<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.3 20210610//EN" "https://jats.nlm.nih.gov/publishing/1.3/JATS-journalpublishing1-3.dtd"><article xml:lang="en" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:ali="http://www.niso.org/schemas/ali/1.0/" dtd-version="1.3" article-type="research-article"><front><journal-meta><journal-id journal-id-type="issn">2460-0245</journal-id><journal-title-group><journal-title>Journal of the Indonesian Mathematical Society</journal-title><abbrev-journal-title>JIMS</abbrev-journal-title></journal-title-group><issn pub-type="epub">2460-0245</issn><issn pub-type="ppub">2086-8952</issn><publisher><publisher-name>IndoMS</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.22342/jims.v32i2.2246</article-id><article-categories></article-categories><title-group><article-title>Smoothed Particle Hydrodynamics for Heat Transfer in Plates: Analytical Validation and Geometric Effects of Internal Heat Sources</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>Kurniawan</surname><given-names>Riski</given-names></name><address><country country="ID">Indonesia</country><email>riski.kurniawan@brin.go.id</email></address><xref ref-type="aff" rid="AFF-1"></xref><xref ref-type="corresp" rid="cor-0"></xref></contrib></contrib-group><contrib-group><contrib contrib-type="editor"><name><surname>Wijayanti</surname><given-names>Indah Emilia</given-names></name><address><country country="ID">Indonesia</country><email>ind_wijayanti@ugm.ac.id</email></address><xref ref-type="aff" rid="EDITOR-AFF-1"></xref></contrib></contrib-group><aff id="AFF-1"><institution-wrap><institution>Research Center for Computing, National Research and Innovation Agency (BRIN)</institution><institution-id institution-id-type="ror">https://ror.org/04xtpdj18</institution-id></institution-wrap><country country="ID">Indonesia</country></aff><aff id="EDITOR-AFF-1"><institution-wrap><institution>Universitas Gadjah Mada</institution><institution-id institution-id-type="ror">https://ror.org/03ke6d638</institution-id></institution-wrap><country country="ID">Indonesia</country></aff><author-notes><corresp id="cor-0">Corresponding author: Riski Kurniawan. Email: <email>riski.kurniawan@brin.go.id</email></corresp></author-notes><pub-date date-type="pub" iso-8601-date="2026-04-23" publication-format="electronic"><day>23</day><month>04</month><year>2026</year></pub-date><pub-date date-type="collection" iso-8601-date="2026-04-23" publication-format="electronic"><day>23</day><month>04</month><year>2026</year></pub-date><volume>32</volume><issue>2</issue><issue-title>JUNE</issue-title><fpage>1</fpage><lpage>19</lpage><history><date date-type="received" iso-8601-date="2025-09-23"><day>23</day><month>09</month><year>2025</year></date><date date-type="accepted" iso-8601-date="2026-01-25"><day>25</day><month>01</month><year>2026</year></date></history><permissions><copyright-statement>Copyright (c) 2026 Journal of the Indonesian Mathematical Society</copyright-statement><copyright-year>2026</copyright-year><copyright-holder>Journal of the Indonesian Mathematical Society</copyright-holder><license license-type="open-access" xlink:href="https://creativecommons.org/licenses/by-nc-nd/4.0/"><ali:license_ref xmlns:ali="http://www.niso.org/schemas/ali/1.0/">https://creativecommons.org/licenses/by-nc-nd/4.0/</ali:license_ref><license-p>This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.</license-p></license></permissions><self-uri xlink:href="https://jims-a.org/index.php/jimsa/article/view/2246" xlink:title="2246"></self-uri><abstract><p>Accurate simulation of heat transfer is essential in many engineering applications. This study investigates heat transfer on thin plates by solving twodimensional heat equations using the Smoothed Particle Hydrodynamics (SPH) method. The accuracy of the formulation is evaluated by comparing SPH results with analytical solutions for Dirichlet and Neumann boundary conditions, where small nRMSE values confirm good agreement. The method is then applied to plates with internal heat sources of different but equal-area geometries, showing that the star-shaped source yields the fastest heat transfer. These findings highlight the flexibility of SPH for modeling heat equations under complex geometries and boundary conditions.</p></abstract><kwd-group><kwd>Heat transfer</kwd><kwd>smoothed particle hydrodynamics</kwd><kwd>Dirichlet boundary conditions</kwd><kwd>Neumann boundary conditions</kwd><kwd>internal heat source</kwd></kwd-group><custom-meta-group><custom-meta><meta-name>File created by JATS Editor</meta-name><meta-value>https://jatseditor.com</meta-value></custom-meta><custom-meta><meta-name>issue-created-year</meta-name><meta-value>2026</meta-value></custom-meta></custom-meta-group></article-meta></front><body><sec id="sec-1"><title>1. Introduction</title><p>Heat transfer is a fundamental physical process that plays a critical role in a wide range of engineering applications, from manufacturing and materials processing to energy systems and modern thermal technologies. These include heating plate panels, melting and freezing, metal casting, and thermal spraying [<xref ref-type="bibr" rid="BIBR-1">1</xref>, <xref ref-type="bibr" rid="BIBR-2">2</xref>, <xref ref-type="bibr" rid="BIBR-3">3</xref>, <xref ref-type="bibr" rid="BIBR-4">4</xref>, <xref ref-type="bibr" rid="BIBR-5">5</xref>]. Understanding the mechanisms of heat transfer is essential to improve energy eficiency, predict the thermal response of a system, and design devices that rely on temperature control.</p><p>Various experimental studies have been conducted to observe the conduction patterns and temperature distribution in solid materials [<xref ref-type="bibr" rid="BIBR-6">6</xref>, <xref ref-type="bibr" rid="BIBR-7">7</xref>, <xref ref-type="bibr" rid="BIBR-8">8</xref>]. However, experimental approaches are generally expensive and time-consuming. Therefore, mathematical models have become important alternatives for systematically studying heat transfer phenomena. In this study, the heat transfer process is modeled using the heat equation, which represents the most fundamental form of difusion <xref ref-type="bibr" rid="BIBR-9">[9]</xref>. Conceptually, the heat equation belongs to the family of difusion-type partial diferential equations (PDEs), including the Extended Fisher–Kolmogorov equation (EFK) [<xref ref-type="bibr" rid="BIBR-10">10</xref>, <xref ref-type="bibr" rid="BIBR-11">11</xref>] and the Kuramoto–Sivashinsky equation (KS) [<xref ref-type="bibr" rid="BIBR-12">12</xref>, <xref ref-type="bibr" rid="BIBR-13">13</xref>], which are fourth-order equations.</p><p>The analytical solution of the heat equation depends heavily on the boundary conditions and becomes intractable when the geometry or boundaries are sufficiently complex. In such cases, numerical approaches provide a more practical framework for modeling realistic heat transfer scenarios [<xref ref-type="bibr" rid="BIBR-14">14</xref>, <xref ref-type="bibr" rid="BIBR-15">15</xref>]. Classical gridbased schemes, such as the Finite Diference Method (FDM) <xref ref-type="bibr" rid="BIBR-16">[16]</xref>, the Finite Volume Method (FVM) <xref ref-type="bibr" rid="BIBR-17">[17]</xref>, and the Finite Element Method (FEM) <xref ref-type="bibr" rid="BIBR-18">[18]</xref>, remain widely used for their robustness in structured domains. Various advanced discretization techniques have also been developed, including the One-Step One-Hybrid Block Method for nonlinear oscillatory PDEs <xref ref-type="bibr" rid="BIBR-19">[19]</xref>, Hermite spline methods for the KS equation <xref ref-type="bibr" rid="BIBR-20">[20]</xref>, and hybrid quintic Hermite spline collocation for the EFK equation <xref ref-type="bibr" rid="BIBR-21">[21]</xref>. Despite their strengths, grid-based methods can become restrictive when dealing with highly irregular boundaries, large deformations, or free-surface problems, motivating the use of more flexible mesh-free particle approaches such as Smoothed Particle Hydrodynamics (SPH).</p><p>SPH was first introduced by Lucy <xref ref-type="bibr" rid="BIBR-22">[22]</xref> and later developed independently by Gingold and Monaghan <xref ref-type="bibr" rid="BIBR-23">[23]</xref> for astrophysical simulations. Since then, it has been widely used to simulate solid mechanics and fluid dynamics [<xref ref-type="bibr" rid="BIBR-24">24</xref>, <xref ref-type="bibr" rid="BIBR-25">25</xref>, <xref ref-type="bibr" rid="BIBR-26">26</xref>]. Unlike grid-based schemes that require a predefined mesh, the SPH represents the domain as a set of interacting particles that carry quantities such as mass, position, velocity, and temperature. This mesh-free nature allows SPH to naturally handle large deformations, moving boundaries, and highly irregular geometries. The governing PDEs are reformulated as ordinary diferential equations using integral approximations based on kernels, which form the core of the SPH methodology <xref ref-type="bibr" rid="BIBR-27">[27]</xref>.</p><p>The use of SPH for heat transfer problems began with the pioneering work of Cleary and Monaghan <xref ref-type="bibr" rid="BIBR-28">[28]</xref>, who demonstrated its ability to solve heat conduction equations. Since then, SPH has been extensively applied to a broad range of thermal processes, including conduction, convection, and radiation in complex geometries [<xref ref-type="bibr" rid="BIBR-29">29</xref>, <xref ref-type="bibr" rid="BIBR-30">30</xref>, <xref ref-type="bibr" rid="BIBR-31">31</xref>, <xref ref-type="bibr" rid="BIBR-32">32</xref>, <xref ref-type="bibr" rid="BIBR-33">33</xref>, <xref ref-type="bibr" rid="BIBR-34">34</xref>, <xref ref-type="bibr" rid="BIBR-35">35</xref>]. Recent developments have further expanded its applicability to enhanced heat transfer in nanofluids <xref ref-type="bibr" rid="BIBR-36">[36]</xref> and chemically reactive systems where thermal difusion is coupled with reaction kinetics [<xref ref-type="bibr" rid="BIBR-37">37</xref>, <xref ref-type="bibr" rid="BIBR-38">38</xref>]. Recent advances in manufacturing further emphasize the importance of modeling internal heat sources, as demonstrated by Lin et al. <xref ref-type="bibr" rid="BIBR-39">[39]</xref>), who applied a ray-tracing SPH model to represent laser-induced heating. In most classical heat transfer studies, the heat source is imposed directly within the heat equation [<xref ref-type="bibr" rid="BIBR-40">40</xref>, <xref ref-type="bibr" rid="BIBR-41">41</xref>].</p><p>Although SPH has been applied in various heat transfer studies, several research gaps remain. The comprehensive validation of SPH against two-dimensional analytical solutions, especially for Dirichlet and Neumann boundary conditions, is still limited. In addition, the efect of the geometry of the internal heat source on the heat transfer rate in isolated plates, which is analytically challenging, has not been widely examined using SPH. To address these gaps, this study provides a systematic validation of the SPH against two-dimensional analytical solutions under Dirichlet and Neumann boundary conditions. Furthermore, we applied SPH to simulate heat transfer in plates containing internal heat sources of diferent geometries but equal area, allowing the assessment of how geometric variations influence heat transfer rates. The standard heat equation without a source term is employed, with the internal heat source imposed through Dirichlet conditions within the source region.</p><p>The remainder of this paper is organized as follows. Section <xref ref-type="sec" rid="6698100e-d6b8-2606-adcd-042fd6c2dff6">2</xref> presents the mathematical formulation of the two-dimensional heat equation. Section <xref ref-type="sec" rid="75536165-127b-3a4d-8751-5046d4232b7a">3</xref> describes the SPH numerical scheme used to approximate the solution. Section <xref ref-type="sec" rid="0973a5c5-153f-b66e-a302-ada80dd0c397">4</xref> provides model validation by comparing the SPH results with analytical solutions. Section <xref ref-type="sec" rid="c76bcd9d-ec14-a13c-349d-4535b93611a7">5</xref> investigates the influence of the geometry of the internal heat source on the heat transfer rate. Finally, Section <xref ref-type="sec" rid="824f84da-740f-1dc4-ebbb-99a79cd9170c">6</xref> summarizes the main findings of this study.</p></sec><sec id="sec-2"><title>2. Mathematical Model and Analytical Solutions</title><p>This section discusses the governing equations for heat transfer in a plate. Consider a thin plate <inline-formula><tex-math id="math-1"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Omega \subset \mathbb { R } ^ { 2 } \end{document} ]]></tex-math></inline-formula> made of heat-conducting material. Let <inline-formula><tex-math id="math-2"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u ( x , y , t ) \end{document} ]]></tex-math></inline-formula> be the temperature of the plate at point <inline-formula><tex-math id="math-3"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle ( x , y ) \in \Omega \end{document} ]]></tex-math></inline-formula> and time <inline-formula><tex-math id="math-4"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t \end{document} ]]></tex-math></inline-formula>. This study is restricted to a rectangular plate <inline-formula><tex-math id="math-5"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Omega = [ 0 , a ] \times [ 0 , b ] \end{document} ]]></tex-math></inline-formula>, where <inline-formula><tex-math id="math-6"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle a , b \in \mathbb { R } \end{document} ]]></tex-math></inline-formula>.</p><p>Under the ideal assumption of uniform density and no external heat sources, u satisfies the two-dimensional heat equation:</p><disp-formula id="equation-1"><tex-math id="math-7"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \frac {\partial u}{\partial t} = \alpha \nabla^ {2} u = \alpha \left(\frac {\partial^ {2} u}{\partial x ^ {2}} + \frac {\partial^ {2} u}{\partial y ^ {2}}\right),\tag{1} \end{document} ]]></tex-math></disp-formula><p>for <inline-formula><tex-math id="math-8"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \ 0 < x < a , 0 < y < b \end{document} ]]></tex-math></inline-formula>. Thermal difusivity α is defined as</p><disp-formula id="equation-2"><tex-math id="math-9"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \alpha = \frac {\kappa}{\rho C _ {p}},\tag{2} \end{document} ]]></tex-math></disp-formula><p>where <inline-formula><tex-math id="math-10"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \kappa \end{document} ]]></tex-math></inline-formula> is the thermal conductivity, <inline-formula><tex-math id="math-11"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle C _ { p } \end{document} ]]></tex-math></inline-formula> is the heat capacity, and <inline-formula><tex-math id="math-12"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \rho \end{document} ]]></tex-math></inline-formula> is the density of the material. In this study, the physical domain consists of a 10 cm × 10 cm carbon steel plate characterized by the material properties <inline-formula><tex-math id="math-13"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \rho = 7 8 5 4 ~ \mathrm { k g / m ^ { 3 } } , \kappa = 6 0 . 5 \end{document} ]]></tex-math></inline-formula><inline-formula><tex-math id="math-14"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathrm { W / ( m K ) } \end{document} ]]></tex-math></inline-formula>, and <inline-formula><tex-math id="math-15"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle C _ { p } = 4 3 4 ~ \mathrm { J / ( k g K ) } \end{document} ]]></tex-math></inline-formula>. In steady state, equation (1) reduces to Laplace’s equation.</p><p>The analytical solution of the two-dimensional heat equation (1) with generalized Dirichlet boundary conditions has been discussed by Hsu et al. <xref ref-type="bibr" rid="BIBR-42">[42]</xref>. As for Neumann boundary conditions, to the best of our knowledge, the analytical solutions have not been discussed in the literature. However, Subani et al. <xref ref-type="bibr" rid="BIBR-43">[43]</xref> have addressed this for the one-dimensional case, where the heat equation (1) in one-dimensional form with homogeneous Neumann boundary conditions is solved in two stages: variable separation and the superposition principle.</p><p>In the following, we present the analytical solution of the two-dimensional heat equation (1) with homogeneous Neumann boundary conditions. The plate temperature at the beginning of the observation is given as the initial condition:</p><disp-formula id="equation-3"><tex-math id="math-16"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, 0) = f (x, y), \quad (x, y) \in \Omega .\tag{3} \end{document} ]]></tex-math></disp-formula><p>Furthermore, the homogeneous Neumann boundary conditions are as follows:</p><disp-formula id="equation-4"><tex-math id="math-17"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array}{l l} u _ {x} (0, y, t) = u _ {x} (a, y, t) = 0, & 0 \leq y \leq b, t > 0, \\ u _ {y} (x, 0, t) = u _ {y} (x, b, t) = 0, & 0 \leq x \leq a, t > 0. \end{array}\tag{4} \end{document} ]]></tex-math></disp-formula><p>Physically, this means isolating the four sides of the plate so that no heat enters or leaves the plate through these sides.</p><p>Using a procedure similar to <xref ref-type="bibr" rid="BIBR-43">[43]</xref>, we obtain an analytical solution of the heat equation (1) with the initial conditions (3) and the boundary conditions (4) as follows:</p><disp-formula id="equation-5"><tex-math id="math-18"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{equation*}\begin{aligned}u(x,y,t)&=A_{00}+\sum_{m=1}^{\infty}A_{m0}\cos\left(\frac{m\pi}{a}x\right)e^{-\alpha\pi^2\left(\frac{m}{a}\right)^2t}\\&\quad+\sum_{n=1}^{\infty}A_{0n}\cos\left(\frac{n\pi}{b}y\right)e^{-\alpha\pi^2\left(\frac{n}{b}\right)^2t}\\&\quad+\sum_{m=1}^{\infty}\sum_{n=1}^{\infty}A_{mn}\cos\left(\frac{m\pi}{a}x\right)\cos\left(\frac{n\pi}{b}y\right)e^{-\alpha\pi^2\left(\left(\frac{m}{a}\right)^2+\left(\frac{n}{b}\right)^2\right)t}.\end{aligned}\tag{5}\end{equation*} \end{document} ]]></tex-math></disp-formula><p>where</p><p><inline-formula><tex-math id="math-19"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{align*}A_{00} &= \int_{0}^{a} \int_{0}^{b} f(x, y) \, dy \, dx, & A_{m0} &= \int_{0}^{a} \int_{0}^{b} f(x, y) \cos \left(\frac{m\pi}{a} x\right) dy \, dx, \\A_{0n} &= \int_{0}^{a} \int_{0}^{b} f(x, y) \cos \left(\frac{n\pi}{b} y\right) dy \, dx, & A_{mn} &= \int_{0}^{a} \int_{0}^{b} f(x, y) \cos \left(\frac{m\pi}{a} x\right) \cos \left(\frac{n\pi}{b} y\right) dy \, dx.\end{align*} \end{document} ]]></tex-math></inline-formula></p><p>The detailed derivation of this analytical solution is provided in the Appendix.</p></sec><sec id="sec-3"><title>3. Numerical Method</title><p>In this section, we describe the SPH formulation used to approximate the twodimensional heat equation (1). The domain <inline-formula><tex-math id="math-20"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle Ω \end{document} ]]></tex-math></inline-formula> is discretized into a number of <inline-formula><tex-math id="math-21"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle N \end{document} ]]></tex-math></inline-formula> particles with the initial positions of the <inline-formula><tex-math id="math-22"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula>-particles being <inline-formula><tex-math id="math-23"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathbf { x } _ { i } = ( x _ { i } , y _ { i } ) , i = 1 , 2 , \ldots , N \end{document} ]]></tex-math></inline-formula>. Two types of initial particle arrangement are commonly used: structured and unstructured, as illustrated in <xref ref-type="fig" rid="figure-1">Figure 1</xref>. A structured layout produces higher operator accuracy <xref ref-type="bibr" rid="BIBR-44">[44]</xref>, but is less flexible to capture intricate geometries. In contrast, an unstructured distribution allows particles to reach narrow features of the domain, although the resulting particle disorder may introduce extra numerical noise <xref ref-type="bibr" rid="BIBR-45">[45]</xref>.</p><p>The function <inline-formula><tex-math id="math-24"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u \end{document} ]]></tex-math></inline-formula> at <inline-formula><tex-math id="math-25"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathbf { x } _ { i } \end{document} ]]></tex-math></inline-formula> and time <inline-formula><tex-math id="math-26"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t \end{document} ]]></tex-math></inline-formula> can be approximated by volume integration using the kernel function (also called the weight function) <inline-formula><tex-math id="math-27"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle W \end{document} ]]></tex-math></inline-formula>, as follows</p><disp-formula id="equation-6"><tex-math id="math-28"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (\mathbf {x} _ {i}, t) \approx [ u (\mathbf {x} _ {i}, t) ] \equiv \int_ {\Omega} u (\mathbf {x} _ {j}, t) W (r _ {i j}, h) d \mathbf {x} _ {j},\tag{6} \end{document} ]]></tex-math></disp-formula><p>for <inline-formula><tex-math id="math-29"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j = 1 , 2 , \dots , N \end{document} ]]></tex-math></inline-formula>, where <inline-formula><tex-math id="math-30"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle r _ { i j } \end{document} ]]></tex-math></inline-formula> is the distance between the particles <inline-formula><tex-math id="math-31"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-32"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j \end{document} ]]></tex-math></inline-formula>, and <inline-formula><tex-math id="math-33"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle h \end{document} ]]></tex-math></inline-formula> are the smoothing lengths. Consistent with typical SPH settings [<xref ref-type="bibr" rid="BIBR-24">24</xref>, <xref ref-type="bibr" rid="BIBR-27">27</xref>, <xref ref-type="bibr" rid="BIBR-45">45</xref>], we define the smoothing length as <inline-formula><tex-math id="math-34"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle h = 1 . 2 \Delta p \end{document} ]]></tex-math></inline-formula>, where <inline-formula><tex-math id="math-35"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle ∆p \end{document} ]]></tex-math></inline-formula> is the initial spacing of the particles.</p><fig id="figure-1"><label>Figure 1.</label><caption><p>Particle arrangements used in SPH: (left) structured distribution, (right) unstructured distribution.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13801" mime-subtype="png" mimetype="image"><alt-text>Figure 1.</alt-text></graphic></fig><p>Neighborhood particles are a crucial component in particle kernel approximation. Define the vector <inline-formula><tex-math id="math-36"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathbf { r _ { i j } } \end{document} ]]></tex-math></inline-formula> as the distance vector between particles <inline-formula><tex-math id="math-37"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-38"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j \end{document} ]]></tex-math></inline-formula>,</p><disp-formula id="equation-7"><tex-math id="math-39"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathbf {r} _ {\mathbf {i j}} = \binom{x _ {i} - x _ {j}}{y _ {i} - y _ {j}}. \end{document} ]]></tex-math></disp-formula><p>The distance between the target particle <inline-formula><tex-math id="math-40"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula> and the neighboring particle <inline-formula><tex-math id="math-41"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j \end{document} ]]></tex-math></inline-formula> is defined using the Euclidean norm</p><disp-formula id="equation-8"><tex-math id="math-42"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle r _ {i j} = \| \mathbf {r _ {i j}} \| _ {2} = \sqrt {(x _ {i} - x _ {j}) ^ {2} + (y _ {i} - y _ {j}) ^ {2}}. \end{document} ]]></tex-math></disp-formula><p>In this study, we use a multiplier <inline-formula><tex-math id="math-43"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle k = 2 \end{document} ]]></tex-math></inline-formula> on the smoothing length. If <inline-formula><tex-math id="math-44"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle r _ { i j } \leq 2 h \end{document} ]]></tex-math></inline-formula>, then the particle <inline-formula><tex-math id="math-45"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j \end{document} ]]></tex-math></inline-formula> is considered a neighbor of the particle <inline-formula><tex-math id="math-46"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula>. For example, <xref ref-type="fig" rid="figure-2">Figure 2</xref> (left) illustrates the definition of neighboring particles, where particle <inline-formula><tex-math id="math-47"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula> has 20 neighboring particles.</p><p>Furthermore, several smoothing kernels are commonly used, including cubic spline (B-spline), Gaussian, Supergaussian, Quadratic, and Quintic kernels. The kernel function used in this study is the cubic spline, which is given as</p><disp-formula id="equation-9"><tex-math id="math-48"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle W (s) = \sigma \left\{ \begin{array}{l l} 1 - \frac {3}{2} s ^ {2} + \frac {3}{4} s ^ {3}, & 0 \leq s \leq 1 \\ \frac {1}{4} (2 - s) ^ {3}, & 1 < s \leq 2 \end{array} \right.,\tag{7} \end{document} ]]></tex-math></disp-formula><p>where <inline-formula><tex-math id="math-49"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array} { r } { s \ = \ \frac { r _ { i j } } { h } } \end{array} \end{document} ]]></tex-math></inline-formula>. The constant <inline-formula><tex-math id="math-50"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle σ \end{document} ]]></tex-math></inline-formula> varies for each dimension to satisfy the kernel normalization requirements. For a two-dimensional system, <inline-formula><tex-math id="math-51"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array} { r } { \sigma = \frac { 1 0 } { 7 \pi h ^ { 2 } } } \end{array} \end{document} ]]></tex-math></inline-formula>. Note that the kernel <xref ref-type="disp-formula" rid="equation-1">(7)</xref> is a smooth polynomial function, which allows it to be diferentiated at all <inline-formula><tex-math id="math-52"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle s \end{document} ]]></tex-math></inline-formula>. The cubic spline kernel function and its derivatives are plotted in <xref ref-type="fig" rid="figure-2">Figure 2</xref> (right). It is also important to note that the values of the kernel function and its derivatives are zero for <inline-formula><tex-math id="math-53"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle s > 2 \end{document} ]]></tex-math></inline-formula>, meaning that particles located more than <inline-formula><tex-math id="math-54"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 2h \end{document} ]]></tex-math></inline-formula> away from the target particle do not contribute to the approximation.</p><fig id="figure-2"><label>Figure 2.</label><caption><p>(Left) Particle Neighborhood. (Right) Kernel function.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13802" mime-subtype="png" mimetype="image"><alt-text>Figure 2.</alt-text></graphic></fig><p>Since the domain is modeled as discrete particles, the continuous integral (6) needs to be converted to a discrete sum over all particles in the domain. Let <inline-formula><tex-math id="math-55"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathbb { S } _ { i } \end{document} ]]></tex-math></inline-formula> be the set of neighboring particles <inline-formula><tex-math id="math-56"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j \end{document} ]]></tex-math></inline-formula> surrounding the target particle <inline-formula><tex-math id="math-57"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula>, which is discretized as</p><disp-formula id="equation-10"><tex-math id="math-58"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathbb {S} _ {i} \equiv \{j = 1, 2,..., N | j \neq i \}.\tag{8} \end{document} ]]></tex-math></disp-formula><p>The approximation (6) can be expressed in its discrete particle form as follows:</p><disp-formula id="equation-11"><tex-math id="math-59"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (\mathbf {x} _ {i}, t) \approx \langle \phi (\mathbf {x} _ {i}, t) \rangle \equiv \sum_ {j \in \mathbb {S} _ {i}} \frac {m _ {j}}{\rho_ {j}} u (\mathbf {x} _ {j}, t) W (r _ {i j}, h),\tag{9} \end{document} ]]></tex-math></disp-formula><p>where <inline-formula><tex-math id="math-60"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle m _ { j } \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-61"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \rho _ { j } \end{document} ]]></tex-math></inline-formula> are the mass and density of the particle <inline-formula><tex-math id="math-62"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle j \end{document} ]]></tex-math></inline-formula>, respectively.</p><p>The kernel function derivative is used for the Laplace approximation. The kernel gradient vector is given as</p><disp-formula id="equation-12"><tex-math id="math-63"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \nabla W (r _ {i j}, h) = \binom{d W _ {x}}{d W _ {y}},\tag{10} \end{document} ]]></tex-math></disp-formula><p>where</p><disp-formula id="equation-13"><tex-math id="math-64"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle d W _ {x} = \frac {x _ {i j} (\partial W / \partial s)}{r _ {i j} h}, \quad d W _ {y} = \frac {y _ {i j} (\partial W / \partial s)}{r _ {i j} h}. \end{document} ]]></tex-math></disp-formula><p>Finally, the gradient and Laplace approximations of the SPH method are given as follows:</p><disp-formula id="equation-14"><tex-math id="math-65"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \nabla u (\mathbf {x} _ {i}, t) \approx \langle \nabla u _ {i} \rangle = \sum_ {j \in \mathbb {S} _ {i}} \frac {m _ {j}}{\rho_ {j}} (u _ {j} - u _ {i}) \nabla W _ {i j},\tag{11} \end{document} ]]></tex-math></disp-formula><disp-formula id="equation-15"><tex-math id="math-66"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \nabla^ {2} u (\mathbf {x} _ {i}, t) \approx \left\langle \nabla^ {2} u _ {i} \right\rangle = 2 \sum_ {j \in \mathbb {S} _ {i}} \frac {m _ {j}}{\rho_ {j}} \frac {u _ {j} - u _ {i}}{r _ {i j} ^ {2}} \left(\mathbf {r} _ {i j} \cdot \nabla W _ {i j}\right).\tag{12} \end{document} ]]></tex-math></disp-formula><p>After approximating the Laplace form using the SPH method, we proceed with the time integration of the heat equation (1). To ensure a stable solution, the time step <inline-formula><tex-math id="math-67"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle ∆t \end{document} ]]></tex-math></inline-formula> must satisfy the Courant-Friedrichs-Lewy (CFL) condition. This condition ensures that the numerical domain of dependence contains the physical domain of dependence, which means that the numerical propagation speed must not be smaller than the physical propagation speed [<xref ref-type="bibr" rid="BIBR-46">46</xref>, <xref ref-type="bibr" rid="BIBR-47">47</xref>]. In the case of twodimensional heat difusion, the time step <inline-formula><tex-math id="math-68"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta t \end{document} ]]></tex-math></inline-formula> is formulated as</p><disp-formula id="equation-16"><tex-math id="math-69"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta t \leq \frac {h ^ {2}}{4 \alpha},\tag{13} \end{document} ]]></tex-math></disp-formula><p>The temperature of the particle <inline-formula><tex-math id="math-70"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle i \end{document} ]]></tex-math></inline-formula> at time <inline-formula><tex-math id="math-71"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t ^ { n + 1 } \end{document} ]]></tex-math></inline-formula> is then computed using the forward Euler method, given by</p><disp-formula id="equation-17"><tex-math id="math-72"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{equation}u_i^{n+1} = u_i^n + \Delta t \nabla^2 u_i^n . \tag{14}\end{equation} \end{document} ]]></tex-math></disp-formula><p>To handle the boundary value problem, SPH utilizes the concept of ghost particles, which are additional particles located outside the domain or around the <inline-formula><tex-math id="math-73"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle ∂Ω \end{document} ]]></tex-math></inline-formula> boundary; refer back to <xref ref-type="fig" rid="figure-1">Figure 1</xref>. These particles are not included in the SPH computation, but are arranged to approximate the prescribed boundary conditions. Dirichlet boundary conditions are enforced by setting the temperature of the ghost particles equal to the specified boundary values, as described in <xref ref-type="bibr" rid="BIBR-32">[32]</xref>. Implementing homogeneous Neumann boundary conditions poses additional challenges, such as assigning the temperatures of ghost particles so that the normal temperature gradient vanishes, which requires arranging the particles near the boundary in a structured manner so that the ghost particle temperature can be mirrored from the interior particle across the boundary.</p><p>In summary, the steps for using the SPH method to simulate heat transfer are outlined in <xref ref-type="fig" rid="figure-3">Algorithm 1</xref>.</p><fig id="figure-3"><label>Algorithm 1</label><caption><p>SPH method for solving heat equations (1)</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13803" mime-subtype="png" mimetype="image"><alt-text>Algorithm 1</alt-text></graphic></fig><p>All simulations were performed on a computer equipped with an AMD Ryzen 9 PRO 5945 processor (12 cores, 24 CPUs, 3.0 GHz), 128 GB RAM, and a Windows 11 operating system. Numerical calculations were performed using MATLAB R2024b.</p></sec><sec id="sec-4"><title>4. Model Validation</title><p>In this section, the SPH results obtained using the numerical procedure described in <xref ref-type="fig" rid="figure-3">Algorithm 1</xref> are compared with the corresponding analytical solutions to assess the accuracy of the method. The computational domain is expressed as <inline-formula><tex-math id="math-74"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Omega=[0,1]\;\mathrm{dm}\times[0,1]\;\mathrm{dm} \end{document} ]]></tex-math></inline-formula>. The plate is discretized using a structured particle arrangement, where <inline-formula><tex-math id="math-75"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-76"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta y \end{document} ]]></tex-math></inline-formula> denote the initial particle spacing in the <inline-formula><tex-math id="math-77"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle x- \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-78"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle y- \end{document} ]]></tex-math></inline-formula> directions, respectively, and are taken to be equal in this study.</p><p>The agreement between the SPH and the analytical reference is quantified using the normalized root mean square error (nRMSE). This metric is chosen because it provides a scale-independent measure of accuracy, allowing the error to be interpreted relative to the thermal range of the system and enabling fair comparison between diferent test cases. The nRMSE is defined as</p><disp-formula id="equation-18"><tex-math id="math-79"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \mathrm{nRMSE} = \frac {\mathrm{RMSE}}{\hat {u} _ {\max} - \hat {u} _ {\min}}, \quad \mathrm{RMSE} = \sqrt {\frac {\sum_ {i = 1} ^ {N} (u _ {i} - \hat {u} _ {i}) ^ {2}}{N}},\tag{15} \end{document} ]]></tex-math></disp-formula><p>where <inline-formula><tex-math id="math-80"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \hat { u } _ { \mathrm { m a x } } \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-81"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \hat { u } _ { \mathrm { m i n } } \end{document} ]]></tex-math></inline-formula> denote the maximum and minimum values of the analytical solution in the domain, respectively.</p><sec id="sec-5"><title>4.1. Steady-state heat conduction.</title><p>In the first validation test, the steady-state heat conduction problem is examined. The boundary conditions follow those used in the reference study <xref ref-type="bibr" rid="BIBR-48">[48]</xref>, which are defined as</p><disp-formula id="equation-19"><tex-math id="math-82"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array}{l} u (x, 1, t) = \frac {4 0 0}{\pi} \sin (\pi x) ^ {\circ} \mathrm{C}, \\ u (x, 0, t) = u (0, y, t) = u (1, y, t) = 0 ^ {\circ} \mathrm{C}. \end{array}\tag{16} \end{document} ]]></tex-math></disp-formula><p>The analytical solution of Laplace’s equation associated with this configuration is given as follows</p><disp-formula id="equation-20"><tex-math id="math-83"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y) = \frac {4 0 0}{\pi \sinh \pi} \sinh (\pi y) \sin (\pi x) ^ {\circ} \mathrm{C}.\tag{17} \end{document} ]]></tex-math></disp-formula><p>The reference study <xref ref-type="bibr" rid="BIBR-48">[48]</xref> solves the Laplace equation numerically using FEM and FDM. In contrast, the present work employs the full transient heat equation and advances the solution over time until it converges to the steady state. The initial condition is specified as a uniform temperature distribution:</p><disp-formula id="equation-21"><tex-math id="math-84"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, 0) = 0 ^ {\circ} \mathrm{C}, \quad (x, y) \in \Omega .\tag{18} \end{document} ]]></tex-math></disp-formula><p>The SPH simulation is performed using several particle spacings, namely <inline-formula><tex-math id="math-85"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x = 0.1 dm \end{document} ]]></tex-math></inline-formula>, <inline-formula><tex-math id="math-86"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 0.02 dm \end{document} ]]></tex-math></inline-formula>, and <inline-formula><tex-math id="math-87"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 0.01 dm \end{document} ]]></tex-math></inline-formula>. For each resolution, the particles are uniformly distributed within the computational domain <inline-formula><tex-math id="math-88"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle [0,1] \times [0,1] \operatorname{dm} \end{document} ]]></tex-math></inline-formula>. Resulting in <inline-formula><tex-math id="math-89"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle N = 2601 \end{document} ]]></tex-math></inline-formula> particles for <inline-formula><tex-math id="math-90"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x = 0.02 \operatorname{dm} \end{document} ]]></tex-math></inline-formula>. The solution is advanced in time to <inline-formula><tex-math id="math-91"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 6 0 0 ~ \mathrm { s } \end{document} ]]></tex-math></inline-formula> using a time step of <inline-formula><tex-math id="math-92"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x = 0.02 ~ \mathrm { s } \end{document} ]]></tex-math></inline-formula>. During the computation, the boundary conditions <xref ref-type="disp-formula" rid="equation-3">(16)</xref> are imposed directly on the gost particles.</p><p>The evolution of the temperature distribution for the representative resolution <inline-formula><tex-math id="math-93"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x = 0 . 0 2 \end{document} ]]></tex-math></inline-formula> dm is illustrated in <xref ref-type="fig" rid="figure-4">Figure 3</xref>. The heat gradually difuses downward from the upper edge. By <inline-formula><tex-math id="math-94"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 6 0 0 ~ \mathrm { s } \end{document} ]]></tex-math></inline-formula>, the solution does not exhibit significant temporal changes, indicating that the steady state has been efectively reached.</p><fig id="figure-4"><label>Figure 3.</label><caption><p>Temperature distribution for steady-state heat conduction test at t = 0 s (left), t = 10 s (middle), and t = 600 s (right).</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13804" mime-subtype="png" mimetype="image"><alt-text>Figure 3.</alt-text></graphic></fig><p>To quantify the accuracy of the SPH method, we calculate the RMSE between the steady-state temperature and the analytical solution. The RMSE values for different particle spacings <inline-formula><tex-math id="math-95"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x \end{document} ]]></tex-math></inline-formula> are reported in <xref ref-type="table" rid="table-1">Table 1</xref>. The error decreases consistently with mesh refinement, indicating good numerical convergence. Compared with the reference numerical schemes, SPH achieves a higher precision than the FDM results of <xref ref-type="bibr" rid="BIBR-48">[48]</xref>, while the FEM solution in <xref ref-type="bibr" rid="BIBR-48">[48]</xref> remains the most accurate among the three methods. The table also lists the computational time required for each resolution, showing the expected increase in running time as the number of particles grows. Although accuracy improves at finer resolutions, the computational cost increases accordingly.</p><table-wrap id="table-1"><label>Table 1.</label><caption><p>RMSE values of numerical results for diferent spatial resolutions, along with the corresponding number of particles and computational time of SPH.</p></caption><table><colgroup><col></col><col></col><col></col><col></col><col></col><col></col></colgroup><thead><tr><th scope="col" rowspan="2"><inline-formula><tex-math id="math-96"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x \end{document} ]]></tex-math></inline-formula> (dm)</th><th scope="col" rowspan="2"><inline-formula><tex-math id="math-97"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle N \end{document} ]]></tex-math></inline-formula></th><th scope="col" rowspan="2">Comp. time <inline-formula><tex-math id="math-98"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle (s) \end{document} ]]></tex-math></inline-formula></th><th scope="col" colspan="3">RMSE</th></tr><tr><th scope="col">SPH</th><th scope="col">FEM <xref ref-type="bibr" rid="BIBR-48">[48]</xref></th><th scope="col">FDM <xref ref-type="bibr" rid="BIBR-48">[48]</xref></th></tr></thead><tbody><tr><td>0.10</td><td>121</td><td>14</td><td>0.403</td><td>0.367</td><td>1.749</td></tr><tr><td>0.02</td><td>2601</td><td>432</td><td>0.112</td><td>0.015</td><td>0.353</td></tr><tr><td>0.01</td><td>10201</td><td>1783</td><td>0.059</td><td>-</td><td>-</td></tr></tbody></table></table-wrap></sec><sec id="sec-6"><title>4.2. Nonhomogeneous Dirichlet boundary condition.</title><p>For this case, consider a plate with an initial temperature distribution given by</p><disp-formula id="equation-22"><tex-math id="math-99"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, 0) = \sin (\pi x) + \sin (\pi y).\tag{19} \end{document} ]]></tex-math></disp-formula><p>The four sides of the plate are subjected to sinusoidal boundary conditions that vary spatially and decay exponentially over time, given as</p><disp-formula id="equation-23"><tex-math id="math-100"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array}{r} u (0, y, t) = u (1, y, t) = \sin (\pi y) e ^ {- \pi^ {2} \alpha t}, \\ u (x, 0, t) = u (x, 1, t) = \sin (\pi x) e ^ {- \pi^ {2} \alpha t}. \end{array}\tag{20} \end{document} ]]></tex-math></disp-formula><p>In this simulation, a particle spacing of <inline-formula><tex-math id="math-101"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x = 0 . 0 2 \end{document} ]]></tex-math></inline-formula> dm is used, resulting in a total of <inline-formula><tex-math id="math-102"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle N = 2 6 0 1 \end{document} ]]></tex-math></inline-formula> particles. The simulation is performed up to <inline-formula><tex-math id="math-103"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 2 0 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula> with a time step of <inline-formula><tex-math id="math-104"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta t = 0 . 0 2 \mathrm { \ s } \end{document} ]]></tex-math></inline-formula>, and the total computational time is approximately <inline-formula><tex-math id="math-105"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 14 \mathrm { \ s } \end{document} ]]></tex-math></inline-formula>. The time evolution of the temperature field is shown in <xref ref-type="fig" rid="figure-5">Figure 4</xref>, where the initial sinusoidal pattern gradually decays under exponentially decreasing boundary forcing. As time increases, the temperature amplitude decreases, and the contours progressively flatten toward a more uniform radial distribution.</p><fig id="figure-5"><label>Figure 4.</label><caption><p>Temperature distribution for nonhomogeneous Dirichlet test at t = 0 s (left), t = 10 s (middle), and t = 20 s (right).</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13805" mime-subtype="png" mimetype="image"><alt-text>Figure 4.</alt-text></graphic></fig><p>The heat equation (1) with the initial condition (19) and the boundary condition (20), has been studied by Hsu et al. <xref ref-type="bibr" rid="BIBR-42">[42]</xref>. The analytical solution is given as</p><disp-formula id="equation-24"><tex-math id="math-106"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, t) = (\sin (\pi x) + \sin (\pi y)) e ^ {- \alpha \pi^ {2} t}.\tag{21} \end{document} ]]></tex-math></disp-formula><p>A comparison of the contours between the analytical and SPH solutions at <inline-formula><tex-math id="math-107"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 1 0 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula> is shown in <xref ref-type="fig" rid="figure-6">Figure 5</xref> (left). It can be observed that, near the center of the plate, the SPH results are slightly ahead of the analytical solution. However, the SPH contour fits perfectly with the analytical solution. During computation, the nRMSE is evaluated using equations (15), and the results are shown in <xref ref-type="fig" rid="figure-6">Figure 5</xref> (right). Although the nRMSE increases with the simulation time, it remains very small, staying below <inline-formula><tex-math id="math-108"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 6 \times 1 0 ^ { - 3 } \end{document} ]]></tex-math></inline-formula>. This shows that SPH performs excellently in approximating the analytical solution.</p><fig id="figure-6"><label>Figure 5.</label><caption><p>Error analysis for nonhomogeneous Dirichlet test. (Left) temperature contours at t = 10 s, (right) nRMSE of SPH over time.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13806" mime-subtype="png" mimetype="image"><alt-text>Figure 5.</alt-text></graphic></fig></sec><sec id="sec-7"><title>4.3. Homogeneous Neumann boundary condition.</title><p>The final test case aims to evaluate the performance of SPH in simulating heat transfer when the domain boundaries are isolated. In this case, all four sides of the plate are subjected to homogeneous Neumann boundary conditions, as specified in equations (4). The initial heat distribution of the plate is given by</p><disp-formula id="equation-25"><tex-math id="math-109"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, 0) = x - y.\tag{22} \end{document} ]]></tex-math></disp-formula><p>From equation (5), we derive the analytical solution of the heat equation (1) with the boundary conditions (4) and the initial conditions (22), given by the following expression:</p><disp-formula id="equation-26"><tex-math id="math-110"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, t) = \frac {2}{\pi^ {2}} \left[ \sum_ {m = 1} ^ {\infty} \frac {(- 1) ^ {m} - 1}{m ^ {2}} \cos (m \pi x) e ^ {- \alpha (m \pi) ^ {2} t} + \sum_ {n = 1} ^ {\infty} \frac {1 - (- 1) ^ {n}}{n ^ {2}} \cos (n \pi y) e ^ {- \alpha (n \pi) ^ {2} t} \right]\tag{23} \end{document} ]]></tex-math></disp-formula><p>The computational domain is discretized using a space of <inline-formula><tex-math id="math-111"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta x = 0 . 0 2 dm \end{document} ]]></tex-math></inline-formula>. To properly enforce the boundary conditions (4), the ghost particles are positioned just outside the domain. Consequently, the particles are arranged from <inline-formula><tex-math id="math-112"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle - \frac { \Delta x } { 2 } \end{document} ]]></tex-math></inline-formula> to <inline-formula><tex-math id="math-113"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array} { r } { 1 + \frac { \Delta x } { 2 } } \end{array} \end{document} ]]></tex-math></inline-formula> in both spatial directions, resulting in a total of <inline-formula><tex-math id="math-114"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle N = 2 7 0 4 \end{document} ]]></tex-math></inline-formula> particles. The simulation is carried out up to <inline-formula><tex-math id="math-115"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 2 0 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula> and requires approximately <inline-formula><tex-math id="math-116"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 2 0 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula> computational time.</p><p>The temporal evolution of the temperature field is shown in <xref ref-type="fig" rid="figure-7">Figure 6</xref>. Under homogeneous Neumann boundary conditions, the heat within the plate is gradually redistributed, whereas no flux crosses the boundaries. As difusion progresses, spatial temperature variations diminish and the solution approaches a uniform state corresponding to the average of the initial condition.</p><fig id="figure-7"><label>Figure 6.</label><caption><p>Temperature distribution for homogeneous Neumann test at t = 0 s (left), t = 10 s (middle), and t = 20 s (right).</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13807" mime-subtype="png" mimetype="image"><alt-text>Figure 6.</alt-text></graphic></fig><p>The SPH solution at <inline-formula><tex-math id="math-117"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 1 0 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula> is shown as a contour in <xref ref-type="fig" rid="figure-8">Figure 7</xref> (left), along with the analytical solution given by (23). It can be observed that the SPH solution contour closely matches the analytical solution contour. The nRMSE value during the simulation time is shown in <xref ref-type="fig" rid="figure-8">Figure 7</xref> (Right). From the beginning of the simulation, nRMSE decreases but increases after <inline-formula><tex-math id="math-118"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 1 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula>. However, the nRMSE value is still very small, that is, below <inline-formula><tex-math id="math-119"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 1 . 2 \times 1 0 ^ { - 3 } \end{document} ]]></tex-math></inline-formula>. This very small error shows that the SPH is very good at approaching the analytical solution.</p><fig id="figure-8"><label>Figure 7.</label><caption><p>Error analysis for homogeneous Neumann test. (Left) temperature contours at t = 10 s, (right) nRMSE of SPH over time.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13808" mime-subtype="png" mimetype="image"><alt-text>Figure 7.</alt-text></graphic></fig></sec></sec><sec id="sec-8"><title>5. Influence of Heat Source Geometry</title><p>Finally, SPH is used to simulate heat transfer in more complex cases. We investigate the efect of an internal heat source located in the center of the plate on the rate of heat spreading. Heat sources with various geometries, all having the same area, are considered. The objective is to analyze which geometric shapes distribute heat more rapidly than others. All four sides of the plate are insulated, which prevents heat from entering or exiting the edges. This case is quite complex to solve analytically, as it involves nonhomogeneous Dirichlet and homogeneous Neumann boundary conditions, and the geometric shape of the heat source is not simple. To the best of our knowledge, this issue has not been previously discussed in the literature.</p><p>We tested six heat source geometries: circular, triangular, square, hexagonal, star, and star of David. The radius of the circular heat source is 1 cm, and all heat sources have the same area. The dimensions of these heat sources are shown in <xref ref-type="fig" rid="figure-9">Figure 8</xref>. Initially, the plate has a uniform temperature of <inline-formula><tex-math id="math-120"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 300^\circ K \end{document} ]]></tex-math></inline-formula>. Then a constant heat source of <inline-formula><tex-math id="math-121"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle 370^\circ K \end{document} ]]></tex-math></inline-formula> is applied.</p><fig id="figure-9"><label>Figure 8.</label><caption><p>Dimensions of heat source geometry, (a) circular, (b) triangular, (c) square, (d) hexagonal, (e) star, (f) star of David.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13809" mime-subtype="png" mimetype="image"><alt-text>Figure 8.</alt-text></graphic></fig><p>To allow particles to reach narrow corners, we use an unstructured particle distribution, and the particle spacing <inline-formula><tex-math id="math-122"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta p \end{document} ]]></tex-math></inline-formula> is set to be no larger than 0.2 cm. The simulation is carried out up to <inline-formula><tex-math id="math-123"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 3 0 ~ \mathrm { s } \end{document} ]]></tex-math></inline-formula> using a time step of <inline-formula><tex-math id="math-124"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \Delta t = 0 . 2 \mathrm { ~ s ~ } \end{document} ]]></tex-math></inline-formula>. The number of particles and the corresponding computational time for each heat-source eometr are summarized in <xref ref-type="table" rid="table-2">Table 2</xref>.</p><p>The heat distribution at <inline-formula><tex-math id="math-125"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 3 0 ~ \mathrm { s } \end{document} ]]></tex-math></inline-formula> for all heat sources is shown in <xref ref-type="fig" rid="figure-10">Figure 9</xref>. It can be seen that the heat spreads radially toward the edges of the plate, forming a circular pattern. The temperature decreases monotonically from the center to the edges. It can be observed that, among all heat sources, those with star geometries disperse heat more rapidly.</p><table-wrap id="table-2"><label>Table 2</label><caption><p>Number of particles and computational time for each heat source geometry.</p></caption><table><colgroup><col></col><col></col><col></col><col></col><col></col><col></col><col></col></colgroup><thead><tr><th scope="col">Geometry</th><th scope="col">Circular</th><th scope="col">Triangular</th><th scope="col">Square</th><th scope="col">Hexagonal</th><th scope="col">Star</th><th scope="col">Star of David</th></tr></thead><tbody><tr><td><inline-formula><tex-math id="math-126"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle N \end{document} ]]></tex-math></inline-formula></td><td>4259</td><td>4268</td><td>4308</td><td>4227</td><td>4259</td><td>4230</td></tr><tr><td>Comp. time <inline-formula><tex-math id="math-127"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle (s) \end{document} ]]></tex-math></inline-formula></td><td>37</td><td>36</td><td>39</td><td>37</td><td>37</td><td>35</td></tr></tbody></table></table-wrap><fig id="figure-10"><label>Figure 9</label><caption><p>Heat distribution at <inline-formula><tex-math id="math-128"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle t = 3 0 \ \mathrm { s } , \end{document} ]]></tex-math></inline-formula> (a) circular, (b) triangular, (c) square, (d) hexagonal, (e) star, (f) star of David.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13799" mime-subtype="jpeg" mimetype="image"><alt-text>Figure 9</alt-text></graphic></fig><p>To compare the rate of heat propagation, we plot the contours of a selected temperature for all heat source geometries. Here, we plot the contour for <inline-formula><tex-math id="math-129"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u = 3 3 0 ^ { \circ } \mathrm { K } \end{document} ]]></tex-math></inline-formula>, which is depicted in <xref ref-type="fig" rid="figure-11">Figure 10</xref> (left). It can be seen that the temperature range <inline-formula><tex-math id="math-130"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u = 3 3 0 ^ { \circ } \mathrm { K } \end{document} ]]></tex-math></inline-formula> for star geometries is wider than for other geometries. In addition, we also calculated the average plate temperature outside the heat source <inline-formula><tex-math id="math-131"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \bar{u} \end{document} ]]></tex-math></inline-formula>, which is shown in <xref ref-type="fig" rid="figure-11">Figure 10</xref> (right). The average temperature also shows that the star geometry disperses heat more quickly, compared to the other five geometries. The star geometry spreads heat faster because its extended tips reach farther toward cooler areas of the plate, creating stronger temperature diferences that accelerate difusion.</p><fig id="figure-11"><label>Figure 10.</label><caption><p>(Left) contours of u = 330◦K at t = 30 s.  (Right) average temperature as a function of time.</p></caption><graphic xlink:href="https://jims-a.org/index.php/jimsa/article/download/2246/535/13800" mime-subtype="png" mimetype="image"><alt-text>Figure 10.</alt-text></graphic></fig></sec><sec id="sec-9"><title>6. Conclusion</title><p>This study demonstrates that the Smoothed Particle Hydrodynamics (SPH) method can accurately simulate two-dimensional heat transfer on thin plates under various boundary conditions. Validation against analytical solutions for Dirichlet and homogeneous Neumann problems shows excellent agreement, as indicated by consistently low nRMSE values. The method was also applied to plates containing internal heat sources of equal area but diferent geometries, revealing that starshaped sources promote faster heat spread than other configurations. These results highlight the flexibility of SPH in handling complex boundary specifications and geometric variations.</p><p>Despite these strengths, the present formulation has several limitations. SPH requires user-defined parameters such as the smoothing length and the kernel function, both of which introduce uncertainty. In addition, the model used here solves only a scalar temperature field with fixed particle positions, which does not exploit the full potential of SPH for deforming or moving domains. The governing physics is limited to pure conduction, and the validation is restricted to rectangular domains and analytical benchmarks. Future work may include validation against analytical solutions in circular domains as well as comparisons with laboratory experiments, which will require more complex governing equations that incorporate heat sources, convection, or phase change. Extensions to fully coupled thermofluid systems, moving particles, and three-dimensional geometries would further strengthen SPH as a versatile tool for realistic heat-transfer modeling.</p></sec><sec id="sec-10"><title>Appendix</title><p>Details of the search for analytical solutions of the two-dimensional heat equation for homogeneous Neumann boundary conditions:</p><sec id="sec-11"><title>1. Separation of Variables</title><p>Suppose u can be expressed as the product of three functions, namely:</p><disp-formula id="equation-27"><tex-math id="math-132"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, t) = X (x) Y (y) T (t)\tag{24} \end{document} ]]></tex-math></disp-formula><p>By substituting (24) into the model (1) and applying the boundary conditions (4), we obtain the Sturm-Liouville problem</p><disp-formula id="equation-28"><tex-math id="math-133"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle X ^ {\prime \prime} + B X = 0, \quad X _ {x} (0) = X _ {x} (a) = 0,\tag{25} \end{document} ]]></tex-math></disp-formula><disp-formula id="equation-29"><tex-math id="math-134"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle Y ^ {\prime \prime} + C Y = 0, \quad Y _ {y} (0) = Y _ {y} (b) = 0,\tag{26} \end{document} ]]></tex-math></disp-formula><p>and</p><disp-formula id="equation-30"><tex-math id="math-135"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle T ^ {\prime} - \alpha (- B - C) T = 0.\tag{27} \end{document} ]]></tex-math></disp-formula><p>The solutions of (25) and (26) are</p><disp-formula id="equation-31"><tex-math id="math-136"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle X _ {m} (x) = B _ {m} \cos (\omega_ {m} x),\tag{28} \end{document} ]]></tex-math></disp-formula><disp-formula id="equation-32"><tex-math id="math-137"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle Y _ {n} (y) = C _ {n} \cos (\omega_ {n} y),\tag{29} \end{document} ]]></tex-math></disp-formula><p>where <inline-formula><tex-math id="math-138"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \omega _ { m } = \frac { m \pi } { a } \end{document} ]]></tex-math></inline-formula> and <inline-formula><tex-math id="math-139"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{array} { r } { \omega _ { n } = \frac { n \pi } { b } } \end{array} \end{document} ]]></tex-math></inline-formula>. Meanwhile the solution (27) is</p><p><inline-formula><tex-math id="math-140"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle T _ {m n} (t) = e ^ {- \lambda_ {m n} ^ {2} t}, \end{document} ]]></tex-math></inline-formula></p><p>where</p><disp-formula id="equation-33"><tex-math id="math-141"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \lambda_ {m n} ^ {2} = \alpha (\omega_ {m} ^ {2} + \omega_ {n} ^ {2}) \end{document} ]]></tex-math></disp-formula><p>, for <inline-formula><tex-math id="math-142"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle m, n \in \mathbb {N} \end{document} ]]></tex-math></inline-formula></p></sec><sec id="sec-12"><title>2. Superposition</title><p>For each pair <inline-formula><tex-math id="math-143"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle m \end{document} ]]></tex-math></inline-formula>, <inline-formula><tex-math id="math-144"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle n \end{document} ]]></tex-math></inline-formula> we have</p><disp-formula id="equation-34"><tex-math id="math-145"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle \begin{equation*}\begin{aligned}u_{mn}(x,y,t)&=X_m(x)Y_n(y)T_{mn}(t)\\&=A_{mn}\cos(\omega_m x)\cos(\omega_n y)e^{-\lambda_{mn}^{2}t},\end{aligned}\end{equation*} \end{document} ]]></tex-math></disp-formula><p>as a solution, where <inline-formula><tex-math id="math-146"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle A _ { m n } = B _ { m } C _ { n } \end{document} ]]></tex-math></inline-formula>. For each selection of constants <inline-formula><tex-math id="math-147"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle A _ { m n } \end{document} ]]></tex-math></inline-formula>, using the superposition principle, we obtain a general solution to the heat equation (1) with boundary conditions (4) as</p><disp-formula id="equation-35"><tex-math id="math-148"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle u (x, y, t) = \sum_ {m = 0} ^ {\infty} \sum_ {n = 0} ^ {\infty} A _ {m n} \cos (\omega_ {m} x) \cos (\omega_ {n} y) e ^ {- \alpha (\omega_ {m} ^ {2} + \omega_ {n} ^ {2}) t}.\tag{30} \end{document} ]]></tex-math></disp-formula><p>From the initial condition (19) we have</p><disp-formula id="equation-36"><tex-math id="math-149"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle f (x, y) = \sum_ {m = 0} ^ {\infty} \sum_ {n = 0} ^ {\infty} A _ {m n} \cos (\omega_ {m} x) \cos (\omega_ {n} y)\tag{31} \end{document} ]]></tex-math></disp-formula><p>which is a double Fourier series for <inline-formula><tex-math id="math-150"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle f ( x , y ) \end{document} ]]></tex-math></inline-formula>. If f is a function <inline-formula><tex-math id="math-151"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle C ^ { 2 } \end{document} ]]></tex-math></inline-formula>, then</p><disp-formula id="equation-37"><tex-math id="math-152"><![CDATA[ \documentclass{article} \usepackage{amsmath} \begin{document} \displaystyle A _ {m n} = \frac {4}{a b} \int_ {0} ^ {a} \int_ {0} ^ {b} f (x, y) \cos (\omega_ {m} x) \cos (\omega_ {n} y) d y d x\tag{32} \end{document} ]]></tex-math></disp-formula></sec></sec></body><back><ack><title>Acknowledgement</title><p>The author thanks the editors and reviewers who took the time to review the article.</p></ack><ref-list><title>References</title><ref id="BIBR-1"><element-citation publication-type="journal"><article-title>Heat transfer augmentation by recombination reactions in turbulent reacting boundary layers at elevated pressures</article-title><source>International Journal of Heat and Mass Transfer</source><volume>178</volume><issue>121628</issue><person-group person-group-type="author"><name><surname>Perakis</surname><given-names>N.</given-names></name><name><surname>Haidn</surname><given-names>O.J.</given-names></name><name><surname>Ihme</surname><given-names>M.</given-names></name></person-group><year>2021</year><pub-id pub-id-type="doi">10.1016/j.ijheatmasstransfer.2021.121628</pub-id></element-citation></ref><ref id="BIBR-2"><element-citation publication-type="journal"><article-title>Derivation and validation of heat transfer model for spark-ignition engine cylinder head</article-title><source>Appl. 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