Geodesic Deviation Equation in gravity
arXiv:1501.00103 · doi:10.1103/PhysRevD.91.084023
Abstract
In this work, we show that it is possible to study the notion of geodesic deviation equation in gravity, in spite of the fact that in teleparallel gravity there is no notion of geodesics, and the torsion is responsible for the appearance of gravitational interaction. In this regard, we obtain the GR equivalent equations for gravity which are in the modified gravity form such as gravity. Then, we obtain the GDE within the context of this modified gravity. In this way, the obtained geodesic deviation equation will correspond to the gravity. Eventually, we extend the calculations to obtain the modification of Matting relation.
13 pages, 7 figures
References in corpus (23)
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- On Born-Infeld Gravity in Weitzenbock spacetime
- Cosmological perturbations in f(T) gravity
- Observational constraints on theory
- f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
- Teleparallel equivalent of Gauss-Bonnet gravity and its modifications
- Generalizations of teleparallel gravity and local Lorentz symmetry
- Good and bad tetrads in f(T) gravity
- Solar system constraints on f(T) gravity
- Observational information for f(T) theories and Dark Torsion
- Nonminimal torsion-matter coupling extension of f(T) gravity
- Conformal transformation in theories
- Static Solutions with Spherical Symmetry in f(T) Theories
- Exact charged black-hole solutions in D-dimensional f(T) gravity: torsion vs curvature analysis
- Anisotropic Universe Models in f(T) Gravity
- Energy conditions bounds on f(T) gravity
- A special exact spherically symmetric solution in f(T) gravity theories
- Energy conditions in generalized teleparallel gravity models
- Schwarzschild solution in extended teleparallel gravity
- Geodesic Congruences in the Palatini f(R) Theory