<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE ArticleSet PUBLIC "-//NLM//DTD PubMed 2.7//EN" "https://dtd.nlm.nih.gov/ncbi/pubmed/in/PubMed.dtd">
<ArticleSet>
<Article>
<Journal>
				<PublisherName>Shahid Beheshti University</PublisherName>
				<JournalTitle>Computational Mathematics and Computer Modeling with Applications (CMCMA)</JournalTitle>
				<Issn>2783-4859</Issn>
				<Volume>5</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2026</Year>
					<Month>04</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>A Novel Hybrid Architecture Combining High-Order B-Splines and Physics-Informed Neural Networks for Solving an Astrophysical Model</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>1</FirstPage>
			<LastPage>14</LastPage>
			<ELocationID EIdType="pii">106946</ELocationID>
			
<ELocationID EIdType="doi">10.48308/CMCMA.5.1.1</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Sima</FirstName>
					<LastName>Naraghi</LastName>
<Affiliation>Department of Applied Mathematics, Faculty of Mathematical Sciences, Shahid Beheshti University, Tehran, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Kourosh</FirstName>
					<LastName>Parand</LastName>
<Affiliation>Department of Computer and Data Sciences, Faculty of Mathematical Sciences, Shahid Beheshti University, Tehran, Iran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2026</Year>
					<Month>01</Month>
					<Day>30</Day>
				</PubDate>
			</History>
		<Abstract>In this paper, we present a novel architecture for approximating solutions to differential equations in astrophysics. Our approach introduces the innovative use of nonlinear B-spline basis functions as activation functions within a neural network. Furthermore, we develop a physics-informed B-spline neural network framework with associated control points to address the Lane--Emden equations, frequently encountered in astronomy. This new method offers enhanced accuracy while requiring fewer epochs than conventional neural networks.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Physics-Informed Neural Networks</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">High-Order B-Spline</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Astrophysical Modeling</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">{Lane--Emden equations}</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Numerical Methods</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://cmcma.sbu.ac.ir/article_106946_6507053b723f565e3a0fb47d5b99d204.pdf</ArchiveCopySource>
</Article>
</ArticleSet>
