Radiation dominated era and the power of general relativity
arXiv:1205.6954 · doi:10.1209/0295-5075/99/10001
Abstract
An analysis in the framework of the radiation dominated era permits to put bounds on the weak modification of general relativity which arises from the Lagrangian R^{1+epsilon}. Such a theory has been recently discussed in various papers in the literature. The new bounds together with previous ones in the literature rule out this theory in an ultimate way.
arXiv comment7 pages, 1 figure, accepted for publication in Europhysics Letters
References in corpus (26)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Extended Theories of Gravity
- Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
- The Confrontation between General Relativity and Experiment
- Can modified gravity explain accelerated cosmic expansion?
- Unifying inflation with LambdaCDM epoch in modified f(R) gravity consistent with Solar System tests
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- The Power of General Relativity
- Interferometric detection of gravitational waves: the definitive test for General Relativity
- Matter instability in modified gravity
- Non-singular exponential gravity: a simple theory for early- and late-time accelerated expansion
- de Sitter space and the equivalence between f(R) and scalar-tensor gravity
- Time-dependent matter instability and star singularity in gravity
- Further Exact Cosmological Solutions to Higher-Order Gravity Theories
- Repulsive Casimir effect from extra dimensions and Robin boundary conditions: from branes to pistons
- Initial and final de Sitter universes from modified gravity
- Spherically Symmetric Solutions to Fourth-Order Theories of Gravity
- Solar system constraints on R gravity
- Exact cosmological solutions of scale-invariant gravity theories
- Inflation from R^2 gravity: a new approach using nonlinear electrodynamics
- Higher-order gravity and the cosmological background of gravitational waves
- Primordial production of massive relic gravitational waves from a weak modification of General Relativity
- R^n gravity and the chameleon
- A spherically symmetric and stationary universe from a weak modification of general relativity
- A precise response function for the magnetic component of Gravitational Waves in Scalar-Tensor Gravity