6+1 lessons from f(R) gravity
arXiv:0810.5594 · doi:10.1088/1742-6596/189/1/012039
Abstract
There has been a recent stimulus in the study of alternative theories of gravity lately, mostly triggered from combined motivation coming from cosmology/astrophysics and high energy physics. Among the proposed theories, one that has attracted much attention is f(R) gravity. It is certainly debatable whether such a simplistic modification of General Relativity can constitute a viable alternative theory of gravitation. However, it is quite straightforward to see the merits of such a theory when viewed as a toy theory whose role is to help us understand the implications and difficulties of beyond-Einstein gravity. Under this perspective, I review some of the main lessons we seem to have learned from the study of f(R) gravity in the recent past.
Talk given at the 13th Conference on Recent Developments in Gravity (NEBXIII), Thessaloniki, Greece, 4-6 Jun 2008
References in corpus (17)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Disappearing cosmological constant in f(R) gravity
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
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- A no-go theorem for polytropic spheres in Palatini f(R) gravity
- Perturbed Kerr Black Holes can probe deviations from General Relativity
- Curvature scalar instability in f(R) gravity
- Curvature singularities, tidal forces and the viability of Palatini f(R) gravity
- How (Not) to Palatini