Deep learning-assisted Hubble parameter analysis

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Özet

We turn our attention on evaluating the most recent Hubble parameter data measured via the differential evolution of cosmic-chronometers from a deep learning perspective. To achieve this goal, we start our investigation by introducing the selected theoretical setup and compiling the most recent statistical data obtained in cosmology experiments. Then we implement a tuned version of the long-short term memory (LSTM) architecture and run it to predict possible values of the Cosmic Hubble parameter for different red-shift states. Since we observe a good correlation between the observed and predicted datasets of the Hubble parameter, we conclude that the machine learning approaches can play important roles in the future cosmology investigations.

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https://rdlopen.rawdatalibrary.net/r/munzur/2327Resmi atıflarda kullanılan kalıcı adres
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https://doi.org/10.1142/s0217732323502024Yayıncı resmi DOI adresi
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AlanDeğerDil
dc.contributor.authorSalti, Mehmet
dc.contributor.authorKangal, Evrim Ersin
dc.contributor.authorZengin, Bilgin
dc.date.accessioned2026-10-28T14:55:14.413014528Z
dc.date.available2026-10-28T14:55:14.413014528Z
dc.date.issued2024
dc.description.abstractWe turn our attention on evaluating the most recent Hubble parameter data measured via the differential evolution of cosmic-chronometers from a deep learning perspective. To achieve this goal, we start our investigation by introducing the selected theoretical setup and compiling the most recent statistical data obtained in cosmology experiments. Then we implement a tuned version of the long-short term memory (LSTM) architecture and run it to predict possible values of the Cosmic Hubble parameter for different red-shift states. Since we observe a good correlation between the observed and predicted datasets of the Hubble parameter, we conclude that the machine learning approaches can play important roles in the future cosmology investigations.
dc.identifier.articlenumber2350202
dc.identifier.doi10.1142/s0217732323502024
dc.identifier.eissn1793-6632
dc.identifier.issn0217-7323
dc.identifier.issue4
dc.identifier.scopus2-s2.0-85186421938
dc.identifier.urihttps://rdlopen.rawdatalibrary.net/r/munzur/2327
dc.identifier.volume39
dc.identifier.wosWOS:001176258100006
dc.language.isoen
dc.publisherWorld Scientific
dc.relation.ispartofModern Physics Letters A
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectartificial intelligence
dc.subjectCosmology
dc.subjectdeep learning
dc.subjectHubble parameter
dc.subject.classificationAstronomy & Astrophysics
dc.subject.classificationPhysics, Nuclear
dc.subject.classificationPhysics, Particles & Fields
dc.subject.classificationPhysics, Mathematical
dc.subject.classificationPhysics
dc.subject.otherDYNAMICAL MASS MEASUREMENTS
dc.subject.otherMACHINE
dc.subject.otherUNIVERSE
dc.subject.otherSUPERNOVAE
dc.subject.otherMODEL
dc.subject.otherGAS
dc.subject.otherBIG
dc.titleDeep learning-assisted Hubble parameter analysis
dc.typeArticle
rdl.citation.openalex2
rdl.citation.scopus2
rdl.citation.wos2
rdl.oa.statusclosed
rdl.scopus.quartileQ2
rdl.source.indexSCOPUS
rdl.source.indexWOS
rdl.wos.indexScience Citation Index Expanded (SCI-EXPANDED)