Abstract
AbstractIn the context of Finsler–Randers theory we consider, for the first time, the cosmological scenario of the varying vacuum. In particular, we assume the existence of a cosmological fluid source described by an ideal fluid and the varying vacuum terms. We determine the cosmological history of this model by performing a detailed study on the dynamics of the field equations. We determine the limit of General Relativity, while we find new eras in the cosmological history provided by the geometrodynamical terms provided by the Finsler–Randers theory.
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Reference147 articles.
1. A.G. Riess et al., Astron. J. 116, 1009 (1998)
2. S. Perlmutter et al., Astrophys. J. 517, 565 (1999)
3. N. Aghanim et al., arXiv:1807.06209 [astro-ph.CO]
4. E.J. Copeland, M. Sami, S. Tsujikawa, Int. J. Mod. Phys. D 15, 1753 (2006)
5. P.J.E. Peebles, B. Ratra, Rev. Mod. Phys. 75, 559 (2003)
Cited by
23 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献