Einstein-Cartan cosmologies

被引:37
|
作者
Bravo Medina, Sergio [1 ]
Nowakowski, Marek [1 ]
Batic, Davide [2 ]
机构
[1] Univ Los Andes, Dept Fis, Cra 1E 18A-10, Bogota, Colombia
[2] Khalifa Univ Sci & Technol, Dept Math, Main Campus, Abu Dhabi, U Arab Emirates
关键词
Torsion; Einstein-Cartan; Spin fluid; Torsion gravity; GENERAL-RELATIVITY; SPINNING FLUIDS; VARIATIONAL PRINCIPLE; PERFECT FLUIDS; TORSION; INFLATION; EQUATION; UNIVERSE;
D O I
10.1016/j.aop.2018.11.002
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Cosmologies based on General Relativity encompassing an anti-symmetric connection (torsion) can display nice desirable features as the absence of the initial singularity and the possibility of inflation in the early stage of the universe. After briefly reviewing the standard approach to the cosmology with torsion, we generalize it to demonstrate that several theories of torsion gravity are possible using different choices of the diffeomorphic invariants in the Lagrangians. As a result, distinct cosmologies emerge. In all of them it is possible that the universe avoids the initial singularity and passes through an initial accelerated expansion. Differences between these theories are highlighted. (C) 2018 Elsevier Inc. All rights reserved.
引用
收藏
页码:64 / 108
页数:45
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