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dc.contributor.authorNakerst, Goran
dc.contributor.authorDenysov, Sergiy
dc.contributor.authorHaque, Masudul
dc.date.accessioned2024-03-21T07:59:27Z
dc.date.available2024-03-21T07:59:27Z
dc.date.created2023-07-24T14:56:19Z
dc.date.issued2023
dc.identifier.citationPhysical Review E (PRE). 2023, 108 (1), .en_US
dc.identifier.issn2470-0045
dc.identifier.issn2470-0053
dc.identifier.urihttps://hdl.handle.net/11250/3123506
dc.description.abstractThe evolution of a complex multi-state system is often interpreted as a continuous-time Markovian process. To model the relaxation dynamics of such systems, we introduce an ensemble of random sparse matrices which can be used as generators of Markovian evolution. The sparsity is controlled by a parameter ϕ, which is the number of non-zero elements per row and column in the generator matrix. Thus, a member of the ensemble is characterized by the Laplacian of a directed regular graph with D vertices (number of system states) and 2ϕD edges with randomly distributed weights. We study the effects of sparsity on the spectrum of the generator. Sparsity is shown to close the large spectral gap that is characteristic of non-sparse random generators. We show that the first moment of the eigenvalue distribution scales as ∼ ϕ, while its variance is ∼ √ϕ. By using extreme value theory, we demonstrate how the shape of the spectral edges is determined by the tails of the corresponding weight distributions, and clarify the behavior of the spectral gap as a function of D. Finally, we analyze complex spacing ratio statistics of ultra-sparse generators, ϕ = const, and find that starting already at ϕ > 2, spectra of the generators exhibit universal properties typical of Ginibre’s Orthogonal Ensembleen_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleRandom sparse generators of Markovian evolution and their spectral propertiesen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionacceptedVersionen_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.doihttps://doi.org/10.1103/PhysRevE.108.014102
dc.identifier.cristin2163270
dc.source.journalPhysical Review E (PRE)en_US
dc.source.volume108en_US
dc.source.issue1en_US
dc.source.pagenumber22en_US


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