pith. sign in

arxiv: 1004.0150 · v3 · submitted 2010-04-01 · ✦ hep-th · astro-ph.CO· gr-qc

Brane f(R) gravity cosmologies

classification ✦ hep-th astro-ph.COgr-qc
keywords branebulkcosmologicaltensorcontributionexistsgravitynon-static
0
0 comments X
read the original abstract

By the application of the generalized Israel junction conditions we derive cosmological equations for the fourth-order $f(R)$ brane gravity and study their cosmological solutions. We show that there exists a non-static solution which describes a four-dimensional de-Sitter $(dS_4)$ brane embedded in a five-dimensional anti-de-Sitter $(AdS_5)$ bulk for a vanishing Weyl tensor contribution. On the other hand, for the case of a non-vanishing Weyl tensor contribution, there exists a static brane only. We claim that in order to get some more general non-static $f(R)$ brane configurations, one needs to admit a dynamical matter energy-momentum tensor in the bulk rather than just a bulk cosmological constant.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.