Inhomogeneous Universe in f(T) Theory
arXiv:1205.0565 · doi:10.1134/S0202289314020108
Abstract
We obtain the equations of motions of the theory considering the Lemaître-Tolman-Bondi's metric for a set of diagonal and non-diagonal tetrads. In the case of diagonal tetrads the equations of motion of the theory impose a constant torsion or the same equations of the General Relativity, while in the case of non-diagonal set the equations are quite different from that obtained in GR. We show a simple example of an universe dominated by the matter for the two cases. The comparison of the mass in the non-diagonal case shows a sort of increased with respect to the diagonal one. We also perform two examples for the non-diagonal case. The first concerns a black hole solution of type Sshwarzschild which presents a temperature higher than that of Schwarzschild, and a black hole in a dust-dominated universe.
21 pages
References in corpus (17)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- f(R,T) gravity
- Dark energy in modified Gauss-Bonnet gravity: late-time acceleration and the hierarchy problem
- Generalizations of teleparallel gravity and local Lorentz symmetry
- Good and bad tetrads in f(T) gravity
- Solar system constraints on f(T) gravity
- Time drift of cosmological redshifts as a test of the Copernican principle
- Anisotropic Universe Models in f(T) Gravity
- CMB anisotropies seen by an off-center observer in a spherically symmetric inhomogeneous universe
- Analysis of F(R,T) Gravity Models Through Energy Conditions
- Local Void vs Dark Energy: Confrontation with WMAP and Type Ia Supernovae
- Lemaitre-Tolman-Bondi collapse from the perspective of loop quantum gravity
- Cylindrical Solutions in Modified f(T) Gravity
- Accelerating cosmology in F(T) gravity with scalar field
- The Great Attractor and the Shapley Concentration
- Evaporation phenomena in f(T) gravity
- Metric-affine Myrzakulov gravity and its generalizations
Cited by in corpus (17)
- f(T) teleparallel gravity and cosmology
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- New observational constraints on f(T) gravity from cosmic chronometers
- A Built-in Inflation in the -Cosmology
- Phase Portraits of general f(T) Cosmology
- Finite-time future singularities models in gravity and the effects of viscosity
- Black-Bounce in Gravity
- Born-Infeld and Charged Black Holes with non-linear source in Gravity
- Modelling of a compact anisotropic star as an anisotropic fluid sphere in gravity
- Black holes and regular black holes in coincident gravity coupled to nonlinear electrodynamics
- Unimodular gravity
- Evaporation phenomena in f(T) gravity
- Realistic f(T) model describing the de Sitter epoch of the dark energy dominated universe
- Relativistic virial relation for cosmological structures
- Interactions of some fluids with dark energy in f(T) theory
- A new type of second order cosmological lagrangians