Effective Potential of Scalar-Tensor Gravity
arXiv:2007.06306 · doi:10.1088/1361-6382/abc572
Abstract
Effective potential of a scalar field induced by weak gravity is studied. The set of operators relevant for leading effects and preserving the second order of field equations is found. It is shown that only the mass term and a specific Brans-Dicke-like interaction are relevant within such a setup. The explicit form of the potential is found. The model has room for a natural inflationary scenario similar to the well-known case of the Starobinsky inflation. Possible implications for the Standard Model are highlighted.
Minor corrections. Class. Quantum Grav (2020)
References in corpus (31)
- f(R) Theories Of Gravity
- Modified Gravity and Cosmology
- f(R) theories
- Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
- Chameleon Cosmology
- Testing General Relativity with Present and Future Astrophysical Observations
- General relativity as an effective field theory: The leading quantum corrections
- Generalized G-inflation: Inflation with the most general second-order field equations
- Quantum Gravity in Everyday Life: General Relativity as an Effective Field Theory
- Horndeski theory and beyond: a review
- Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian
- The Relation between Physical and Gravitational Geometry
- General second order scalar-tensor theory, self tuning, and the Fab Four
- Testing General Relativity in Cosmology
- Tests of Chameleon Gravity
- f(R) Gravity and Chameleon Theories
- Question of quantum equivalence between Jordan frame and Einstein frame
- Bending of Light in Quantum Gravity
- The renormalization group for non-renormalizable theories: Einstein gravity with a scalar field
- Renormalization-Group Improved Effective Lagrangian for Interacting Theories in Curved Spacetime
- One-loop divergences for gravity non-minimally coupled to a multiplet of scalar fields: calculation in the Jordan frame. I. The main results
- One loop renormalization of the four-dimensional theory for quantum dilaton gravity.
- Renormalization-Group Improved Effective Potential for Interacting Theories with Several Mass Scales in Curved Spacetime
- Effective Lagrangian and the back-reaction problem in a self-interacting scalar theory in curved spacetime
- Renormalization-Group Improved Effective Potential for Finite Grand Unified Theories in Curved Spacetime
- Improved Effective Potential in Curved Spacetime and Quantum Matter - Higher Derivative Gravity Theory
- Three Waves for Quantum Gravity
- Fab Four Effective Field Theory Treatment
- Scalar-tensor black holes in an expanding universe
- Basic issues of conservative approaches to quantum theory of gravity
- Fab Four self-interaction in quantum regime
Cited by in corpus (8)
- Dynamical features and shadows of quantum Schwarzschild black hole in effective field theories of gravity
- Effective potential of scalar-tensor gravity with quartic self-interaction of scalar field
- On the Coupling of Generalized Proca Fields to Degenerate Scalar-Tensor Theories
- Beyond Horndeski interactions induced by quantum effects
- Inflationary solutions in the simplest gravity model with conformal symmetry
- Black Holes in Einstein-scalar-Gauss-Bonnet model probed with scattering amplitudes
- FeynGrav and Recent Progress in Computational Perturbative Quantum Gravity
- Inflation in simple one-loop effective potentials of perturbative quantum gravity