Closed time like curve and the energy condition in 2+1 dimensional gravity
arXiv:hep-th/9212078 · doi:10.1016/0370-2693(93)90715-T
Abstract
We consider gravity in 2+1 dimensions in presence of extended stationary sources with rotational symmetry. We prove by direct use of Einstein's equations that if i) the energy momentum tensor satisfies the weak energy condition, ii) the universe is open (conical at space infinity), iii) there are no CTC at space infinity, then there are no CTC at all.
10 pages (REVTEX 3.0), IFUP-60/92
References in corpus (1)
Cited by in corpus (16)
- Energy-Momentum Restrictions on the Creation of Gott Time Machines
- Poincaré gauge theory of gravity
- Solving The N-Body Problem in (2+1)-Gravity
- Gravitating Chern-Simons vortices
- Hollow cosmic string: the general-relativistic hollow cylinder
- Negative Energy Densities in Extended Sources Generating Closed Timelike Curves in General Relativity with and without Torsion
- Chern-Simons Quantization of (2+1)-Anti-De Sitter Gravity on a Torus
- Stationary Solutions and Closed Time-Like Curve in 2+1 Dimensional Gravity
- (2+1)-Gravity Solutions with Spinning Particles
- No Time Machine Construction in Open 2+1 Gravity with Timelike Total Energy Momentum
- Exact Results in Chern-Simons Supergravity
- (2+1)-Gravity on Riemann Surfaces in Conformal Gauge
- Chronology protection in stationary 3D spacetimes
- Effective action of quantum fields in the space-time of a cylindrically symmetric spinning body
- Fermi-Walker gauge in 2+1 dimensional gravity.
- How much energy do closed timelike curves in 2+1 spacetimes need?