Cycle-Star Motifs: Network Response to Link Modifications

dc.authoridEroglu, Deniz/0000-0001-6725-6949
dc.authorscopusid57219787223
dc.authorscopusid59035647900
dc.authorscopusid37006533200
dc.authorscopusid56027158200
dc.authorwosidEroglu, Deniz/F-9587-2013
dc.contributor.authorEroğlu, Deniz
dc.contributor.authorKiran, Narcicegi
dc.contributor.authorEroglu, Deniz
dc.contributor.authorPereira, Tiago
dc.date.accessioned2024-06-23T21:37:45Z
dc.date.available2024-06-23T21:37:45Z
dc.date.issued2024
dc.departmentKadir Has Universityen_US
dc.department-temp[Bakrani, Sajjad; Kiran, Narcicegi; Eroglu, Deniz] Kadir Has Univ, Fac Engn & Nat Sci, TR-34083 Istanbul, Turkiye; [Bakrani, Sajjad; Kiran, Narcicegi; Pereira, Tiago] Univ Sao Paulo, Inst Ciencias Matemat & Computacao, Sao Carlos, Brazil; [Pereira, Tiago] Imperial Coll London, Dept Math, London SW7 2AZ, Englanden_US
dc.descriptionEroglu, Deniz/0000-0001-6725-6949en_US
dc.description.abstractUnderstanding efficient modifications to improve network functionality is a fundamental problem of scientific and industrial interest. We study the response of network dynamics against link modifications on a weakly connected directed graph consisting of two strongly connected components: an undirected star and an undirected cycle. We assume that there are directed edges starting from the cycle and ending at the star (master-slave formalism). We modify the graph by adding directed edges of arbitrarily large weights starting from the star and ending at the cycle (opposite direction of the cutset). We provide criteria (based on the sizes of the star and cycle, the coupling structure, and the weights of cutset and modification edges) that determine how the modification affects the spectral gap of the Laplacian matrix. We apply our approach to understand the modifications that either enhance or hinder synchronization in networks of chaotic Lorenz systems as well as R & ouml;ssler. Our results show that the hindrance of collective dynamics due to link additions is not atypical as previously anticipated by modification analysis and thus allows for better control of collective properties.en_US
dc.description.sponsorshipTUBITAK; BAGEP Award of the Science Academy, Turkey; Newton Advanced Fellowship of the Royal Society [NAF \ \, 180236, 1709-16124]; FAPESP [2023/04294-0]; Leverhulme Trust [RPG-2021-072]; [119F125]en_US
dc.description.sponsorshipSB, NK, and DE were supported by TUBITAK Grant No. 119F125. DE was supported by the BAGEP Award of the Science Academy, Turkey. TP was supported by a Newton Advanced Fellowship of the Royal Society NAF \ \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\backslash $$\end{document} R1 \ \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\backslash $$\end{document} 180236, by Serrapilheira Institute (Grant No. Serra- 1709-16124), and FAPESP (grant 2013/07375-0). SB and TP acknowledge the support of FAPESP (grant no. 2023/04294-0). SB acknowledges the support of Leverhulme Trust grant RPG-2021-072.en_US
dc.identifier.citation0
dc.identifier.doi10.1007/s00332-024-10034-6
dc.identifier.issn0938-8974
dc.identifier.issn1432-1467
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-85192143593
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1007/s00332-024-10034-6
dc.identifier.urihttps://hdl.handle.net/20.500.12469/5741
dc.identifier.volume34en_US
dc.identifier.wosWOS:001214836400001
dc.identifier.wosqualityQ1
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectLaplacian matrixen_US
dc.subjectSpectral gapen_US
dc.subjectBraess's paradoxen_US
dc.subjectEigenvalue modificationen_US
dc.subjectEigenvalue perturbationen_US
dc.subjectGlobal perturbationen_US
dc.subjectNetwork modificationen_US
dc.subjectSpectral analysisen_US
dc.titleCycle-Star Motifs: Network Response to Link Modificationsen_US
dc.typeArticleen_US
dspace.entity.typePublication
relation.isAuthorOfPublication5bae555f-a8aa-4b95-bcfe-54cc47812e13
relation.isAuthorOfPublication.latestForDiscovery5bae555f-a8aa-4b95-bcfe-54cc47812e13

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