Post-Newtonian Approximation of Teleparallel Gravity Coupled with a Scalar Field
arXiv:1410.7715 · doi:10.1016/j.nuclphysb.2015.03.012
Abstract
We use the parameterized post-Newtonian (PPN) formalism to explore the weak field approximation of teleparallel gravity non-minimally coupling to a scalar field , with arbitrary coupling function and potential . We find that all the PPN parameters are identical to general relativity (GR), which makes this class of theories compatible with the Solar System experiments. This feature also makes the theories quite different from the scalar-tensor theories, which might be subject to stringent constraints on the parameter space, or need some screening mechanisms to pass the Solar System experimental constraints.
15 pages, revtex4; v2: discussions added, Nucl. Phys. B in press; v3: published version
References in corpus (14)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Dark torsion as the cosmic speed-up
- Einstein's Other Gravity and the Acceleration of the Universe
- Cosmological constant and vacuum energy: old and new ideas
- Conformal transformation in theories
- Constraints on scalar-tensor models of dark energy from observational and local gravity tests
- Scalar Tensor Teleparallel Dark Gravity via Noether Symmetry
- Post-Newtonian parameters gamma and beta of scalar-tensor gravity with a general potential
- Teleparallel dark energy model with a fermionic field via Noether symmetry
- Singularity Problem in Teleparallel Dark Energy Models
- Acausality and Nonunique Evolution in Generalized Teleparallel Gravity
- Parametrized Post-Newtonian Limit of Teleparallel Dark Energy Model
- Exact cosmological solution of a Scalar-Tensor Gravity theory compatible with the model
Cited by in corpus (25)
- Teleparallel Gravity: From Theory to Cosmology
- Covariant formulation of scalar-torsion gravity
- Bounce inflation in Cosmology: A unified inflaton-quintessence field
- Solar System Tests in Modified Teleparallel Gravity
- Scalar-torsion theories of gravity III: analogue of scalar-tensor gravity and conformal invariants
- Scalar-torsion theories of gravity I: general formalism and conformal transformations
- Scalar-torsion theories of gravity II: theory
- General relativity as an attractor for scalar-torsion cosmology
- Post-Newtonian limit of Teleparallel Horndeski gravity
- Higgs inflation and teleparallel gravity
- Parameterized post-Newtonian limit of general teleparallel gravity theories
- Post-Newtonian parameter for multiscalar-tensor gravity with a general potential
- Stability of scalar perturbations in scalar-torsion gravity theories in the presence of a matter fluid
- Post-Newtonian limit of generalized scalar-torsion theories of gravity
- Post-Newtonian limit of scalar-torsion theories of gravity as analogue to scalar-curvature theories
- Symmetron and de Sitter attractor in a teleparallel model of cosmology
- Spherical collapse model and cluster number counts in power law gravity
- Onset of acceleration in a Universe initially filled by dark and baryonic matters in nonminimally coupled teleparallel model
- Inflation with teleparallelism: Can torsion generate primordial fluctuations without local Lorentz symmetry?
- Unexplored regions in teleparallel gravity: Sign-changing dark energy density
- Parametrized post-Newtonian limit of the Nieh-Yan modified teleparallel gravity
- Interacting Quintessence in a New Scalar-Torsion Gravity
- Parameterized second post-Newtonian framework with conservation Laws
- Global portraits of nonminimal teleparallel inflation
- Neutron Stars in Scalar Torsion Theories with Nonminimal Coupling