From Big to Little Rip in modified F(R,G) gravity
classification
🌀 gr-qc
keywords
gravitymodifiedcosmologicalfuturelittlecosmologydemonstratedderive
pith:G6LMFAW3 Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{G6LMFAW3}
Prints a linked pith:G6LMFAW3 badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
We discuss the cosmological reconstruction in modified Gauss-Bonnet (GB) gravity. It is demonstrated that the modified GB gravity may describe the most interesting features of late-time cosmology. We derive explicit form of effective phantom cosmological models ending by the finite-time future singularity (Big Rip) and without singularities in the future (Little Rip).
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.