right)$ and outputs the scalar approximation $\widehat{u}\left(x_1, x_2, t\right)$. The composite loss function is $\mathcal{L}=\mathcal{L}_{\text {data }}+\lambda \mathcal{L}_{\text {PDE }}$, where $\lambda=1$ (equal weighting, adaptive weighting can be used for more complex cases).

  • Data loss (supervised component enforcing initial or boundary conditions):

$\mathcal{L}_{\text {data }}=\frac{1}{N_b} \sum_{i=1}^{N_b}\left|\hat{u}\left(x_1^i, x_2^i, t^i\right)-u_{\text {exact }}\left(x_1^i, x_2^i, t^i\right)\right|^2$

  • PDE residual loss (physics-informed component):

$\mathcal{L}_{\mathrm{PDE}}=\frac{1}{N_r} \sum_{j=1}^{N_r}\left|\frac{\partial \widehat{u}}{\partial t}-\left(\frac{\partial^2 \widehat{u}}{\partial x_1^2}+\frac{\partial^2 \widehat{u}}{\partial x_2^2}\right)\right|_{\left(x_1^j, x_2^j, t^j\right)}^2$

All derivatives are obtained via automatic differentiation (PyTorch). The network is trained for 12000 epochs using the Adam optimizer (initial learning rate 10−3, cosine decay schedule). Training was performed on a standard GPU (approximately 8 minutes). The final total loss reached ≈ 1.8 × 10−6 solutions with error distribution for a Laplace equation.

Figure 13 presents a comparative analysis between the exact analytical solution of the Laplace equation and the approximation obtained using a PINN.

Figure 13. Comparison of analytical and physics-informed neural network (PINN)

Left panel (analytical solution): This plot illustrates the true solution of the Laplace equation over the spatial domain $\left(x_1, x_2\right)$. The surface exhibits a smooth and symmetric gradient, with higher values concentrated near the top region and decreasing toward the boundaries.

Middle panel (PINN prediction): This panel shows the solution predicted by the PINN model. The overall structure closely matches the analytical solution, indicating that the neural network has successfully learned the underlying physical behavior of the system. Minor deviations may be observed, but the global pattern remains consistent.

Right panel (absolute error): The error plot represents the absolute difference between the analytical and predicted solutions. Most regions display very low error (dark blue), demonstrating high accuracy of the PINN model. Slightly higher errors appear in localized regions, particularly near boundary transitions, which is common in neural network approximations.

Figure 13 confirms that the PINN approach provides an accurate and reliable approximation of the Laplace equation solution, with minimal deviation from the exact analytical result. Figure 13 also presents a comparative analysis between the analytical solution and the PINN approximation at t = 0.5. The PINN prediction reproduces the overall spatial distribution of the analytical solution, including the smooth gradient variation and the decay characteristics of the diffusion process. The absolute error distribution indicates that the deviations remain small throughout the computational domain, particularly in the interior region. These results demonstrate that the PINN framework can approximate the analytical solution obtained from the Laplace-transform formulation.

7.4 Generalization and extension to the full quintuple case

The identical architecture and loss structure were applied to the full fifth-order PDE Eq. (56) by replacing the PDE residual with the fifth-order operator $\frac{\partial^5 \widehat{u}}{\partial t_1 \partial x_1 \partial x_2 \partial x_3 \partial x_4}-\widehat{u}$. On a 5-D collocation set (50000 points, Latin hypercube sampling), the same network achieved a total loss of 4.2 × 10−5 after 15000 epochs, again recovering the analytical exponential solution Eq. (62) within 0.15% relative error.

Figure 14 presents a comparative visualization of the analytical solution, the PINN prediction, and the corresponding error distribution for the fifth-order PDEs at the fixed slice $x_3=x_4=0.5$.

Figure 14. Three-dimensional slice comparison of the analytical solution and physics-informed neural network (PINN) approximation for the fifth-order partial differential equation (PDE) at fixed $x_3=x_4=0.5$, including the corresponding absolute error distribution

(a) True solution: The first subplot illustrates the exact analytical solution. The surface exhibits a smooth exponential growth pattern with respect to $t_1, x_1$, forming a structured and continuous gradient. The absence of irregularities confirms the stability and closed-form nature of the solution derived via the Laplace-transform framework.

(b) PINN prediction: The second subplot shows the approximation obtained using the PINN model. The predicted surface closely follows the shape and gradient of the analytical solution, indicating that the neural network successfully captures the underlying functional relationship. Minor deviations are visually negligible, demonstrating strong learning capability even in the high-dimensional setting.

(c) Absolute error: The third subplot provides a heatmap of the absolute error between the analytical and predicted solutions. The error remains uniformly low across the domain, with slightly higher values near boundary regions. The predominantly dark (low-value) color distribution confirms that the approximation error is minimal, consistent with the reported relative error of approximately 0.15%.

Figure 14 clearly demonstrates that the PINN framework achieves high accuracy in approximating the solution of the fifth-order PDE. The close agreement between the true and predicted surfaces, along with the low error magnitude, validates the effectiveness and scalability of the proposed data-driven approach for solving high-dimensional differential equations.

8. Overview of the Results and Discussion

This study generalizes the classical Laplace transform to address quintuple (five-dimensional) and general n-dimensional PDEs. A formal definition of the n-th order Laplace transform and its operational properties for higher-order and mixed partial derivatives are developed, allowing complex multidimensional PDEs to be converted into algebraic forms in the transform domain. This transformation simplifies analytical solution procedures and enables reconstruction of the original functions. Theoretical results establish existence and uniqueness conditions, confirming that the transforms are well-defined under exponential growth assumptions. In addition, the generalized Bromwich inversion integral guarantees accurate and unique recovery of solutions in the original domain.

To illustrate the practical implementation of the method, several computational examples and visualizations were generated using MATLAB. One representative example considered a scaled Laplace slice F(s1, s2), which exhibited a Gaussian-like peak of approximately 5.8 near the point (1,7). Surface plots revealed symmetric patterns and resonance-type structures in the transform domain, highlighting how multidimensional variable interactions influence the transformed solution space. Additional tabulated results for selected bivariate functions and their partial derivatives further validated the consistency of the transformation and inversion processes.

The results show that the generalized Laplace transform framework is an effective analytical approach for simplifying and solving high-dimensional PDEs. Unlike traditional numerical methods such as the finite difference method and finite element method, the transform approach provides clearer insight into the structural behavior of solutions in multidimensional systems. However, computational difficulty increases as the dimension n exceeds five, particularly during the numerical inversion stage. Overall, higher-order Laplace transforms form a strong analytical basis for studying complex systems, and future work will aim to improve inversion techniques, investigate fractional extensions, and integrate machine learning to broaden practical applications.

9. Recent Advances in Numerical Laplace Transform Inversion

While the provided study focuses on analytical and symbolic aspects of higher-order Laplace transforms for PDEs, with numerical inversion mentioned as a future direction, recent research has advanced numerical methods for inverting Laplace transforms, often integrating stability improvements, fractional derivatives, and even machine learning for parameter optimization. Below is a summary of key works from 2024–2026, emphasizing practical applications in PDEs and related fields:

  1. Application of inverse Laplace transform techniques to the generalized Bagley–Torvik Equation: This study evaluates three numerical inversion methods (Fourier series, Gauss–Hermite, and another variant) for solving fractional PDEs like the Bagley–Torvik equation, which models viscoelastic phenomena. It demonstrates improved accuracy for equations with Caputo fractional derivatives, relevant to multidimensional diffusion problems similar to those in study [26].
  2. Modified inversion of the Laplace transform for nonlinear circuit simulation: Introduces a stable numerical inversion scheme (NILT) for time-domain simulation of nonlinear circuits, converting frequency-domain models to time-domain without instability. This could extend to higher-dimensional PDEs in engineering, offering faster computations than traditional methods.
  3. Optimal parameter selection in the Weeks' method using machine learning: Building on the classic Weeks' method (Laguerre expansions for inversion), recent adaptations use convolutional neural networks to optimize parameters for matrix exponentials, which appear in PDE discretizations. This hybrid machine learning-numerical approach reduces errors in high-dimensional inversions, aligning with the study's MATLAB visualizations [27].
  4. Numerical inverse Laplace beyond the Abate–Whitt framework (Extensions in 2024): Expands traditional frameworks by optimizing accuracy using transform function properties, enabling inversions for complex PDEs without standard limitations. Applications include real-time systems, potentially useful for the study's quintuple transforms [28].

These advances emphasize efficiency and stability, which could complement the study's theoretical framework by enabling practical inversion of higher-order transforms in MATLAB or similar environments.

10. Conclusion

This study extends the Laplace transform methodology to quintuple and general n-dimensional forms, providing a comprehensive theoretical foundation for their use in solving higher-order PDEs. Through detailed derivations of transform definitions, partial derivative properties, and theorems on existence and uniqueness under exponential growth conditions, we have established a unified framework that simplifies complex multidimensional PDEs into algebraic equations. The applicability is illustrated via representative examples, with MATLAB-based numerical computations and visualizations such as lower-dimensional slices, surface plots, and tables offering clear insights into solution behaviors, including resonant patterns and symmetry in the transform domain.

The results affirm the transforms' efficacy in handling systems with multiple variables, such as multi-phase diffusion and wave propagation, surpassing the limitations of lower-order methods. While computational challenges arise for very high dimensions, the framework's scalability and practical visualizations enhance its utility for analytical and numerical PDE solutions in science and engineering. Future extensions could explore fractional variants or integrations with computational tools to address nonlinear and stochastic problems, further advancing multidimensional mathematical modeling.

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