One-loop f(R) Gravitational Modified Models
arXiv:hep-th/0511233 · doi:10.1088/0305-4470/39/21/S15
Abstract
The one-loop quantisation of a general class of modified gravity models around a classical de Sitter background is presented. Application to the stability of the models is addressed.
Latex, 8 pages, no figures. To appear in Journal of Physics A. Two references added
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Cited by in corpus (40)
- f(R) Theories Of Gravity
- Beyond the Cosmological Standard Model
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- String-inspired Gauss-Bonnet gravity reconstructed from the universe expansion history and yielding the transition from matter dominance to dark energy
- Matter instability in modified gravity
- The (pseudo)issue of the conformal frame revisited
- Spherical symmetry in -gravity
- de Sitter space and the equivalence between f(R) and scalar-tensor gravity
- Solar System experiments do not yet veto modified gravity models
- Static Spherically Symmetric Solutions in F(R) Gravity
- A viability criterion for modified gravity with an extra force
- Classifying and avoiding singularities in the alternative gravity dark energy models
- Viability of f(R) Theories with Additional Powers of Curvature
- Dark energy and dust matter phases from an exact -cosmology model
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- gravity constrained by PPN parameters and stochastic background of gravitational waves
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