Deep learning-assisted Hubble parameter analysis
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.
Anahtar Kelimeler
- Scopus
- 2
- WoS
- 2
- OpenAlex
- 2
Tam Kayıt
| Alan | Değer | Dil |
|---|---|---|
| dc.contributor.author | Salti, Mehmet | |
| dc.contributor.author | Kangal, Evrim Ersin | |
| dc.contributor.author | Zengin, Bilgin | |
| dc.date.accessioned | 2026-10-28T14:55:14.413014528Z | |
| dc.date.available | 2026-10-28T14:55:14.413014528Z | |
| dc.date.issued | 2024 | |
| dc.description.abstract | 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. | |
| dc.identifier.articlenumber | 2350202 | |
| dc.identifier.doi | 10.1142/s0217732323502024 | |
| dc.identifier.eissn | 1793-6632 | |
| dc.identifier.issn | 0217-7323 | |
| dc.identifier.issue | 4 | |
| dc.identifier.scopus | 2-s2.0-85186421938 | |
| dc.identifier.uri | https://rdlopen.rawdatalibrary.net/r/munzur/2327 | |
| dc.identifier.volume | 39 | |
| dc.identifier.wos | WOS:001176258100006 | |
| dc.language.iso | en | |
| dc.publisher | World Scientific | |
| dc.relation.ispartof | Modern Physics Letters A | |
| dc.rights | info:eu-repo/semantics/closedAccess | |
| dc.subject | artificial intelligence | |
| dc.subject | Cosmology | |
| dc.subject | deep learning | |
| dc.subject | Hubble parameter | |
| dc.subject.classification | Astronomy & Astrophysics | |
| dc.subject.classification | Physics, Nuclear | |
| dc.subject.classification | Physics, Particles & Fields | |
| dc.subject.classification | Physics, Mathematical | |
| dc.subject.classification | Physics | |
| dc.subject.other | DYNAMICAL MASS MEASUREMENTS | |
| dc.subject.other | MACHINE | |
| dc.subject.other | UNIVERSE | |
| dc.subject.other | SUPERNOVAE | |
| dc.subject.other | MODEL | |
| dc.subject.other | GAS | |
| dc.subject.other | BIG | |
| dc.title | Deep learning-assisted Hubble parameter analysis | |
| dc.type | Article | |
| rdl.citation.openalex | 2 | |
| rdl.citation.scopus | 2 | |
| rdl.citation.wos | 2 | |
| rdl.oa.status | closed | |
| rdl.scopus.quartile | Q2 | |
| rdl.source.index | SCOPUS | |
| rdl.source.index | WOS | |
| rdl.wos.index | Science Citation Index Expanded (SCI-EXPANDED) |
