| dc.contributor.author | Berkoez, G. | |
| dc.contributor.author | Sevinc, Oe. | |
| dc.date.accessioned | 2021-03-04T18:12:47Z | |
| dc.date.available | 2021-03-04T18:12:47Z | |
| dc.identifier.citation | Berkoez G., Sevinc O., "Bianchi models with Chaplygin gas", 6th International Conference of the Balkan-Physical-Union, İstanbul, Türkiye, 22 - 26 Ağustos 2006, cilt.899, ss.141-142 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_89801b72-08ae-49ac-bef1-e0db27f70c63 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/93248 | |
| dc.identifier.uri | https://doi.org/10.1063/1.2733076 | |
| dc.description.abstract | Einstein Gravitational Field Equations (EFE) of Chaplygin gas dominated Bianchi-type models are obtained by using metric approximation. The solutions of equations for a special case, namely Bianchi I model which is a generalization of isotropic Friedmann-Robertson-Walker (FRW) cosmology, are obtained. The early and late behaviours of some kinematic parameters in model are presented in graphically. | |
| dc.language.iso | eng | |
| dc.subject | Disiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları | |
| dc.subject | Temel Bilimler | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Fizik | |
| dc.subject | FİZİK, MULTİDİSİPLİNER | |
| dc.title | Bianchi models with Chaplygin gas | |
| dc.type | Bildiri | |
| dc.contributor.department | İstanbul Üniversitesi , , | |
| dc.identifier.volume | 899 | |
| dc.contributor.firstauthorID | 132956 | |
