Holographic reconstruction of scalar fields in extended Kaluza Klein cosmology
Özet
In recent years, many studies have been conducted to reconstruct the physical properties of scalar fields by establishing a connection between some energy densities and a scalar field of dark energies. In this paper, using the extended five-dimensional (5D) Kaluza- Klein model, we establish a correspondence among modified holographic dark energy and the tachyon, K-essence and dilaton scalar-field models. We also graphically illustrate the evolution of the equation-of-state parameter versus time.
Anahtar Kelimeler
RDL Kalıcı Bağlantı (PID)
https://rdlopen.rawdatalibrary.net/r/munzur/3194Resmi atıflarda kullanılan kalıcı adresİndeks kayıtları
Kaydın indeks veri tabanlarındaki sayfası (aktarımda alınan kayıt numarasıyla). Erişim, indeksin kendi koşullarına bağlıdır.Atıflar
- Scopus
- 7
- WoS
- 7
- OpenAlex
- 7
Tam Kayıt
| Alan | Değer | Dil |
|---|---|---|
| dc.contributor.author | Korunur, Murat | |
| dc.date.accessioned | 2026-10-28T14:56:19.493696721Z | |
| dc.date.available | 2026-10-28T14:56:19.493696721Z | |
| dc.date.issued | 2018 | |
| dc.description.abstract | In recent years, many studies have been conducted to reconstruct the physical properties of scalar fields by establishing a connection between some energy densities and a scalar field of dark energies. In this paper, using the extended five-dimensional (5D) Kaluza- Klein model, we establish a correspondence among modified holographic dark energy and the tachyon, K-essence and dilaton scalar-field models. We also graphically illustrate the evolution of the equation-of-state parameter versus time. | |
| dc.identifier.articlenumber | 1850002 | |
| dc.identifier.doi | 10.1142/s0217732318500025 | |
| dc.identifier.eissn | 1793-6632 | |
| dc.identifier.issn | 0217-7323 | |
| dc.identifier.issue | 1 | |
| dc.identifier.scopus | 2-s2.0-85039557246 | |
| dc.identifier.uri | https://rdlopen.rawdatalibrary.net/r/munzur/3194 | |
| dc.identifier.volume | 33 | |
| dc.identifier.wos | WOS:000419927400003 | |
| dc.language.iso | en | |
| dc.publisher | World Scientific Publishing Co. Pte Ltd | |
| dc.relation.ispartof | Modern Physics Letters A | |
| dc.rights | info:eu-repo/semantics/closedAccess | |
| dc.subject | Kaluza-Klein cosmology | |
| dc.subject | Modified holographic dark energy | |
| dc.subject | Scalar field | |
| 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 | DARK ENERGY MODELS | |
| dc.subject.other | COMPONENT | |
| dc.subject.other | EQUATION | |
| dc.subject.other | DYNAMICS | |
| dc.subject.other | RICCI | |
| dc.title | Holographic reconstruction of scalar fields in extended Kaluza Klein cosmology | |
| dc.type | Article | |
| rdl.citation.openalex | 7 | |
| rdl.citation.scopus | 7 | |
| rdl.citation.wos | 7 | |
| rdl.oa.status | closed | |
| rdl.scopus.quartile | Q3 | |
| rdl.source.index | SCOPUS | |
| rdl.source.index | WOS | |
| rdl.wos.index | Science Citation Index Expanded (SCI-EXPANDED) |
