Stephani Cosmological Models with Accelerated Expansion

M. P. Korkina; E. M. Kopteva; A. A. Egurnov

doi:10.1007/s11182-016-0776-x

Stephani Cosmological Models with Accelerated Expansion

作者: Korkina M.P.¹, Kopteva E.M.¹, Egurnov A.A.¹
隶属关系:
1. Dnepropetrovsk National University
期: 卷 59, 编号 3 (2016)
页面: 328-334
栏目: Elementary Particle Physics and Field Theory
URL: https://journals.rcsi.science/1064-8887/article/view/237065
DOI: https://doi.org/10.1007/s11182-016-0776-x
ID: 237065

如何引用文章

全文:

开放存取

##reader.subscriptionAccessGranted##
受限制的访问

订阅存取

详细
作者简介
参考
补充文件
统计

详细

Stephani cosmological models are considered which describe spacetimes for a shear-free matter distribution and include Friedmann models as a particular case. The possibility is considered of constructing cosmological models in which a change of sign of the acceleration of the Universe expansion arises only due to curvature.