pith. sign in

arxiv: astro-ph/0411209 · v2 · submitted 2004-11-08 · 🌌 astro-ph · gr-qc· hep-th

Cosmic Acceleration and Modified Gravitational Models

classification 🌌 astro-ph gr-qchep-th
keywords modelsacceleratingaccelerationcosmicgravitationallate-timemodifiedsolutions
0
0 comments X
read the original abstract

There is now overwhelming observational evidence that our Universe is accelerating in its expansion. I discuss how modified gravitational models can provide an explanation for this observed late-time cosmic acceleration. We consider specific low-curvature corrections to the Einstein-Hilbert action. Many of these models generically contain unstable de Sitter solutions and, depending on the parameters of the theory, late-time accelerating attractor solutions.

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.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution

    gr-qc 2017-05 accept novelty 2.0

    Modified gravity theories supply viable mathematical frameworks for inflation, bounces, and dark energy eras that match observational data.