Carter spacetime

The Carter spacetime is the standard example of a spacetime that is distinguishing, but not strongly causal, and contains imprisonned curves that are not closed causal curves.

1. History

2. Topology

3. Metrics and coordinates

$$ds^2 = (\cosh(t) - 1)^2 (-dt^2 + dy^2) - 2 dt dy + dz^2$$

The coordinates have the following identifications :

\begin{eqnarray} (t,y,z) \sim (t,y,z+1)\\ (t,y,z) \sim (t, y+1, z+a) \end{eqnarray}

where $a$ is an irrational number between $0$ and $1$ ($a \in (0,1) \cap (\mathbb{R} \setminus \mathbb{Q}$).

4. Tensor quantities

5. Symmetries

6. Stress-energy tensor

7. Curves

8. Equations

9. Causal structure

10. Asymptotic structure

11. Energy conditions

12. Limits and related spacetimes

13. Misc.

Bibliography