Violation of causality in gravity
arXiv:1705.02226 · doi:10.1140/epjc/s10052-017-5367-7
Abstract
[Abridged] In its standard formulation, the field equations are not invariant under local Lorentz transformations, and thus the theory does not inherit the causal structure of special relativity. A locally Lorentz covariant gravity theory has been devised recently, and this local causality problem has been overcome. The nonlocal question, however, is left open. If gravitation is to be described by this covariant gravity theory there are a number of issues that ought to be examined in its context, including the question as to whether its field equations allow homogeneous Gödel-type solutions, which necessarily leads to violation of causality on nonlocal scale. Here, to look into the potentialities and difficulties of the covariant theories, we examine whether they admit Gödel-type solutions. We take a combination of a perfect fluid with electromagnetic plus a scalar field as source, and determine a general Gödel-type solution, which contains special solutions in which the essential parameter of Gödel-type geometries, , defines any class of homogeneous Gödel-type geometries. We extended to the context of covariant gravity a theorem, which ensures that any perfect-fluid homogeneous Gödel-type solution defines the same set of Gödel tetrads up to a Lorentz transformation. We also shown that the single massless scalar field generates Gödel-type solution with no closed timelike curves. Even though the covariant gravity restores Lorentz covariance of the field equations and the local validity of the causality principle, the bare existence of the Gödel-type solutions makes apparent that the covariant formulation of gravity does not preclude non-local violation of causality in the form of closed timelike curves.
10 pages, V2: Presentation of Sec.2 improved, references added, version published in Eur.Phys.J.C
References in corpus (21)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Dark torsion as the cosmic speed-up
- Einstein's Other Gravity and the Acceleration of the Universe
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Palatini Approach to Modified Gravity: f(R) Theories and Beyond
- Cosmological perturbations in f(T) gravity
- f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
- Generalizations of teleparallel gravity and local Lorentz symmetry
- Good and bad tetrads in f(T) gravity
- Solar system constraints on f(T) gravity
- Degrees of freedom of gravity
- Growth factor in f(T) gravity
- Observational information for f(T) theories and Dark Torsion
- Static Solutions with Spherical Symmetry in f(T) Theories
- Energy conditions bounds on f(T) gravity
- Weak-Field Spherically Symmetric Solutions in gravity
- gravitational baryogenesis
- Gödel-type universes in f(R) gravity
- Remnant Symmetry, Propagation and Evolution in f(T) Gravity
- Gödel-type universes in Palatini f(R) gravity
- Gödel-type universes in f(T) gravity
Cited by in corpus (13)
- Structure formation in gravity and a solution for tension
- Model parameters in the context of late time cosmic acceleration in gravity
- Gödel-type universes in bumblebee gravity
- Growth of matter overdensities in non-minimal torsion-matter coupling theories
- Dynamics in interacting scalar-torsion theory
- Dynamical features of cosmology
- Gödel and Gödel-type solutions in the Palatini gravity theory
- Gödel-type solutions in ) gravity
- A study on causality in theory
- Generalized Hidden Conformal Symmetry in Quadratic Gravity
- Gödel-type solutions in hybrid metric-Palatini gravity
- Reconciling the ACT Preference in Gravity: Inflation and Reheating Constraints
- Parametrized post-Newtonian formalism in higher-order Teleparallel Gravity