dc.contributor.author | Sofuoglu, DEĞER | |
dc.date.accessioned | 2021-03-05T07:37:47Z | |
dc.date.available | 2021-03-05T07:37:47Z | |
dc.date.issued | 2016 | |
dc.identifier.citation | Sofuoglu D., "Rotating and expanding Bianchi type-IX model in f (R, T) theory of gravity", ASTROPHYSICS AND SPACE SCIENCE, cilt.361, 2016 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.other | vv_1032021 | |
dc.identifier.other | av_94cf6aa8-57d7-4fe5-9a71-01c39cd91879 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/100223 | |
dc.identifier.uri | https://doi.org/10.1007/s10509-015-2593-z | |
dc.description.abstract | The spatially homogeneous shear-free, rotating and expanding Bianchi type-IX universe has been considered in the presence of perfect fluid in f (R, T) theory of gravity. The exact solution of the field equations has been obtained and the functional form of f (R, T) = R + 2f (T) gravity has been reconstructed. The existence of such a solution suggests that the general relativistic shear-free perfect fluid conjecture which claims that a shear-free perfect fluid cannot rotate and expand at the same time, is not valid in this modified theory. | |
dc.language.iso | eng | |
dc.subject | Fizik | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Temel Bilimler | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Uzay bilimi | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.title | Rotating and expanding Bianchi type-IX model in f (R, T) theory of gravity | |
dc.type | Makale | |
dc.relation.journal | ASTROPHYSICS AND SPACE SCIENCE | |
dc.contributor.department | İstanbul Üniversitesi , , | |
dc.identifier.volume | 361 | |
dc.identifier.issue | 1 | |
dc.contributor.firstauthorID | 227340 | |